CAC-Ausstellung Lüneburg

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Jorogz’ Domino Moonkist erste Ausstellung am 28.08.2011 in der Jüngstenklasse VV1
Richter: Dr. Wilfried Peper

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The RS-68 engine continued burning through the initial four minutes of flight by consuming liquid hydrogen and liquid oxygen.Shortly before the first stage’s burn concluded, having already left the atmosphere, the 47-foot-long nose shroud covering the satellite was jettisoned.The first stage finished its job and separated about 100 nautical miles over the ocean, leaving rocket’s upper stage and cryogenic RL10B-2 powerplant to perform a lengthy firing to achieve an intermediate parking orbit and then a second, brief burn near the western coast of Africa that sent the payload toward an orbit that was targeted to hit 237 nautical miles at perigee, 36,167 nautical miles at apogee and inclined 24 degrees.The payload separated from the launcher just before T+plus 41 minutes while soaring away from the planet over the Indian Ocean.”Now more than ever, our nation depends on our ability to successfully deliver space-based capabilities with 100 percent mission success,” Col. 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WGS 1 entered service last year to cover the vast Pacific Command that stretches from the U.S. western coast all the way to Southeast Asia. The WGS 2 satellite launched earlier this year was placed into operation over the Indian Ocean for use by U.S. Central Command to provide coverage for the warfighters in Afghanistan, Iraq and other parts of Southwest Asia.The new WGS 3 satellite will be positioned above the Eastern Atlantic at an orbital slot of 12 degrees West longitude. Its broad reach will cover U.S. European Command and U.S. Africa Command, plus lend additional support over the Middle East.”WGS 3 is the next step in deploying Wideband Global SATCOM to augment and eventually replace the legacy Defense Satellite Communications System, or DSCS, which has been the Department of Defense’s backbone for satellite communications over the last three decades,” said Col. Bill Harding, vice commander, Military Satellite Communications Systems Wing.”WGS 3 is slated for operations over EUCOM and AFRICOM and will provide an order of magnitude increase in military communications bandwidth for Soldiers, Sailors, Airmen and Marines.”The satellite will be maneuvered into a circular geostationary orbit 22,300 miles above the planet where it can match the Earth’s rotation and appear parked over one area of the globe. On-orbit testing is scheduled to last a few months, enabling the craft to begin full use next April.The WGS spacecraft are constructed around Boeing’s powerhouse 702-model design used by commercial satellite operators. But within the WGS craft are Ka- and X-band military communications packages.The WGS craft offer X-band communications, like the venerable DSCS satellites, to connect with military users anywhere within the field of view from orbit. What’s new on WGS is Ka-band communications. Officials describe the extra frequency as a way of serving up large amounts of information for reception by U.S. and allied forces across a wide area using the so-called Global Broadcast System, or GBS.”The GBS is like DirecTV to the warfighter. With the emerging requirements for more and more Predator and Reaper unmanned aerial system data, the GBS is allowing us to double the amount of full motion video we are able to carry,” Harding said. “With the GBS data, it allows us to bring that full motion video down to small, one-meter terminals.”The satellites also adjust and shift their multiple beams of coverage, a feature that is employed as local hotspots on Earth move.”That is a key advance for our warfighters of giving them the communications where they need it, when they need it,” said Mark Spiwak, the WGS program director for satellite-builder Boeing.”We can make (the beams) more oblong, we can put notches in them, we can make them bigger and global. But we can shape the beams and shape the throughput.”The Air Force says nine DSCS satellites remain in use while the new WGS craft are continuing to be built and deployed.”We’re trying to squeeze as much as capability out of the DSCS birds as we possible can. We continue to monitor the capability of the spacecraft and how much fuel in there,” Harding said.With the first two WGS satellites already in use and the third en route, the Air Force seems pleased with the new constellation of spacecraft they are assembling.”We’re getting great feedback in terms of the support they are providing,” Harding said. “The first one went up over (Pacific Command). As you realize, that particular theater deals with the tyranny of distance a lot more than some of the other theaters, so (satellite communications) is extremely important to them. Of course, the X-band — the DSCS replacement capability — plus the Ka-band provide them not only a lot of bandwidth…but a lot more coverage area. So there’s a lot of antennas and we’re able to cover forces no matter where they are in the Pacific.”"Quality-of-life for the folks on the ships has been significantly increased due to WGS being fielded,” Spiwak added, noting that WGS 1 can provide 24/7 Internet and television to the military deployed across the Pacific.Three more WGS satellites are under construction at Boeing’s manufacturing plant in El Segundo, California. They are incorporating a slight upgrade from the previous trio of spacecraft and should be ready to begin launching in 2011.”We are very active on satellites 4, 5 and 6. In fact, before the end of the year we will be assembling the F4 satellite into a complete satellite,” Spiwak said.”Those satellites are on schedule…we’ve got the formula now.”Harding said the WGS program — and its six satellites ordered thus far — is valued at $2.1 billion.”WGS addresses our military’s ever-growing appetite for high-bandwidth satellite communications,” said Craig Cooning, vice president and general manager at Boeing Space and Intelligence Systems. “We’re now working with the Air Force to determine how future WGS satellites could be enhanced to handle missions involving airborne intelligence, surveillance and reconnaissance, and communications-on-the-move.”Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA’s first new human spacecraft developed since the space shuttle a quarter-century earlier. The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.New era of rocket launches begins at California baseSPACEFLIGHT NOW

