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STORY WRITTEN FOR & USED WITH PERMISSIONPosted: June 12, 2004 Cassini fires its engine to enter orbit around Saturn as illustrated in this artist's concept. Credit: NASA/JPLOn May 27, Cassini's flight computer fired the craft's main engine for six minutes and two seconds, setting up a June 11 flyby of Phoebe and fine-tuning the craft's trajectory for the all-important Saturn Orbit Insertion burn the night of June 30. Trajectory Correction Maneuver 20 was a relatively short, but critical rocket firing because it marked the first use of the main engine system since the Deep Space Maneuver back in 1998. To everyone's relief, TCM-20 came off without a hitch. The helium latch valve opened 70 seconds before ignition and the leaky regulator worked as required to maintain the proper pressure. "We've got a real nice propulsion system," said lead propulsion engineer Todd Barber. "It's a plumber's nightmare, there are so many valves and alternate paths and contingency paths available that basically, we're able to handle a lot of anomalies. And the regulator leak we saw was right after launch and we've been able to accommodate that with the way we time the opening of valves, etc." Even so, Barber will feel much better after Cassini successfully brakes into orbit. "It's been a long time coming and the hopes and dreams of thousands of engineers are resting on that one evening. When we get the signal back is when we'll all go take a deep breath. Hold your ears, because they might pop." To get into the desired orbit around Saturn, Cassini's main engine must fire for 96.4 minutes beginning at 10:35:42 p.m. EDT on June 30 (0235:42 GMT July 1). An underburn, or early cutoff, could doom the mission. Rocket Engine Assembly A - REA-A - must fire for more than 85 minutes to put Cassini into any kind of usable orbit. Asked what keeps him awake at night, program manager Bob Mitchell gave the obvious answer. "In general, just worrying that SOI is going to work," he said in an interview. "The confidence that it will is very high, just based on all of the testing, all the elaborate work that we have put into this, as well as our experience with the spacecraft to date. We've done 15 or 16 maneuvers using the main engine ... and so we have every reason to believe this thing is going to work just fine." But, he added, "the software the thing flies is all complex and I just worry about what bugs are still in there. I think it must be inevitable that there are still bugs in there for something this complex. We've tested it extensively, we have a test bed here in the basement of our building that is a quite high fidelity spacecraft simulator and the sequences have been run through there many, many times. We have injected faults, we've had various components break, where we simulated a break in the test bed and looked to see what response we got. And at the moment, everything works. All the tests that we've done, all the simulations indicate that everything is just fine." This graphic shows the ring plane crossing and orbit insertion burn. Credit: NASA/JPLThe maneuver has little margin for error. Cassini first must avoid any crippling debris impacts when it crosses the ring plane between the F and G rings, moving from the lower side of the rings to the upper side as viewed from Earth. Pioneers 10 and 11, along with Voyager 2, flew through the gap with no problems but Cassini flight planners are taking no chances. Before traversing the ring plane, the spacecraft will be oriented with its high-gain dish antenna facing the direction of travel to act as a shield. Voyager 2 went through outer edge of the G ring and its instruments recorded "lots of evidence of micrometeoroid hits when going through, but nothing serious," said Voyager veteran Torrence Johnson, a Cassini imaging team member and chief scientist for the Galileo mission. "So we have that maneuvering to do and then there's the fact that the place is just a junky system," he said in an interview. "We're going in close, we're skimming right over the rings, everybody thinks we've modeled all this right and we're being reasonably cautious. But I told some of the guys early on, if they're going to be scared of ring particles they ought to remember John Paul Jones' letter to Congress, 'give me a fast ship for I intend to sail in harm's way.' "I don't think anybody's real complacent about this thing," Johnson said. "I think we've done everything we can to make sure we don't have any human or systems screw ups, but nature can still get you." Jerry Jones, Cassini's chief navigator, said flying through the ring plane relatively close to Saturn will save propellant and makes the rocket firing more efficient. "But the real clincher, given all that, is the science in that close. We're going to be sitting there looking right down on those rings." "We've got one class-A camera on this spacecraft," he said in an interview. "It's a beautiful telescope, it has great resolution, very sharp edges and for optical navigation, I'm just pleased as punch. ... The science opportunity going over the rings should be just fantastic, to say nothing of showing the public what they've paid for." Once safely through the ring plane, Cassini will re-orient itself once again, swapping ends to put the main engine forward for the SOI burn. NASA originally planned to carry out the rocket firing "in the blind," with Cassini focusing on science observations while the engine put on the brakes. But in the wake of back-to-back Mars mission failures in 1999, NASA management ordered engineers to figure out a way for Cassini to provide