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Between January 1960 and December 1965, 35 Delta missions were launched from SLC-17 facilities.In the spring of 1965, the Air Force transferred SLC-17 and other Thor-related facilities to NASA seeing no further military use for Thor facilities at the Cape. However, following the Challenger accident in January 1986, military and commercial launch services shifted back to expendable launch vehicles. In response, Boeing built a new generation of launch vehicle, Delta 2, to meet the growing military and commercial space launch requirements.The Air Force eventually transferred all of its new NAVSTAR 2 Global Positioning System (GPS) payloads from the Space Shuttle to Delta 2. Civilian customers also began signing up for launches on Delta 2. Launch Complex 17 was chosen as the launch site for the Delta 2, and transfer of responsibility for SLC-17 from NASA back to the Air Force was completed in October 1988.SLC-17 underwent major modifications to support the larger Delta 2. Structural changes included the installation of new platforms and a hydraulic lifting system, as well as a liquid hydrogen storage and supply system. A major reconstruction effort raised the complex’s mobile service tower 10 feet to accommodate the taller launch vehicle. The Air Force launched the first Delta 2 from Pad 17A in February 1989. Work on Launch Complex 17 continued, and the first commercial Delta mission was launched from Pad 17B in August 1989. Since then, SLC-17 has supported more than 50 commercial, Air Force, and NASA launches.To meet the changing needs of its customers, Boeing developed the Delta 3 with twice the payload of Delta 2. The Delta 2 and Delta 3 share SLC 17B, and modifications to that pad to accommodate both vehicles were completed in October 1997.Because the blockhouse on Complex 17 was considered inadequate for Delta 3’s heavier launches, the Air Force built a new 39,000-square-foot administrative and launch-operations facility, called the 1st Space Launch Squadron Operation Building (1 SLS OB). The new facility, completed in June 1996, is located two miles south of Complex 17 and houses the new “soft blockhouse” or Launch Control Center (LCC).Columbia ReportA reproduction of the official accident investigation report into the loss of the space shuttle Columbia and its crew of seven. Choose your store: - - - Mars PanoramaDISCOUNTED! This 360 degree image was taken by the Mars Pathfinder, which landed on the Red Planet in July 1997. The Sojourner Rover is visible in the image. 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Photo: U.S. Air ForceSpace Launch Complex 2 (SLC-2) at Vandenberg Air Force Base (VAFB), Calif., is the home of west coast launch operations for the Delta 2 expendable launch vehicle. From SLC-2, Boeing launches satellite payloads into polar and near-polar orbits.The base is on a western projection of California’s central coast, midway between San Francisco and San Diego. SLC-2 overlooks the Pacific Ocean and is just northwest of the VAFB airfield.SLC-2 had its beginnings with the Thor intermediate-range ballistic missile, which was the predecessor of the Delta launch vehicle family. 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Credit: ULA videoThe Geosynchronous Space Situational Awareness Program, or GSSAP, launched from Cape Canaveral at 7:28 p.m. EDT en route to operational orbits 22,300 miles above Earth.The GSSAP project was designed in secrecy and only announced to the public by AFSPC commander Gen. William Shelton in February.”It’s time to stipulate that we’ve got a critical dependence on space. I would challenge…each of you to bring me an example of a miliary operation that doesn’t somehow involve space. That’s from humanitarian relief operations all the way up through major combat,” said Shelton.It’s that overarching dependence on space that has spurred the U.S. military to ramp up its surveillance on man-made objects and threats in orbit.Some 170 countries now have at least one satellite of their own and 11 nations have the capability to launch a spacecraft into orbit, Shelton said, adding that with space launch also comes missile technology and the potential for anti-satellite shootdowns.The Chinese carried out a dramatic kinetic-energy anti-satellite demonstration in 2007, blasting one of its own orbiting spacecraft with a missile, drawing international condemnation. “And then there are the overt threats, anything from jamming, which is actually mission affecting, obviously, all the way up through high powered laser activity that’s coming along, to kinetic ASAT (anti-satellite) activity. Threats to our spacecraft that not too many years ago we didn’t have to concern ourselves with,” Shelton said.Built by Orbital Sciences Corp., the twin GSSAP satellites are small in size and stature with an important mission before them. Fitted with an electro-optical sensors, the craft will drift just above and below the geosynchronous satellite belt 22,300 miles above the Earth.”(They) will drift in probably just below and just above the GEO belt depending on which direction you want to drift and provide that neighborhood watch capability,” Shelton said. Credit: ULAGeosynchronous orbit allows communications, missile launch detection spacecraft and eavesdropping reconnaissance spy satellites to match the Earth’s rotation and appear fixed above one part of the globe.It is a place where some of the most “precious” Air Force satellites reside.”Think about Advanced EHF satellites on orbit,” Shelton said of the nuclear survivable communications spacecraft constellation. “When the chips are down that’s the system the President is going to use to communicate his orders; the President and National Command Authority to communicate orders to deployed forces. One cheap shot against the AEHF constellation would be devastating.”There’s also the Space Based Infrared System, or SBIRS, that monitors the world on the lookout for enemy missile launches to sound the alarm to friendly countries.”One cheap shot creates a hole in our environment,” Shelton said.”SBIRS is great. We can tell you anytime a missile has launched on the planet, we can tell you where it launched from, we can tell you the type of missile it is, we can tell you the impact point. It’s what the President uses to determine his response options; and in the situation of the United States under attack, deciding what to do and when to do it.”We can’t afford to be down Advanced EHF; down SBIRS.”That’s where GSSAP will help close the surveillance gap on what’s happening 22,300 miles up.”Our decision to declassify this program was simple. We need to monitor what happens 22,000 miles above the Earth, and we want to make sure that everyone knows we can do so,” said Douglas Loverro, deputy assistant secretary of defense for space policy, at the Department of Defense..”We believe that such efforts add immeasurably to both the safety of spaceflight and the stability that derives from the ability to attribute actions — to the benefit of all space-faring nations and all who rely on space-based services.”"If we’re going to be a global power, we want global coverage, we want global access and we want it at a time and a place of our choosing,” Shelton said of space situational awareness.Two more GSSAP satellites are due to launch in 2016 aboard an Atlas 5 rocket.”GSSAP will present a significant improvement in space object surveillance, not only for better collision avoidance, but also for detecting threats,” Shelton said. “GSSAP will bolster our ability to discern when adversaries attempt to avoid detection and to discover capabilities they may have, which might be harmful to our critical assets at these higher altitudes.” Credit: USAFShelton said the Air Force tracks about 23,000 objects routinely on a daily basis. “There are some 500,000 objects in space, so a big traffic management problem and a big threat to fragile spacecraft,” he said.The GSSAP satellites will be operated by the 1st Space Operations Squadron at Shriever Air Force Base in Colorado. “GSSAP will not replace the capabilities that the 1st SOPS currently operates,” said Brig. Gen. David Buck, AFSPC director of Air, Space and Cyberspace Operations. “SBSS and ATRR operate in low-earth orbits and have different capabilities. GSSAP will be placed in a near-geosynchronous orbit at approximately 22,300 miles above the Earth. It will have a very distinct vantage point in relation to the objects it will be observing in geosynchronous orbit. With GSSAP, we will actually be able to characterize an object to a very discriminate level, not just track it.”Launching below the GSSAP spacecraft aboard the Delta 4 rocket was ANGELS, a microsatellite from the Air Force Research Laboratory to test autopilot space situational awareness in geosynchronous orbit. Credit: USAFThe Automated Navigation and Guidance Experiment for Local Space, or ANGELS, will fly above the GPS constellation but use those positioning signals to demonstrate maneuverability around the spent Delta 4 upper stage.”The ANGELS spacecraft hosts a (space situational awareness) sensor payload to evaluate techniques for detection, tracking and characterizing of space objects, as well as, attribution of actions in space,” according to the AFRL fact sheet.Additional payloads on ANGELS will assist operations using a GPS for geosynchronous orbit and high performance accelerometers.”The GPS system uses advanced algorithms from NASA to receive GPS side lobe signals and generate near continuous navigation solutions. The high performance accelerometers precisely measure small spacecraft accelerations for enhanced guidance and navigation,” the fact sheet said.”The experimental onboard vehicle safety system explores methods for dramatically reducing the probability of collision with other space objects in an increasingly congested space environment.”Orbital Sciences also built ANGELS under a $29.5 million deal signed in November 2007. Credit: USAF”The ANGELS program will develop key technologies and capabilities for a broad spectrum of defense and civilian space missions,” Antonio Elias, Orbital’s executive vice president and general manager of its Advanced Programs Group, said at the time. “Under AFRL’s leadership, this effort will help maintain the United States’ continuing technological and industrial superiority in space.”The mission is scheduled to last one year.”As other nations show their commitment to invest in systems capable of harming our satellites, we are committed to investing in space surveillance assets like GSSAP that will directly enable safe operations, protect our spacecraft and indirectly enable a range of decisive responses that will render counter-space threats ineffective,” said Shelton.The launch was the 368th for a Delta rocket, the 27th Delta 4 and the 12th to fly in the Medium+ (4,2) configuration with a pair of strap-on solid motors. For United Launch Alliance, it was the company’s 33rd flight for the Air Force, the 85th launch overall since 2006 and the eighth this year.The next Delta 4 launch is the much-anticipated Heavy with NASA’s Orion capsule on Exploration Flight Test No. 1, set to lift off from Cape Canaveral on Dec. 4.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is now available in our store. Get this piece of history!STS-134 PatchFree shipping to U.S. addresses!The final planned flight of space shuttle Endeavour is symbolized in the official embroidered crew patch for STS-134. Available in our store!Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Project OrionThe Orion crew exploration vehicle is NASA’s first new human spacecraft developed since the space shuttle a quarter-century earlier. The capsule is one of the key elements of returning astronauts to the Moon.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Space Tracking and Surveillance SystemMISSILE DEFENSE AGENCY FACT SHEET An artist’s concept depicts two Space Tracking and Surveillance System (STSS) satellites. Credit: Northrop Grumman The Missile Defense Agency is pursuing the Space Tracking and Surveillance System (STSS) program as a space-based sensor component of the Ballistic Missile Defense System (BMDS). Using sensors capable of detecting visible and infrared light, the Space Tracking and Surveillance System constellation of satellites will become part of a collection of land-, sea-, air-, and space-based BMDS sensors.OverviewTwo research and development satellites will be launched into low earth orbit in 2009.A ground segment has been developed to operate the satellites and provide an interface to the BMDS.The STSS Demonstration Program will demonstrate the key functions of a space-based sensor, passing missile tracking data to missile defense interceptors with the accuracy and timeliness necessary to enable them to successfully intercept missile targets.Lessons learned from the on-orbit operation of the demonstration satellites will provide a foundation to proceed with the fielding of an operational constellation.Initial ProgramThe demonstration satellites have completed buildup, integration, systems testing, and environmental testing, and are in final prelaunch preparation.Two satellites will be launched together on a single Delta 2 launch vehicle in 2009.The STSS ground station is currently functional and is being used to train and certify operators. The ground segment will communicate with the BMDS Command and Control, Battle Management and Communication system.The STSS will perform on-orbit testing of sensor performance against ground targets, airborne targets and short and long range ballistic missile targets.The demonstration satellites are expected to be available for two to four years after launch. Next StepsThe Missile Defense Agency will use early on-orbit testing of the Demonstration Program satellites to refine software and processes to enhance the usefulness of the demonstration satellites.On-orbit satellites will test and demonstrate key knowledge areas in 2009/2010:Birth-to-death tracking of strategic and tactical missiles.Ability to hand-off timely midcourse track data to the BMDS kill chain.Integrated space-based tracking in support of missile defense.Upgrading ground station and spacecraft software will improve the demonstration satellites and reduce risk for future satellite development. John Glenn Mission PatchFree shipping to U.S. addresses!The historic first orbital flight by an American is marked by this commemorative patch for John Glenn and Friendship 7.Final Shuttle Mission PatchFree shipping to U.S. addresses!The crew emblem for the final space shuttle mission is available in our store. Get this piece of history!Celebrate the shuttle programFree shipping to U.S. addresses!This special commemorative patch marks the retirement of NASA’s Space Shuttle Program. Available in our store!Anniversary Shuttle PatchFree shipping to U.S. addresses!This embroidered patch commemorates the 30th anniversary of the Space Shuttle Program. The design features the space shuttle Columbia’s historic maiden flight of April 12, 1981.Mercury anniversaryFree shipping to U.S. addresses!Celebrate the 50th anniversary of Alan Shephard’s historic Mercury mission with this collectors’ item, the official commemorative embroidered patch.Fallen Heroes Patch CollectionThe official patches from Apollo 1, the shuttle Challenger and Columbia crews are available in the store. | | | | 2014 Spaceflight Now Inc.Spacecraft launched to observe cataclysmic blasts BY WILLIAM HARWOOD

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Data will be relayed back to Earth by Cassini, which will be flying past at the same time.The density of Titan’s atmosphere, however, is a critical factor in the Huygens’ descent. The probe is scheduled to be released from Cassini on Christmas Eve and depending on what today’s TA flyby data show, engineers could elect to make slight changes to its trajectory.The data were considered so vital that engineers programmed playback through two DSN ground stations to ensure successful capture.Along with characterizing the moon’s atmosphere, Cassini also was programmed to photograph the Huygens landing site at a resolution of .62 miles per pixel, hopefully providing insights into what the probe can expect when it reaches the surface in January.Cassini braked into orbit around Saturn the night of June 30, firing its main engine for a nerve-wracking 96.4 minutes. Another long rocket firing in late August raised the low point of Cassini’s orbit and set the stage for an extended voyage of discovery.Equipped with state-of-the-art telescopes, an imaging radar system and a battery of other powerful instruments, Cassini will spend at least four years orbiting the sixth planet from the sun, studying its rings in unprecedented detail, making high-resolution movies of its windy atmosphere, charting its magnetic field and mapping a host of icy moons.Titan will get special treatment. Bigger than Mercury and Pluto, Titan is the only moon in the solar system with a thick atmosphere, one in which hydrocarbons fall as rain and liquid ethane pools on its ultra-cold surface. Or so astronomers believe.TITAN FACTS AND FIGURES Discovered by………..Christiaan Huygens, 1655Mass (Earth=1)……….0.02259Radius………………1,600 milesDiameter…………….3,200 milesDistance from Saturn….745,000 milesRotation period………15.94 daysOrbital period……….15.94 daysOrbital inclination…..0.33 degreesAtmospheric pressure….1.6 times Earth’sTemperature………….-290 FahrenheitDaylight at surface…..1/1000 the intensity of sunlight on EarthIn a pre-launch news conference seven years ago, Jonathan Lunine, a University of Arizona physicist and a member of the Cassini science team, provided an educated guess about what today’s flyby and the Huygens probe might reveal.”Imagine a world that’s smaller than Mars and bigger than the planet Mercury, where the air is four times denser at its surface than the air in this room and the surface pressure is about the same as you’d experience at the bottom of a neighborhood swimming pool,” he said. “On that world, the distant sun is never seen and at high noon, things are no brighter than a partly moonlit night on the Earth.”Because of its great distance, the cold is so enormous that water is always frozen out of the atmosphere. Nitrogen is nearly so, but not quite. And the simplest organic molecule, methane, is there to take the place of water as a cloud former, possibly a rain maker and maybe even the stuff of lakes or seas of hydrocarbons.”The methane is lofted hundreds of miles above the surface of this world,” Lunine said before Cassini’s launch in 1997. “It’s cracked open by sunlight and cosmic rays and a menagerie of more complicated organics is produced from the methane and these then float down to the surface to accumulate over time, perhaps to depths of hundreds of meters or more. Volcanism and impacts shape the surface and provide energy to make ever more complex organic molecules in a planet-wide tapestry that is an organic chemist’s dream.”What I have described to you is Titan, the second largest moon in the solar system, nearly the largest. It was partly revealed to us by Voyager 1 in 1980. Through its many instruments, Voyager discovered and characterized a dense atmosphere around this cold world. Yet … Voyager’s cameras could not penetrate the organic haze and so we still do not know what awaits Cassini-Huygens at the end of its journey.”But in the years since Cassini’s launch, optical and radar observations from Earth have given scientists at least a hint of what the spacecraft might find. Scientists are convinced lakes or small oceans of liquid hydrocarbons exist on Titan, but not a globe-spanning sea. One way or the other, Cassini and Huygens should resolve the matter.”Titan is almost certainly not the home of life today,” Lunine said. “But the organic chemical cycles that go on may constitute a chemical laboratory for replaying some of the steps that led to life on Earth. Titan is in some ways the closest analogue we have to the Earth’s environment before life began and this makes Titan very important.”Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Cassini getting ever closer to colorful Saturn CICLOPS/SPACE SCIENCE NEWS RELEASEPosted: June 3, 2004As Cassini coasts into the final month of its nearly seven-year trek, the serene majesty of its destination looms ahead. The spacecraft’s cameras are functioning beautifully and continue to return stunning views from Cassini’s position, 1.2 billion kilometers (750 million miles) from Earth and now 15.7 million kilometers (9.8 million miles) from Saturn. Credit: NASA/JPL/Space Science InstituteDownload larger image version In this narrow angle camera image from May 21, 2004, the ringed planet displays subtle, multi-hued atmospheric bands, colored by yet undetermined compounds. Cassini mission scientists hope to determine the exact composition of this material. This image also offers a preview of the detailed survey Cassini will conduct on the planet’s dazzling rings. Slight differences in color denote both differences in ring particle composition and light scattering properties. Images taken through blue, green and red filters were combined to create this natural color view. The image scale is 132 kilometers (82 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colorado. 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Both programs were to be built around the same Mariner Mark II spacecraft design to minimize costs. CRAF, or the Comet Rendezvous and Flyby Mission, was to do what its name suggested. Cassini was to explore Saturn. But the CRAF mission was cancelled in 1992 and a few months later, new NASA Administrator Daniel Goldin, author of what would become known as the “faster, better, cheaper” mission design philosophy, threatened to cancel Cassini as well, deriding the expensive spacecraft as a “Battlestar Galactica.” Cassini lifts off from Cape Canaveral atop a Titan 4B rocket. Credit: NASA-KSC”With many countries participating in this great mission, none of us could imagine Goldin taking this drastic step and damaging our country’s relationship with the Europeans,” wrote former Cassini mission manager Charles Kohlhase in an article for The Planetary Society. “To our joy, on June 14, 1994, Jean-Marie Luton (then director general of ESA) sent a powerful letter to Vice President Al Gore, with copies to the U.S. secretary of state, key office directors, and of course Dan Goldin.” The letter concluded with a paragraph that Kohlhase said saved Cassini from the budget axe: “Europe therefore views any prospect of a unilateral withdrawal from the cooperation on the part of the United States as totally unacceptable. Such an action would call into question the reliability of the U.S. as a partner in any future major scientific and technological cooperation.” European participation in upcoming NASA projects, including the agency’s flagship international space station program, was considered crucial and in the end, the Cassini project survived. When all was said and done, NASA spent $2.6 billion on the project, the European Space Agency spent $500 million and the Italian Space Agency chipped in $160 million for a total cost of about $3.26 billion. Getting to Saturn took almost as much time as it took to get the project approved and launched: 6.7 years. Because NASA did not have a rocket capable of boosting the heavyweight Cassini directly to Saturn, the spacecraft was forced to take a convoluted route, using the gravity of Venus, Earth and Jupiter to build up the velocity necessary to reach its target. The Centaur upper stage of the U.S. Air Force Titan 4B rocket that launched Cassini on Oct. 15, 1997, was used to slow the craft down so it could fall into the inner solar system. After flying by Venus on April 26, 1998, and again on June 24, 1999, Cassini streaked past Earth at an altitude of just 727 miles or so on Aug. 18, 1999. From there, the spacecraft headed for Jupiter and a final velocity boosting flyby on Dec. 30, 2000. This graphic illustrates Cassini’s long trek to Saturn. Credit: NASA/JPLWhile Cassini’s primary mission is to last four years, it has enough power and propellant to last many years beyond, should NASA choose to fund additional mission support. “We’re long overdue for a visit to the lord of the rings,” said Orlando Figueroa, director of solar system exploration at NASA headquarters. “We’re looking forward to significant science coming out of the mission and we intend to keep it alive for as long as we can. This is a flagship mission of incredible importance to solar system exploration.” Throughout its seven-year voyage to Saturn, Cassini has operated in near flawless fashion. Aside from the issue with the receiver needed to collect data from Huygens, engineers have encountered only four other problems of any significance. For reasons still not fully understood, the optics in Cassini’s narrow-angle camera clouded up after launch, producing blurry images. But by warming the optics in a carefully controlled fashion, engineers were able to clear up the problem “to the point where we think it is at least as good as it ever was before,” said program manager Bob Mitchell. Another problem involved a radio science experiment, one unrelated to the issue with the Huygens probe. A component in a Ka-band radio failed well into the mission, resulting in a loss of sensitivity for certain gravitational wave studies. Part of that research was completed before the failure and other aspects of the experiment can be conducted as originally planned. The overall impact, Mitchell said, was minimal. A third problem is a large leak in the main helium regulator used to pressurize Cassini’s propulsion system for major rocket firings. Engineers believe foreign object debris, possibly from an explosive pyrotechnic device, which was fired shortly after launch to activate the system, lodged in the regulator, preventing a valve from seating fully. Helium is used to push propellants through Cassini’s plumbing and into the main engine’s combustion chamber at a constant pressure. The regulator controls that pressurization, which is needed for long firings like the upcoming Saturn Orbit Insertion burn. In this case, Cassini’s complexity and built-in redundancy came to the rescue. By delaying the opening of a downstream latch valve to just 70 seconds or so before main engine ignition, engineers were able to work around the regulator issue with no impact to mission operations. The procedure was used for a major 88-minute Deep Space Maneuver rocket firing back in 1998 and again in late May for a six-minute burn to fine-tune the Phoebe flyby trajectory. No one expects any problems for the Saturn Orbit Insertion burn. An artist’s concept of Cassini performing an engine firing. Credit: NASA/JPLThe fourth problem, and one that has at least some potential for downstream impact to normal operations, involves Cassini’s stabilizing reaction wheels. By controlling the spin of three such wheels, oriented 120 degrees apart, flight engineers can re-orient Cassini or keep it rigidly locked on target, reducing the spacecraft’s motion to 10 times less than the movement of a clock’s hour hand. A fourth wheel can be moved into position to take over in case of problems with any one of the other three. Two years ago, engineers noticed “some chatter, some vibration” in the bearings of reaction wheel No. 3. It’s a phenomenon known as cage instability, “kind of like a rattling ball bearing in your axle bearings of your car,” said Julie Webster, lead spacecraft engineer. To be on the safe side, wheel No. 4, the spare, was spun up and No. 3 was moved into the backup position. “So now we’re operating on wheels 1, 2 and 4 and they’re operating just fine,” Mitchell said. But friction levels also are increasing, albeit very slowly, in the other wheels. “We think it’s probably pretty normal, standard behavior,” Mitchell said. “We have talked to some projects … that have used wheels like this, or similar to this, and none of them has seen this kind of a problem. But none of them had the level of instrumentation that we’ve got, either. So we suspect they probably had exactly the same phenomena occurring and they just didn’t see it.” Engineers have analyzed the telemetry from the three operating wheels and “we have extrapolated it out to well beyond end of mission and it doesn’t get even close to what the torque threshold is for our ability to spin these things,” Mitchell said. “But it’s something that we’re keeping an eye on.”MISSION PREVIEWFallen Heroes special patchThis special 12-inch embroidered patch commemorates the U.S. astronauts who made the ultimate sacrifice, honoring the crews of Apollo 1, Challenger and Columbia.Choose your store: - - - Moon RushThis book examines how the exploration of space, specifically a commercial base on the Moon and Mars would transform our economies on the Earth as surely as the discovery of the New World transformed the old world of Europe.Choose your store: - - - Apollo 11 special patchSpecial collectors’ patch marking the 35th anniversary of the historic Apollo 11 moon landing is now available.Choose your store: - - - Get inside Apollo!Full color drawings reveal like never before the details of the Apollo Command and Service Modules.Choose your store: - - - | | | | 2014 Spaceflight Now Inc.Follow the Huygens probe’s descent to the surface of Saturn’s moon Titan! Reload this page for the latest on the mission.SATURDAY, JANUARY 15, 2005A missing computer command - apparently the result of human error - caused the loss of half the pictures taken by Europe’s Huygens probe as it descended to the surface of Saturn’s moon Titan. But project officials said today the 350 pictures that made it back, along with high-quality data fromthe spacecraft’s other instruments and unexpected measurements by Earth-based radio telescopes, should fulfill all of the mission’s primary objectives.Read our .Also, you can see our montage of Huygens pictures showing the landing area .Video coverage for subscribers only:VIDEO:THE NEW PICTURES PRESENTED WITH EXPERT NARRATION VIDEO:LISTEN TO SOUNDS FROM HUYGENS WITH NARRATION AUDIO:LISTEN TO SOUNDS FROM HUYGENS WITH NARRATION VIDEO:RESULTS FROM HUYGENS’ SURFACE SCIENCE PACKAGE VIDEO:CHIEF SCIENTIST EXPLAINS COMMUNICATIONS ERROR VIDEO:TODAY’S PHOTO AND SCIENCE BRIEFING AUDIO:TODAY’S PHOTO AND SCIENCE BRIEFING 2015 GMT (3:15 p.m. EST)Here is a press statement from Lockheed Martin:”After over seven years in space, the European Space Agency’s (ESA) Huygens probe has descended through the atmosphere of Titan, the largest of Saturn’s multitude of moons.”Pictures of Titan’s exotic environment were provided by the Descent Imager/ Spectral Radiometer (DISR), a complex instrument designed and built by Lockheed Martin for the University of Arizona and the NASA Jet Propulsion Laboratory (JPL). NASA’s Cassini spacecraft, with the Huygens probe in tow, was inserted into orbit around Saturn on June 30, 2004, initiating four years of orbital science investigations of the giant ringed planet and its many mysterious moons.”We couldn’t be more pleased for our colleagues at the University of Arizona, NASA and ESA as Huygens has allowed us unprecedented access to one of the most mysterious moons in the solar system,’ said James Crocker, vice president, Civil Space, at Lockheed Martin Space Systems Company. ‘The superb performance of the DISR hardware and the many years of hard work by the DISR team are equally gratifying, and we’re proud to play a role in this exciting international voyage of exploration.’”As Huygens descended by parachute through Titan’s thick atmosphere, DISR made a range of imaging and spectral observations using several sensors and fields of view. The radiation balance of the atmosphere was measured by monitoring the upward and downward flow of radiation. A calculation of the size, number and density of suspended particles in the atmosphere was made possible by measuring the light intensity around the Sun. Two imagers (one visible, one infrared) observed the surface during the latter stages of the descent, and built up a mosaic of pictures around the touch down site. A side-view visible imager captured a horizontal view of the horizon and the underside of the cloud deck. The spectral measurements of the surface were enabled by a lamp that switched on shortly before touch down to augment the weak sunlight.”The study of Titan, Saturn’s largest moon, is one of the major goals of the Cassini/Huygens mission. Although it is believed to be too cold to support life, haze-covered Titan may preserve, in deep-freeze, many of the same chemical compounds that preceded life on Earth. The Huygens descent and touch down is the most distant descent by a robotic probe ever attempted on another object in the solar system. Over the course of the orbital mission, Cassini will have executed 45 flybys of Titan, coming as close as approximately 590 miles (950 km) above the surface.”This will permit high-resolution mapping of the moon’s surface with an imaging radar instrument, which can see through the opaque haze of Titan’s upper atmosphere.”The second largest planet in our solar system, after Jupiter, Saturn serves as a natural laboratory to better understand the formation of our Solar System five billion years ago, as the planet and its rings are a close analog to the disc of gas and dust surrounding the nascent Sun that formed the planets. Detailed knowledge of the dynamics of interactions among Saturn’s elaborate rings and numerous moons will provide valuable data for understanding how each of the solar system’s planets evolved.”The Cassini spacecraft was launched on a Lockheed Martin-built Air Force Titan IV/Centaur rocket Oct. 15, 1997. The Cassini propulsion module - also built by Lockheed Martin - is the largest U.S. planetary spacecraft propulsion system ever built, and was fired 17 times en route to Saturn, and will be ignited approximately 150 more times before the end of the mission. In addition to DISR, the Titan IV/Centaur and the propulsion system, Lockheed Martin Space Systems Company designed and built the three radioisotope thermoelectric generators (RTGs) that power spacecraft systems.”JPL designed, developed and assembled the Cassini orbiter. ESA managed the development of Huygens and is in charge of operations of the probe from its control center in Darmstadt, Germany. The Italian Space Agency provided the high-gain antenna, much of the radio system and elements of several of Cassini’s science instruments. JPL manages the overall program for NASA’s Office of Space Science, Washington, D.C.”1135 GMT (6:35 a.m. EST)Tired and weary after a sleepless night spent sorting through their data, scientists today unveiled more pictures returned from the European Space Agency’s Huygens probe that landed on Saturn’s moon Titan Friday.PHOTO: PHOTO: PHOTO: PHOTO: 1040 GMT (5:40 a.m. EST)An apparently missing command caused the loss of Huygens’ Channel A data stream during descent to Titan yesterday, prompting ESA to form an investigation into the error. The Channel B data link worked, allowing over 300 pictures and information from the probe’s instruments to be relayed up to the Cassini orbiter. With two data paths, scientists had their choice of either relaying the same set of pictures to Cassini twice for redundancy or taking two sets of pictures to maximize the potential number of images. They opted to acquire two sets of pictures, and the lack of Channel A caused half of the expected number of pictures from Huygens to be lost. The Channel A problem also resulted in the loss of data for the Doppler wind experiment between Huygens and Cassini. But ESA’s chief scientist says data from radio telescopes on Earth that were listening to the tones from Huygens should allow researchers to complete the winds experiment. FRIDAY, JANUARY 14, 2005Initial pictures of Saturn’s moon Titan snapped by Europe’s Huygens probe during its historic atmospheric descent and touchdown today show an active world likely carved by the flow of cryogenic liquids that may still pool on its frigid surface, a leading planetary scientist says.Read our .Video coverage for subscribers only:VIDEO:THE FIRST PICTURE FROM HUYGENS IS REVEALED VIDEO:OFFICIALS OFFER THOUGHTS AFTER SEEING PICTURE VIDEO:HUYGENS POST-LANDING BRIEFING AUDIO:HUYGENS POST-LANDING BRIEFING VIDEO:STATUS REPORT DURING DESCENT AUDIO:MISSION STATUS REPORT DURING DESCENT VIDEO:HUYGENS PRE-ARRIVAL NEWS BRIEFING AUDIO:HUYGENS PRE-ARRIVAL NEWS BRIEFING VIDEO:OVERVIEW OF HUYGENS PROBE’S SCIENCE OBJECTIVES VIDEO:JULY NEWS BRIEFING ON CASSINI’S PICTURES OF TITAN VIDEO:PICTURES SHOWING TITAN SURFACE FROM OCT. FLYBY VIDEO:WHAT’S KNOWN ABOUT TITAN BEFORE THE FIRST FLYBY VIDEO:NARRATED MOVIE OF CLOUDS MOVING NEAR SOUTH POLE VIDEO:OCT. BRIEFING ON RADAR IMAGES OF TITAN SURFACE 2225 GMT (5:25 p.m. EST)ESA has not released any additional pictures. Another report is scheduled for 1000 GMT (5 a.m. EST) on Saturday.2129 GMT (4:29 p.m. EST)The European Space Agency unveiled the first raw images from the Huygens Titan probe today, black-and-white pictures showing ice blocks strewn across the surface and hard-to-interpret features resembling drainage channels and, possibly, a frigid shoreline of sorts.Read our .2043 GMT (3:43 p.m. EST)An extraordinary raw picture returned from Huygens shows the view from Titan’s surface. You can see the picture .2005 GMT (3:05 p.m. EST)There was just one picture released so far. European Space Agency plans to unveil more photos about two hours from now.2002 GMT (3:02 p.m. EST)You can see the first picture . It was taken at an altitude of 16 km as Huygens made its descent.1956 GMT (2:56 p.m. EST)The first image shows what appear to be drainage channels flowing to a possible shoreline, the camera’s scientist says. The pictures are raw and unprocessed.1955 GMT (2:55 p.m. EST)The first picture from the descending Huygens probe showing the Titan surface has been revealed in mission control!1930 GMT (2:30 p.m. EST)ESA has released some quote by various officials following today’s landing on Titan:”This is a great achievement for Europe and its U.S. partners in this ambitious international endeavour to explore the Saturnian system,” said Jean-Jacques Dordain, ESA’s director general. “Titan was always the target in the Saturn system where the need for ‘ground truth’ from a probe was critical. It is a fascinating world and we are now eagerly awaiting the scientific results,” says Professor David Southwood, director of ESA’s scientific program. “The Huygens scientists are all delighted. This was worth the long wait,” says Dr Jean-Pierre Lebreton, ESA Huygens mission manager. Huygens is expected to provide the first direct and detailed sampling of Titan’s atmospheric chemistry and the first photographs of its hidden surface, and will supply a detailed ‘weather report.’One of the main reasons for sending Huygens to Titan is that its nitrogen atmosphere, rich in methane, and its surface may contain many chemicals of the kind that existed on the young Earth. Combined with the Cassini observations, Huygens will afford an unprecedented view of Saturn’s mysterious moon. “Descending through Titan was a once-in-a-lifetime opportunity and today’s achievement proves that our partnership with ESA was an excellent one,” says Alphonso Diaz, NASA associate administrator of science. “The teamwork in Europe and the USA, between scientists, industry and agencies has been extraordinary and has set the foundation for today’s enormous success,” concludes Jean-Jacques Dordain. 1800 GMT (1:00 p.m. EST)Robert Mitchell, NASA’s Cassini program manager at the Jet Propulsion Laboratory in Pasadena, Calif., says the loss of one telemetry stream from the Huygens Titan probe appears to be the result of an actual problem of some sort on board the spacecraft.Read our .1745 GMT (12:45 p.m. EST)There will be a pause in live reports from ESA while the rest of the data is downlinked from Cassini and scientists have a chance to begin examining the mounds of information. The next event is expected after 1945 GMT (2:45 p.m. EST) with some initial science news, potentially the first pictures from Huygens. We’ll be posting them here as soon as they are released.1722 GMT (12:22 p.m. EST)NASA’s Cassini Saturn orbiter began downlinking science data from the European Space Agency’s Huygens probe at 11:19 a.m. EST (1619 GMT), confirming the spacecraft not only survived its high-speed plunge into the atmosphere of Saturn’s moon, Titan, but that its instruments worked to remotely explore one of the strangest worlds in the solar system.Read our .1706 GMT (12:06 p.m. EST)Engineers says the Channel A and Channel B data paths from Huygens are redundant with the exception that Channel A is needed for the Doppler wind experiment with the Cassini orbiter. The Channel A telemetry stream isn’t working as expected, but Channel B appears normal, ESA says.1701 GMT (12:01 p.m. EST)The temperature inside the probe was 25 degrees C as it was descending through 50 km altitude, the ongoing data review shows. 1658 GMT (11:58 a.m. EST)The probe went through the entry phase, the parachute deployment was within 15 seconds of the planned time and onboard accelerometer data worked normally, officials are saying at the news conference. The playback of data continues.1655 GMT (11:55 a.m. EST)ESA says data is being received normally on the Channel B telemetry steam. However, the Channel A has a question mark surrounding it.1645 GMT (11:45 a.m. EST)Here is a press statement from Alcatel:”The Huygens space probe has arrived on Titan. The probe was built by prime contractor Alcatel Space, a subsidiary of Alcatel, leading a consortium of 40 companies andlaboratories. Alcatel Space is the first European company to have met thechallenge of constructing a spacecraft designed to resist such draconianconditions. This is the first time that a man-made object has landed on themoon of a planet so far away in our solar system. This is also the firsttime that an European probe has successfully landed on another part of thesolar system.”The interplanetary voyage of Cassini/Huygens took seven years, and made useof successive gravity boosts from Venus (twice), the Earth and Jupiter.Huygens had to stand up to temperatures of 212 deg F near Venus, and made ablind crossing of the asteroid belt between Mars and Jupiter, then therings of Saturn. However, the technical challenge reached its zenith duringthe descent towards Titan, which lasted nearly three weeks after theseparation from the Cassini mother-craft on December 25. Followingaerodynamic braking in the upper atmosphere, then deployment of threeparachutes to control the descent, the probe landed on the surface ofTitan. Huygens is a veritable flying lab, featuring six advancedinstruments to carry out all measurements expected by the scientificcommunity.”Meanwhile, Cassini is in orbit around Saturn for its own observationmission, while relaying data from Huygens back to Earth.”The Cassini/Huygens programs was an unprecedented technical challenge,tackling aspects that had never before been studied:Major restrictions on mass and energy, given the distance to betraveled and the complex trajectory needed to reach Saturn via gravityboosts form Venus, Earth and Jupiter.Completely autonomous operation.High-precision Cassini/Huygens separation maneuvers.Thermal shield adapted to an entry into Titan’s atmosphere.Parachute deployment at supersonic speed.Sufficient robustness to stand up to unknown elements, especiallyatmospheric (furthermore, scientists have continuously changed their modelssince the knowledge of Titan was increased, which required an importanteffort to ensure successful entry).”We are especially proud of this huge success by our customer ESA, inpartnership with NASA and ASI,” said Pascale Sourisse, Chairman and CEO ofAlcatel Space. “Not only is it a world first in exploration of theuniverse, it also marks a major step forward in better understanding theorigins of life. With the Huygens mission now accomplished, we want toreaffirm our unyielding commitment to carrying out the most demandingprograms for interplanetary exploration and observation of the universe,alongside European scientists and space agencies. We hope that this missionwill pave the way to other adventures that prove to be just as exciting,both scientifically and technologically.”1635 GMT (11:35 a.m. EST)The news briefing has begun.”We have a scientific success,” ESA director general Jean-Jacques Dordain reports. “We are the first visitors of Titan.”1630 GMT (11:30 a.m. EST)We’re awaiting the start of a planned news conference. The top science officials from ESA and NASA were in the room and then left.1619 GMT (11:19 a.m. EST)The Huygens data is being received! Applause has erupted in the German control room after the tense and anxious wait. It will take some time to begin examining the information. The first pictures from Huygens could be released later today, if all has gone well. 1605 GMT (11:05 a.m. EST)Scientists, engineers and senior officials have gathered in a large crowd within the European mission control center. Everyone is nervously awaiting the first bits of data from Huygens.1545 GMT (10:45 a.m. EST)NASA’s Cassini Saturn orbiter has turned back toward Earth and started transmitting stored data from Europe’s Huygens probe, which was still broadcasting a faint carrier signal from the surface of the moon Titan more than two hours after touching down and well after Cassini had turned away.Read our .1530 GMT (10:30 a.m. EST)Scientists have another 40 minutes of suspense before the first Huygens data arrives on Earth, which will confirm probe’s transmissions to Cassini and recording aboard the orbiter has worked.1526 GMT (10:26 a.m. EST)The communications link between Cassini and Earth has been established. 1510 GMT (10:10 a.m. EST)”This is clearly an engineering success and we know the probe has been successfully entering the atmosphere, has been descending on the parachute to the surface,” said Jean-Pierre Lebreton, ESA’s Huygens project scientist.”But at this moment we cannot say more. I mean, we have not seen the data. What we have seen is a tone, a signal, which was indicating that the probe was transmitting but we have not seen any real data yet. So I would like to wait a bit more to say whether we have a successful mission or not.”The first Huygens data via the Cassini telemetry playback is expected in about an hour.1501 GMT (10:01 a.m. EST)A tone is still being emitted from Huygens and detected by radio telescopes on Earth, now more than two hours after landing. Meanwhile, Cassini has turned away from Huygens to re-point its communications antenna for relay of data to Earth. 1445 GMT (9:45 a.m. EST)Here is the press statement issued by the European Space Agency:”The Robert C. Byrd Green Bank Telescope (GBT) in West Virginia, USA, a part of the global network of radio telescopes involved in tracking the Huygens Titan probe, has detected the probe’s ‘carrier’ (tone) signal.”The detection occurred between 11:20 and 11:25 CET (5:20-5:25 a.m. EST), shortly after the probe began its parachute descent through Titan’s atmosphere. The extremely feeble signal was first picked up by the Radio Science Receiver supplied by the NASA Jet Propulsion Laboratory. This signal is an important indication that the Huygens probe is ‘alive’. However, it does not contain yet any substance; the latter is expected to come a few hours later via the Cassini spacecraft. “What the Green Bank radio telescope has detected is only a ‘carrier’ signal. It indicates that the back cover of Huygens must have been ejected, the main parachute must have been deployed and that the probe has begun to transmit, in other words, the probe is ‘alive’. This, however, still does not mean that any data have been acquired, nor that they have been received by Cassini. The carrier signal is sent continuously throughout the descent and as such does not contain any scientific data. It is similar to the tone signal heard in a telephone handset once the latter is picked up. “Only after having received the data packets at ESOC will it be possible to say with certainty whether data were properly acquired. The first data set from Cassini will reach ESOC in the afternoon. Additional downlinks will follow throughout the evening and night for redundancy. “Further analysis of the signals will be conducted using other three independent data acquisition systems at the Green Bank Telescope. In addition to the GBT, sixteen other radio telescopes in Australia, China, Japan and the USA are involved in tracking the Huygens probe. “The ultimate goal of the tracking experiment is to reconstruct the probe’s descent trajectory with an unprecedented accuracy of the order of one kilometre. The measurements will be conducted using Very Long Baseline Interferometry (VLBI) and Doppler tracking techniques. This would enable studies of the dynamics of Titan’s atmosphere, which is considered to be a ‘frozen’ copy of that of the early Earth. “The VLBI component of the tracking experiment is coordinated by the Joint Institute for VLBI in Europe (JIVE) and ESA; the Doppler measurements are conducted by the Jet Propulsion Laboratory.”1403 GMT (9:03 a.m. EST)Huygens remains alive and sending its beeping signal from the surface — more than an hour after controllers calculate it landed. The relay of science data to Cassini concludes later this hour as the orbiter goes over the horizon from the landing site.The first science information is expected on Earth about two hours from now.1332 GMT (8:32 a.m. EST)Mission controllers say the tone from Huygens is still being received! The craft appears to have landed around 1245 or 1246 GMT (7:45 or 7:46 a.m. EST) on Titan and continues to operate from the moon’s surface.1300 GMT (8:00 a.m. EST)A huge radio telescope at Green Bank, West Virginia, was able to detect and lock onto a faint carrier signal from the Huygens Titan probe for more than two hours this morning, confirming the spacecraft’s continued descent through the moon’s atmosphere following a high-speed entry.A second radio telescope now has picked up the signal as well and Europoean Space Agency project scientist Jean-Pierre Lebreton said engineers were even able to confirm at least one of the probe’s six on-board instruments had activated as planned.Read our .1115 GMT (6:15 a.m. EST)Huygens should be continuing its long, parachute-aided fall to the surface of Titan, with the large suite of science instruments operating to study the atmosphere and obtain volumes of pictures. Huygens is doing its work out of view from mission control. Real-time confirmation that the science program is being performed is not available because the craft is sending the information directly to the Cassini orbiter, which itself has turned away from Earth to receive the Huygens data.Earlier, controllers heard a simple tone emitted from Huygens that did announce the craft was at least alive.A news conference is coming up at 1230 GMT (7:30 a.m. EST). Cassini will resume communications with Earth about three hours later, and the data playback will continue for several hours.1033 GMT (5:33 a.m. EST)SIGNAL FROM HUYGENS! A radio telescope on Earth has detected a faint signal from the descending Huygens spacecraft, confirming the probe is alive, has survived its super-hot entry into the atmosphere and should be carrying out its scientific exploration on the way to the surface of Saturn’s moon Titan.This is just a signal with no actual data included. The data is being relayed to the Cassini orbit and will be played to Earth later today.Nonetheless, the fact that a signal has been received to verify that Huygens is functioning prompted screams and cheers in mission control.THURSDAY, JANUARY 13, 2005The European Space Agency’s Huygens probe, closing in on Saturn’s mysterious moon Titan, is racing toward a dramatic, high-speed plunge into the moon’s thick nitrogen atmosphere early Friday for a long-awaited parachute descent to an enigmatic surface.Released from NASA’s Cassini Saturn orbiter on Christmas Eve, the flying saucer-shaped probe is targeted to slam into Titan’s atmosphere at a velocity of 12,400 mph at 5:13 a.m. EST (1013 GMT).Over the next three to four minutes, the 705-pound probe is expected to endure peak heating of nearly 3,500 degrees and a braking force of some 16 Gs, slowing the craft to a more sedate 895 mph. At that point - 5:17 a.m. - the probe should release a small 8.5-foot pilot chute that will pull away a protective rear cover.Just 2.5 seconds later, the craft’s 27.2-foot-wide main parachute will unfurl. For the first time since pre-release tests, an on-board radio will begin transmitting data to Cassini around 5:18 a.m. as the NASA spacecraft streaks past Titan some 37,000 miles away.Huygens is expected to reach the surface of Titan around 7:31 a.m. But with its main antenna pointed toward the landing zone, Cassini will be out of contact with Earth, leaving anxious engineers and scientists in the dark until the NASA craft turns back toward Earth and begins transmitting recorded data around 10:17 a.m. That’s nearly three hours after Huygens touches down.Read our .WEDNESDAY, JANUARY 12, 2005In one of the boldest space missions ever attempted, a small European-built probe will slam into the atmosphere of Saturn’s mysterious moon Titan Friday for a two-and-a-half hour parachute descent to its smog-shrouded surface.Beaming pictures and a torrent of data to NASA’s Cassini Saturn orbiter, the flying saucer-shaped Huygens probe will give scientists their first close-up look at one of the largest expanses of unexplored territory in the solar system.Researchers are hopeful Huygens will answer their most pressing questions: whether hydrocarbons fall like rain and form pools of liquid ethane and similar compounds on the moon’s frigid surface; and what erosional or depositional processes are responsible for covering up impact craters and producing a relatively flat, mountain-free surface.No matter what Huygens actually sees on the surface, scientists expect to gain insights into the workings of a thick, complex atmosphere that in some respects mirrors Earth’s shortly after the planet’s birth.Read our .Read our earlier coverage.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Music rings of Saturn CASSINI PHOTO RELEASEPosted: September 29, 2004 Looking something like the fibrous bow of a violin, Saturn’s colorful rings sweep through this spectacular natural color view while two small moons look on. Credit: NASA/JPL/Space Science InstituteDownload larger image version From left, the moons visible here are Janus (181 kilometers, or 112 miles across) and Mimas (398 kilometers, or 247 miles across). Cassini’s view in this image is from beneath the ring plane; the moons are on the far side of Saturn. Janus leads Mimas as the two moons orbit the planet. Nearly the entire ring system can be seen in this view. The diaphanous C ring appears at the upper right, followed by the multi-hued B ring. Next, the famous Cassini division (4,800 kilometers, or 2,980 miles wide) separates the A and B rings. The outer edge of the B ring which forms the inner boundary of the Cassini division is maintained by a gravitational resonance with Mimas. Near the outer edge of the A ring are the Encke Gap (325 kilometers, or 202 miles wide) and the barely visible Keeler Gap (35 kilometers, or 22 miles wide). The faint, thread-like F ring is discernible just beyond the main rings. The image was obtained with the Cassini spacecraft narrow angle camera on August 27, 2004, at a distance of 9.1 million kilometers (5.6 million miles) from Saturn. Images taken with red, green and blue filters were combined to create this color view. The moons have been enhanced in brightness to increase their visibility. The image scale is 54 kilometers (34 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Nature’s canvas at Saturn CASSINI PHOTO RELEASEPosted: November 29, 2004In a splendid portrait created by light and gravity, Saturn’s lonely moon Mimas is seen against the cool, blue-streaked backdrop of Saturn’s northern hemisphere. Delicate shadows cast by the rings arc gracefully across the planet, fading into darkness on Saturn’s night side. Credit: NASA/JPL/Space Science InstituteDownload larger image version The part of the atmosphere seen here appears darker and more bluish than the warm brown and gold hues seen in Cassini images of the southern hemisphere, due to preferential scattering of blue wavelengths by the cloud-free upper atmosphere. The bright blue swath near Mimas (398 kilometers, or 247 miles across) is created by sunlight passing through the Cassini division (4,800 kilometers, or 2,980 miles wide). The rightmost part of this distinctive feature is slightly overexposed and therefore bright white in this image. Shadows of several thin ringlets within the division can be seen here as well. The dark band that stretches across the center of the image is the shadow of Saturn’s B ring, the densest of the main rings. Part of the actual Cassini division appears at the bottom, along with the A ring and the narrow, outer F ring. The A ring is transparent enough that, from this viewing angle, the atmosphere and threadlike shadows cast by the inner C ring are visible through it. Images taken with red, green and blue filters were combined to create this color view. The images were obtained with the Cassini spacecraft narrow angle camera on Nov. 7, 2004, at a distance of 3.7 million kilometers (2.3 million miles) from Saturn. The image scale is 22 kilometers (14 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Cassini posterJust in time for the Cassini spacecraft’s arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12×12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA’s Mars Exploration Rover is now available from the Astronomy Now Store.Apollo 11 special patchSpecial collectors’ patch marking the 35th anniversary of the historic Apollo 11 moon landing is now available.Choose your store: - | | | | 2014 Spaceflight Now Inc.New Cassini picture shows rings in extraordinary detail CASSINI PHOTO RELEASEPosted: December 14, 2004This fantastic close-up of Saturn’s outer C ring shows large and sharp changes in brightness across the rings, owing to the extreme variations in ring particle concentrations at different distances from the planet. The dark gap running through the center contains the Maxwell ringlet, as well as a faint, narrow ringlet discovered in Cassini images. Another very dark region to the right of the Maxwell gap is also a narrow gap. Credit: NASA/JPL/Space Science InstituteDownload larger image version The image was taken in visible light with the Cassini spacecraft narrow angle camera at a distance of about 836,000 kilometers (519,000 miles) from Saturn. The image scale is 4.6 kilometers (2.9 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.New view of Saturn’s rings and moons from Cassini CASSINI PHOTO RELEASEPosted: June 21, 2004 Credit: NASA/JPL/Space Science InstituteDownload larger image version Saturn’s magnificent rings show some of their intricate structure in this image taken on May 11, 2004, by the Cassini spacecraft’s narrow angle camera. Although they appear to be solid structures, the rings are composed of billions of individual particles, each one orbiting the planet on its own path. Satellites visible in this image: Janus (181 kilometers, or 113 miles across) above the rings, and icy Enceladus (499 kilometers, or 310 miles across) below the rings. The F ring shepherd moons Prometheus and Pandora can be seen along Saturn’s outermost F ring if the image is further contrast enhanced. The image was taken in visible light from a distance of 26.3 million kilometers (16.4 million miles) from Saturn. The image scale is 158 kilometers (98 miles) per pixel. Contrast in the image was enhanced to aid visibility. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Newest picture from Cassini shows Saturn in color CASSINI PHOTO RELEASEPosted: August 6, 2004A frigid ball of gas in the blackness of space, Cassini’s new home, Saturn, appears cool and serene in this natural color image. The spacecraft obtained this view as it sped outward from the planet on its initial orbit. At the left, Saturn’s shadow stretches almost completely across the rings, while at the right, the planet’s illuminated face appears to gaze down at the far-off Sun. Credit: NASA/JPL/Space Science InstituteDownload a larger version of image Images taken through blue, green and red filters with the Cassini spacecraft wide angle camera were combined to create this view. The images were taken on July 17, 2004, from a distance of about 5.8 million kilometers (3.6 million miles) from Saturn. The Sun-Saturn-spacecraft, or phase angle of the image is 93 degrees. The image scale is 346 kilometers (215 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The Cassini orbiter and its two onboard cameras, were designed, developed and assembled at JPL. The imaging team is based at the Space Science Institute, Boulder, Colo. Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Observatory watched Titan when Huygens arrived KECK OBSERVATORY NEWS RELEASEPosted: January 16, 2005The Huygens probe impacted Titan’s atmosphere at 0906 GMT (local time on Titan) Friday, with an expected landing on Titan’s mysterious surface three hours later. This near-infrared image shows Titan at the moment Huygens reached its target. Near-infrared surface image of Titan captured with Keck adaptive optics system moments after the Huygens probe reached its target. The bright and dark patterns on Titan’s surface may be regions of solid ice and of liquid hydrocarbons. Credit: W. M. Keck Observatory”Although no disturbances in Titan’s atmosphere were detected, the observations provide the best images that characterize the satellite at the moment of probe entry”, says Antonin Bouchez, a staff member at the Keck observatory, who was leading the observing effort.”It was worth getting up in the middle of the night for this historic moment”, says Fred Chaffee, director of the Keck Observatory, “despite the bad weather on the mountain”. Winds were blowing at 40-50 mph, while the mountain top itself was still cloaked with snow and ice from a recent storm. Other team members that particpated in the observations were David LeMignant from the Keck Observatory, Imke de Pater, a professor at the University of California at Berkeley, and Michael Brown, a professor at Caltech.Titan is of particular interest to scientists because it is the only moon in our solar system with a dense, methane-rich, nitrogen atmosphere, reminiscent of our own atmosphere here on Earth. The moon is cloaked in a thick, smog-like haze produced by the breakup of methane by sunlight. Further study of this moon could provide clues to planetary formation and evolution and, perhaps, about the early days of Earth as well. To get a closer look at Titan, scientists from three different international space agencies developed the Cassini-Huygens mission, a spacecraft orbiter that arrived in Saturn’s orbit in July 2004 after a seven-year voyage. The four-year mission will include 70 orbits around the ringed planet with an array of instruments to study the planet, its rings and its 30 known moons.The Huygen’s probe detached from Cassini on Christmas Eve, Dec. 24th, 2004. The probe has since been falling to Titan and entered the atmosphere shortly after midnight, local time on Friday morning (0906 GMT) January 14, 2005. Three sets of parachutes were to slow the probe and to provide a stable platform for scientific measurements. Instruments on board will collect information about the atmosphere’s chemical composition and the clouds surrounding Titan during its 2-2.5 hour descent. The data will be radioed to the Cassini orbiter, which will then relay the data to Earth.Near-infrared images were taken from the W. M. Keck Observatory with the near infrared camera, NIRC2, and the adaptive optics system at the time of probe entry. The team had planned imaging sequences to look for thermal emissions or condensates at the probe entry site. Video coverage for subscribers only:VIDEO:NEW PICTURES PRESENTED WITH EXPERT NARRATION VIDEO:LISTEN TO SOUNDS FROM HUYGENS WITH NARRATION AUDIO:LISTEN TO SOUNDS FROM HUYGENS WITH NARRATION VIDEO:RESULTS FROM HUYGENS’ SURFACE SCIENCE PACKAGE VIDEO:CHIEF SCIENTIST EXPLAINS COMMUNICATIONS ERROR VIDEO:SATURDAY PHOTO & SCIENCE BRIEFING AUDIO:SATURDAY PHOTO & SCIENCE BRIEFING VIDEO:THE FIRST PICTURE FROM HUYGENS IS REVEALED VIDEO:HUYGENS POST-LANDING NEWS BRIEFING VIDEO:STATUS REPORT DURING DESCENT AUDIO:MISSION STATUS REPORT DURING DESCENT VIDEO:HUYGENS PRE-ARRIVAL NEWS BRIEFING AUDIO:HUYGENS PRE-ARRIVAL NEWS BRIEFING VIDEO:OVERVIEW OF HUYGENS PROBE’S SCIENCE OBJECTIVES VIDEO:JULY NEWS BRIEFING ON CASSINI’S PICTURES OF TITAN VIDEO:PICTURES SHOWING TITAN SURFACE FROM OCT. FLYBY VIDEO:WHAT’S KNOWN ABOUT TITAN BEFORE THE FIRST FLYBY VIDEO:NARRATED MOVIE OF CLOUDS MOVING NEAR SOUTH POLE VIDEO:OCT. BRIEFING ON RADAR IMAGES OF TITAN SURFACE Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Odd-looking moon Mimas photographed by Cassini CASSINI PHOTO RELEASEPosted: July 26, 2004Soon after orbital insertion, Cassini returned its best look yet at heavily cratered Mimas (398 kilometers, 247 miles across). The enormous crater at the top of this image, named Herschel, is about 130 kilometers (80 miles) wide and 10 kilometers (6 miles) deep. Credit: NASA/JPL/Space Science InstituteThe image was taken in visible light with the narrow angle camera on July 3, 2004, from a distance of 1.7 million kilometers (1 million miles) from Mimas and at a Sun-Mimas-spacecraft, or phase, angle of about 102 degrees. The image scale is 10 kilometers (6 miles) per pixel. It has been magnified here by a factor of 2 to aid visibility.The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Office of Space Science, Washington, D.C. The imaging team is based at the Space Science Institute, Boulder, Colorado.Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.One of Huygens’ two data routes not working BY WILLIAM HARWOOD

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    STORY WRITTEN FOR & USED WITH PERMISSIONPosted: July 3, 2004New pictures of Saturn’s enigmatic moon Titan, taken by cameras aboard the Cassini probe that are capable of penetrating the thick smog-like haze that blankets the frigid world, show strange looking surface features and a deck of methane clouds the size of Arizona. But so far, the instruments have not detected reflections from the surfaces of lakes or small seas of liquid hydrocarbons many scientists believe must form in the ultra-cold environment. Piercing the ubiquitous layer of smog enshrouding Titan, this combination of images from the Cassini visual and infrared mapping spectrometer reveals an exotic surface covered with a variety of materials in the southern hemisphere. Image: NASA/JPL/University of Arizona.But like the sun glint off rivers and lakes visible from airplanes on Earth, the reflections in question can only be seen in a small region of Titan, about 1 percent of the visible surface, based on the relative positions of the sun and Cassini.”If we go by 30 times and we haven’t seen it, we’re going to start getting worried,” said Kevin Baines, a member of Cassini’s Visual Infrared Mapping Spectrometer team. “But I’d say so far, just going by once, it may have been that the specular reflection point was a continent, a dry area.”So the planet could have plenty of liquids and we just got faked out. We don’t know,” he said in a telephone interview. “It’s just 1 percent of the planet, we shouldn’t reach any conclusions from that.”Cassini’s first flyby of Titan, the day after the craft braked into orbit around the ringed planet, was at a distance of more than 200,000 miles. In October, the nuclear-powered probe will pass within just 745 miles of Titan and “we really expect to get a great view then,” said Elizabeth Turtle, a member of the Cassini imaging team. A mosaic of Titan’s south polar region acquired as Cassini passed by at a range of 339,000 kilometers (210,600 miles) on July 2. These images were acquired through special filters designed to see through the thick haze and atmosphere. The surface features become more blurry toward the limb, where the light reflected off the surface must pass through more atmosphere before reaching the camera. The bright spots near the bottom represent a field of clouds near the south pole. Image: NASA/JPL/Space Science Institute.In the meantime, “I can’t tell you how excited I am to be able to show you the images we’ve got of Titan,” she said at a news conference today. “These are just spectacular. It’s our first good look at Titan and Titan hasn’t disappointed us. It’s different from anything we’ve ever seen before.”Using filters to look through specific spectral “windows” in the hazy atmosphere, “we’re seeing surface features as small as 10 to 20 kilometers (six to 12 miles) across,” Turtle said. “This is 10 times better than what we saw during approach. It’s a huge improvement.”A mosaic made up of the best pictures from Cassini’s long-distance flyby show a broad region of Titan’s surface stretching from just above its equator to the moon’s south pole. A large dark feature vaguely resembling the letter H on its side was visible at the top of the mosaic. The equatorial zones below were dominated by brighter areas while a large deck of clouds was prominent near the south pole.Drifting some nine miles up in Titan’s thick nitrogen atmosphere, the clouds clearly moved and changed shape in pictures shot over a five-hour period.”These are dynamical clouds and a meteorologically interesting part of the planet where storms might be happening,” said Baines. “There’s speculation that it may even be associated with a feature on the ground, so we may have some wind motion lifting up air, methane moisture-laden air, to the point where it can condense out and form clouds.”Titan’s atmosphere is made up primarily of nitrogen with small levels of methane and molecular hydrogen. Nitrogen and methane combine in the atmosphere but the action of sunlight, even at Saturn’s distance, causes the compounds to disassociate and hydrocarbons fall to the surface.Based on a variety of lines of evidence, including a surface temperatures as low as -292 degrees Fahrenheit, scientists believe those hydrocarbons must exist in liquid form, as lakes or large pools. It’s also possible Titan is more like a giant sponge, with liquids filling cavities in the materials making up its surface. Shown here is a blowup of a region of Titan imaged on July 2, 2004. This image was taken at a distance of 339,000 kilometers (210,600 miles) and shows brightness variations on the surface of Titan and a bright field of clouds near the south pole. The field of clouds is 450 kilometers (280 miles) across and is the about the size of Arizona. Features as small as 10 kilometers (6 miles) can be discern. Image: NASA/JPL/Space Science InstituteBased on Cassini’s initial, long-distance flyby, the questions remain open. But scientists were nonetheless disappointed not to catch that tell-tale glint on the mission’s first try.”The simulations I’ve done indicate that if the surface liquid is calm and not roughed up a lot by waves, it would be enormously bright, it would be the brightest thing we would see on Titan,” said Bob West, a scientist at the Jet Propulsion Laboratory in Pasadena, Calif. “The calculations also show you can have quite a bit of overlying haze and even with a rough surface, I would have expected to see it by now. And we haven’t.”Even so, Turtle was elated at what the pictures did show.”It’s dangerous to start interpreting a brand new surface that we’ve never seen before, especially on so little sleep,” she said. “But we can’t really resist. We’re seeing surface brightness variations, we’re not seeing topographic shading, the same way you would on a cloudy day on Earth, you don’t see shadows or anything like that.”What we’re seeing is just variations in the brightness of the surface. We see some surface features that are circular, others are linear. There are some features that look like they’re rather concentric to near the south pole. … And the sense that we’re not just seeing circular blobs all over the place suggests it’s not just a heavily cratered body, that there has been geologic activity on Titan.”Now, it’s anyone’s guess as to what that has been, there are quite a lot of candidates, But from these images, we can’t say what the geologic activity has been.”She said the apparent fuzziness of the surface could be the result of overlying haze, but “we are seeing some fairly fine detail as well.”Perhaps not surprisingly, the Cassini data already has forced scientists to change their thinking about the processes going on at the surface.”It had been hypothesized that the dark materials on Titan are hydrocarbons that have fallen out of the atmosphere,” Turtle said. “There’s a lot of methane in the atmosphere and that gets processed and it falls out onto the surface in simple and complex hydrocarbons. It’s been hypothesized that the dark areas were regions where that material had accumulated and that the bright areas might actually be cleaner water-ice regions that were perhaps even swept clean by methane rain coming out of the atmosphere.”That was the theory until Friday night. Data from the infrared mapping spectrometer, Baines said, indicates “the brighter areas are mixtures of water ice but there’s a mixture of other things in it which contributes to the brightness. So we think there are organics that contribute to that brightness. The brighter areas have been contaminated in a sense with organics, the dark areas are more pure water ice.”Stay tuned.In other news, Don Gurnett, principal investigator with Cassini’s Radio and Plasma Wave Science experiment, played a recording of particles slamming into the spacecraft as it passed through the plane of Saturn’s rings.Moving at some 53,000 mph, Cassini crossed the plane between the F and G rings, a region thought to be devoid of large particles that could cause any serious damage. Playing it safe, the spacecraft was oriented with its big dish antenna facing forward to act as a shield.As it turned out, that was probably a good idea. Gurnett said his instrument recorded 680 impacts per second, some 100,000 in all, during the ascending ring plane crossing and a similar number on the other side of Saturn as Cassini flew back down through the plane.The average size of the particles was on the order of a thousandth of a millimeter, about the size of smoke particles. But some were possibly as large as a tenth of a millimeter.”When one of these particles comes in and hits the spacecraft, it essentially makes a little explosion,” Gurnett said. “Hopefully the particle’s not too big so it would go through the spacecraft. … When that explosion occurs, there’s a little puff of gas that’s produced, part of it is spacecraft material and part of it the particle. And it’s heated to like a hundred thousand degrees. And this puff of gas, which is ionized, when it expands over our (instrument) antenna, some of the charge is collected on the antenna and it makes a voltage pulse.”He then played a recording of the impact data, converted into an audio file, which sounded like heavy rain hitting Cassini as it plowed through the ring plane.”I would say it was a good thing to have (Cassini’s dish) antenna pointed into the direction the particles were arriving,” he said. “That was a good move.”Additional coverage for subscribers:VIDEO:WATCH SATURDAY’S NEWS CONFERENCE ON TITAN PICTURES VIDEO:WATCH FRIDAY’S SCIENCE NEWS CONFERENCE VIDEO:THURSDAY’S NEWS BRIEFING ON CASSINI’S FIRST PICTURES VIDEO:RING PICTURES ARE PRESENTED WITH EXPERT NARRATION VIDEO:CASSINI RE-DISCOVERS TINY MOONS ATLAS AND PAN VIDEO:CASSINI BOOMING SOUNDS FROM BOW-SHOCK CROSSING VIDEO:CASSINI BEGINS ENGINE FIRING TO ENTER ORBIT VIDEO:BURN ENDS SUCCESSFULLY TO PUT CASSINI IN ORBIT VIDEO:POST-ARRIVAL NEWS CONFERENCE VIDEO:WEDNESDAY’S 12 P.M. EDT CASSINI STATUS BRIEFING VIDEO:A LOOK AT INTERNATIONAL COOPERATION VIDEO:’RING-SIDE CHAT’ ABOUT SPACE EXPLORATION VIDEO:AN OVERVIEW OF CASSINI’S RADIO SCIENCE VIDEO:TUESDAY’S CASSINI MISSION OVERVIEW BRIEFING VIDEO:CASSINI’S ARRIVAL AT SATURN EXPLAINED VIDEO:SCIENCE OBJECTIVES FOR CASSINI ORBITER VIDEO:HUYGENS LANDER SCIENCE OBJECTIVES Mars rover collectible patchFree shipping to U.S. addresses!This commemorative patch celebrates NASA’s Curiosity rover mission of the Mars Science Laboratory in search of clues whether the Red Planet was once hospitable to life.Gemini 7Gemini 7: The NASA Mission Reports covers this 14-day mission by Borman and Lovell as they demonstrated some of the more essential facts of space flight. Includes CD-ROM.Choose your store: - - - Apollo patchesThe Apollo Patch Collection: Includes all 12 Apollo mission patches plus the Apollo Program Patch. Save over 20% off the Individual price.Choose your store: - - - Mars Rover mission patchA mission patch featuring NASA’s Mars Exploration Rover is available from our online.Choose your store: - - - Apollo 9 DVDOn the road to the moon, the mission of Apollo 9 stands as an important gateway in experience and procedures. This 2-DVD collection presents the crucial mission on the voyage to the moon. Choose your store: - - - Gemini 7Gemini 7: The NASA Mission Reports covers this 14-day mission by Borman and Lovell as they demonstrated some of the more essential facts of space flight. Includes CD-ROM.Choose your store: - - - Apollo patchesThe Apollo Patch Collection: Includes all 12 Apollo mission patches plus the Apollo Program Patch. Save over 20% off the Individual price.Choose your store: - - - Mars Rover mission patchA mission patch featuring NASA’s Mars Exploration Rover is available from our online.Choose your store: - - - Apollo 9 DVDOn the road to the moon, the mission of Apollo 9 stands as an important gateway in experience and procedures. This 2-DVD collection presents the crucial mission on the voyage to the moon. Choose your store: - - - Ares 1-X PatchThe official embroidered patch for the Ares 1-X rocket test flight, is available for purchase.Apollo CollageThis beautiful one piece set features the Apollo program emblem surrounded by the individual mission logos.Expedition 21The official embroidered patch for the International Space Station Expedition 21 crew is now available from our stores.Hubble PatchThe official embroidered patch for mission STS-125, the space shuttle’s last planned service call to the Hubble Space Telescope, is available for purchase. | | | | 2014 Spaceflight Now Inc.Cassini radar sees flow-like feature across Titan UNIVERSITY OF ARIZONA NEWS RELEASEPosted: November 8, 2004A strikingly bright, lobate feature has turned up in one of Cassini’s first radar images of Saturn’s moon Titan.”It may be something that flowed,” Cassini radar team member Ralph Lorenz of the University of Arizona said. “Or it could be something carved by erosion. It’s too early to say.”But it looks very much like it’s something that oozed across the surface.It may be some sort of ‘cryovolcanic’ flow, an analog to volcanism on Earththat is not molten rock but, at Titan’s very cold temperatures, molten ice.” This is a synthetic aperture radar image of Titan. Dark regions may represent areas that are smooth, made of radar-absorbing materials, or are sloped away from the direction of illumination. A striking lobate bright feature stretches from upper left to lower right across this image, with connected ‘arms’ to the east. The fact that the lower (southern) edges of the features are brighter is consistent with the lobate structure being raised above the relatively featureless darker background. Credit: NASA/JPLCassini radar mapped about one percent of Titan’s surface during theCassini spacecraft’s first close Titan flyby Oct. 26. The radar surveycovered a strip 75 miles wide (120 kilometers) and 1,200 miles (1,960kilometers) long in Titan’s northern hemisphere.Cassini was flying about 1,550 miles (2,494 kilometers) above Titan’ssurface, with its radar centered at about 45 degrees north, 30 degreeswest, when it mapped the 90-square-mile (230-square-kilometer) area shownin the new radar image.The Cassini radar team presented the image today at the 86th annual meetingof the American Astronomical Society Division of Planetary Sciences inLouisville, Ky.The radar instrument works by bouncing radio signals off Titan’s surfaceand timing their return. The more signal reflected back to thespacecraft, the brighter the imaged area. Turning radio signals intoradar images is time consuming because so many numerical calculations mustbe made. “There’s no such thing as a ‘raw’ radar image,” Lorenz said.But two days after the Oct. 26 flyby, Cassini scientists knew that Titan isno impact-crater-pocked dead world, but a much more interesting place.Titan’s surface is young — it’s been shaped by dynamic geologicprocessing, Lorenz, Cassini interdisciplinary scientist Jonathan Lunine ofthe University of Arizona, and other Cassini scientists agree.Given this newest image, Lunine said, “Radar has provided the firstevidence for possible young cryovolcanism on Titan’s surface. Now ourchallenge is to find out what is flowing, how it works, and theimplications for Titan’s evolution.”The Cassini-Huygens mission is a cooperative project of NASA, the EuropeanSpace Agency and the Italian Space Agency. The Jet Propulsion Laboratory, adivision of the California Institute of Technology in Pasadena, manages theCassini-Huygens mission for NASA’s Science Mission Directorate, Washington,D.C. The Cassini orbiter and its two onboard cameras were designed,developed and assembled at JPL. The radar instrument team is based at JPL,working with team members from the United States and several Europeancountries.Cassini posterJust in time for the Cassini spacecraft’s arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12×12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA’s Mars Exploration Rover is now available from the Astronomy Now Store.Columbia ReportThe official accident investigation report into the loss of the space shuttle Columbia and its crew of seven. Includes CD-ROM. Choose your store: | | | | 2014 Spaceflight Now Inc.Cassini radar shows diversity on Saturn’s moon Titan CASSINI PHOTO RELEASEPosted: October 28, 2004 Credit: NASA/JPLDownload larger image version This radar image of the surface of Saturn’s moon Titan was acquired on October 26, 2004, when the Cassini spacecraft flew approximately 1,200 kilometers (745 miles) above the surface and acquired radar data for the first time. It reveals a complex geologic surface thought to be composed of icy materials and hydrocarbons. A wide variety of geologic terrain types can be seen on the image; brighter areas may correspond to rougher terrains and darker areas are thought to be smoother. A large dark circular feature is seen at the western (left) end of the image, but very few features resembling fresh impact craters are seen. This suggests that the surface is relatively young. Enigmatic sinuous bright linear features are visible, mainly cutting across dark areas. The image is about 150 kilometers (93 miles) wide and 250 kilometers (155 miles) long, and is centered at 50 N, 82 W in the northern hemisphere of Titan, over a region that has not yet been imaged optically. The smallest details seen on the image are about 300 meters (186 miles) across. The data were acquired in the synthetic aperture radar mode of Cassini’s radar instrument. In this mode, radio signals are bounced off the surface of Titan. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA’s Science Mission Directorate, Washington, D.C. The Cassini orbiter and its two onboard cameras were designed, developed and assembled at JPL. The instrument team is based at NASA’s Jet Propulsion Laboratory, Pasadena, Calif. Cassini posterJust in time for the Cassini spacecraft’s arrival at Saturn, this new poster celebrates the mission to explore the ringed planet and its moons. 2005 CalendarThe 2005 edition of the Universe of the Hubble Space Telescope calendar is available from our U.S. store and will soon be available worldwide. This 12×12-inch calendar features spectacular images from the orbiting observatory.Moon panoramaTaken by Apollo 14 commander Alan Shepard, this panoramic poster shows lunar module pilot Edgar Mitchell as a brilliant Sun glare reflects off the lunar module Antares.Mars Rover mission patchA mission patch featuring NASA’s Mars Exploration Rover is now available from the Astronomy Now Store.Columbia ReportThe official accident investigation report into the loss of the space shuttle Columbia and its crew of seven. Includes CD-ROM. Choose your store: | | | | 2014 Spaceflight Now Inc.Cassini sails to Saturn ‘Flagship mission of our time’ BY WILLIAM HARWOOD

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    Hey, how’s it going?

    I want to pass along some very important news that everyone needs to hear!

    In December of 2017, Donald Trump made history by recognizing Jerusalem as the captial of Israel. Why is this big news? Because by this the Jewish people of Israel are now able to press forward in bringing about the Third Temple prophesied in the Bible.

    The Jewish people deny Jesus as their Messiah and have stated that their Messiah has been identified and is waiting to be revealed. They say this man will rule the world under a one world religion called “spiritualism”.

    They even printed a coin to raise money for the Temple with Donald Trumps face on the front and with king Cyrus’(who built the second Temple) behind him. On the back of the coin is an image of the third Temple.

    The Bible says this false Messiah who seats himself in the Third Temple will be thee antichrist that will bring about the Great Tribulation, though the Jewish people believe he will bring about world peace. It will be a false peace for a period of time. You can watch interviews of Jewish Rabbi’s in Israel speaking of these things. They have their plans set in place. It is only years away!

    More importantly, the power that runs the world wants to put a RFID microchip in our body making us total slaves to them. This chip matches perfectly with the Mark of the Beast in the Bible, more specifically Revelation 13:16-18:

    He causes all, both small and great, rich and poor, free and slave, to receive a mark on their right hand or on their foreheads, and that no one may buy or sell except one who has the mark or the name of the beast, or the number of his name.

    Here is wisdom. Let him who has understanding calculate the number of the beast, for it is the number of a man: His number is 666.

    Referring to the last days, this could only be speaking of a cashless society, which we have yet to see, but are heading towards. Otherwise, we could still buy or sell without the mark amongst others if physical money was still currency. RFID microchip implant technology will be the future of a one world cashless society containing digital currency. It will be implanted in the right-hand or the forehead, and we cannot buy or sell without it! We must grow strong in Jesus. AT ALL COSTS, DO NOT TAKE IT!

    Then a third angel followed them, saying with a loud voice, “If anyone worships the beast and his image, and receives his mark on his forehead or on his hand, he himself shall also drink of the wine of the wrath of God, which is poured out full strength into the cup of His indignation. He shall be tormented with fire and brimstone in the presence of the holy angels and in the presence of the Lamb. And the smoke of their torment ascends forever and ever; and they have no rest day or night, who worship the beast and his image, and whoever receives the mark of his name.” (Revelation 14:9-11).

    People have been saying the end is coming for many years, but we need two key things. One, the Third Temple, and two, the technology for a cashless society to fulfill the prophecy of the Mark of the Beast.

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  667. Michaela Pettinato Says:

    Hey, how’s it going?

    I want to pass along some very important news that everyone needs to hear!

    In December of 2017, Donald Trump made history by recognizing Jerusalem as the captial of Israel. Why is this big news? Because by this the Jewish people of Israel are now able to press forward in bringing about the Third Temple prophesied in the Bible.

    Jewish Rabbis have publicly announced that their Messiah will be revealed in the coming years who will be a leader and spiritual guide to all nations, gathering all religions under the worship of one God. They deny Jesus as their Messiah, and the Bible tells us this Jewish Messiah will be the counterfiet that will bring about a false peace, and ultimatley the great tribulation.

    They even printed a coin to raise money for the Temple with Donald Trumps face on the front and with king Cyrus’(who built the second Temple) behind him. On the back of the coin is an image of the third Temple.

    More importantly, the power that runs the world wants to put a RFID microchip in our body making us total slaves to them. This chip matches perfectly with the Mark of the Beast in the Bible, more specifically in Revelation 13:16-18:

    “He causes all, both small and great, rich and poor, free and slave, to receive a mark on their right hand or on their foreheads, and that no one may buy or sell except one who has the mark or the name of the beast, or the number of his name.

    Here is wisdom. Let him who has understanding calculate the number of the beast, for it is the number of a man: His number is 666.”

    Referring to the last days, this could only be speaking of a cashless society, which we have yet to see, but are heading towards. Otherwise, we could still buy or sell without the mark amongst others if physical money was still currency. This Mark couldn’t be spiritual because the word references two different physical locations. If it was spiritual it would just say in the forehead. RFID microchip implant technology will be the future of a one world cashless society containing digital currency. It will be implanted in the right-hand or the forehead, and we cannot buy or sell without it! We must grow strong in Jesus. AT ALL COSTS, DO NOT TAKE IT!

    “Then a third angel followed them, saying with a loud voice, “If anyone worships the beast and his image, and receives his mark on his forehead or on his hand, he himself shall also drink of the wine of the wrath of God, which is poured out full strength into the cup of His indignation. He shall be tormented with fire and brimstone in the presence of the holy angels and in the presence of the Lamb. And the smoke of their torment ascends forever and ever; and they have no rest day or night, who worship the beast and his image, and whoever receives the mark of his name” (Revelation 14:9-11).

    People have been saying the end is coming for many years, but we needed two key things. One, the Third Temple, and two, the technology for a cashless society to fulfill the prophecy of the Mark of the Beast.

    Visit WWW.BIBLEFREEDOM.COM to see proof for these things and much more!

    If you haven’t already, it is time to seek God with all your heart. Jesus loves you more than you could imagine. He wants to have a relationship with you and redeem you from your sins. Turn to Him and repent while there is still hope! God bless!

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  670. Emmanuella Love Says:

    Hey, how’s it going?

    I want to pass along some very important news that everyone needs to hear!

    In December of 2017, Donald Trump made history by recognizing Jerusalem as the capital of Israel. Why is this big news? Because by this the Jewish people of Israel are now able to press forward in bringing about the Third Temple prophesied in the Bible.

    Jewish Rabbis have publicly announced that their Messiah will be revealed in the coming years who will be a leader and spiritual guide to all nations, gathering all religions under the worship of one God.

    Biblical prophecy tells us that this Jewish Messiah who will take the stage will be the antichrist “who opposes and exalts himself above all that is called God or that is worshiped, so that he sits as God in the temple of God, showing himself that he is God” (2 Thessalonians 2:4). For a time he will bring about a false peace, but “Therefore when you see the ‘abomination of desolation,’ spoken of by Daniel the prophet, standing in the holy place (Matthew 24:15)…then there will be great tribulation, such as has not been since the beginning of the world until this time, no, nor ever shall be” (Matthew 24:21).

    More importantly, the power that runs the world wants to put a RFID microchip in our body making us total slaves to them. This chip matches perfectly with the Mark of the Beast in the Bible, more specifically in Revelation 13:16-18:

    “He causes all, both small and great, rich and poor, free and slave, to receive a mark on their right hand or on their foreheads, and that no one may buy or sell except one who has the mark or the name of the beast, or the number of his name.

    Here is wisdom. Let him who has understanding calculate the number of the beast, for it is the number of a man: His number is 666.”

    Referring to the last days, this could only be speaking of a cashless society, which we have yet to see, but are heading towards. Otherwise, we could still buy or sell without the mark amongst others if physical money was still currency. This Mark couldn’t be spiritual because the word references two different physical locations. If it was spiritual it would just say in the forehead. RFID microchip implant technology will be the future of a one world cashless society containing digital currency. It will be implanted in the right-hand or the forehead, and we cannot buy or sell without it. Revelation 13:11-18 tells us that a false prophet will arise on the world scene doing miracles before men, deceiving them to receive this Mark. Do not be deceived! We must grow strong in Jesus. AT ALL COSTS, DO NOT TAKE IT!

    “Then a third angel followed them, saying with a loud voice, “If anyone worships the beast and his image, and receives his mark on his forehead or on his hand, he himself shall also drink of the wine of the wrath of God, which is poured out full strength into the cup of His indignation. He shall be tormented with fire and brimstone in the presence of the holy angels and in the presence of the Lamb. And the smoke of their torment ascends forever and ever; and they have no rest day or night, who worship the beast and his image, and whoever receives the mark of his name” (Revelation 14:9-11).

    People have been saying the end is coming for many years, but we needed two key things. One, the Third Temple, and two, the technology for a cashless society to fulfill the prophecy of the Mark of the Beast.

    Visit WWW.BIBLEFREEDOM.COM to see proof for these things and why the Bible truly is the word of God!

    If you haven’t already, it is time to seek God with all your heart. Jesus loves you more than you could imagine. He wants to have a relationship with you and redeem you from your sins. Turn to Him and repent while there is still hope! This is forever…God bless!

    “EITHER HUMAN INTELLIGENCE ULTIMATELY OWES ITS ORIGIN TO MINDLESS MATTER OR THERE IS A CREATOR…” - JOHN LENNOX

    We all know God exists. Why? Because without Him, we couldn’t prove anything at all. Do we live our lives as if we cannot know anything? No. So why is God necessary? In order to know anything for certain, you would have to know everything, or have revelation from somebody who does. Who is capable of knowing everything? God. So to know anything, you would have to be God, or know God.

    A worldview without God cannot account for the uniformity and intelligibility of nature. And why is it that we can even reason that God is the best explanation for this if there is no God? We are given reason to know or reject God, but never to know that He does not exist.

    It has been calculated by Roger Penrose that the odds of the initial conditions for the big bang to produce the universe that we see to be a number so big, that we could put a zero on every particle in the universe, and even that would not be enough to use every zero. What are the odds that God created the universe? Odds are no such thing. Who of you would gamble your life on one coin flip?

    Is there evidence that the Bible is the truth? Yes. Did you know that the creation accounts listed in the book of Genesis are not only all correct, but are also in the correct chronological order? That the Bible doesn’t say the Earth was formed in six 24-hour days but rather six long but finite periods of time? That the Bible makes 10 times more creation claims than all major “holy” books combined with no contradictions, while these other books have errors in them? The Bible stood alone by concurring with the big bang saying, “In the beginning God created the heaven and the earth” (Genesis 1:1); and says our universe is expanding, thousands of years before scientists discovered these things. Watch a potential life-changing video on the front page of WWW.BIBLEFREEDOM.COM with Astronomer(PhD) Hugh Ross explaining all these facts based on published scientific data. He has authored many books, backed even by atheist scientists.

    Jesus came to pay a debt that we could not; to be our legal justifier to reconcile us back to a Holy God; only if we are willing to receive Him: “For the wages of sin is death…” (Romans 6:23).

    God so loved the world that He gave us His only begotten son, so that whoever believes in Him, through faith, shall not perish, but have everlasting life. Jesus says if we wish to enter into life to keep the commands! The two greatest commands are to love God with all your heart, soul, strength, and mind; and your neighbor as yourself. All the law hang on these commands. We must be born of and lead by the Holy Spirit, to be called children of God, to inherit the kingdom. If we are willing to humble ourselves in prayer to Jesus, to confess and forsake our sins, He is willing to give the Holy Spirit to those who keep asking of Him; giving us a new heart, leading us into all truth!

    Jesus came to free us from the bondage of sin. The everlasting fire was prepared for the devil and his angels due to disobedience to God’s law. If we do the same, what makes us any different than the devil? Jesus says unless we repent, we shall perish. For sin is the transgression of the law. We must walk in the Spirit so we may not fulfill the lusts of the flesh, being hatred, fornication, drunkenness and the like. Whoever practices such things will not inherit the kingdom (Galatians 5:16-26). If we sin, we may come before Jesus to ask for forgiveness (1 John 2:1-2). Evil thoughts are not sins, but rather temptations. It is not until these thoughts conceive and give birth by our own desires that they become sin (James 1:12-15). When we sin, we become in the likeness of the devil’s image, for he who sins is of the devil (1 John 3:8); but if we obey Jesus, in the image of God. For without holiness, we shall not see the Lord (Hebrews 12:14).

    The oldest religion in the world is holiness through faith (James 1:27). What religion did Adam and Eve follow before the fall? Jesus, Who became the last Adam, what religion does He follow? Is He not holy? He never told us to follow the rituals and traditions of man but to take up our cross and follow Him (Luke 9:23). There are many false doctrines being taught leading people astray. This is why we need the Holy Spirit for discernment. Unlike religion, holiness cannot be created. It is given to us from above by the baptism of the Spirit. Jesus is more than a religion; He is about having a personal relationship with the Father. Start by reading the Gospel of Matthew, to hear the words of God, to know His character and commandments. Follow and obey Jesus, for He is the way, the truth, and the life!

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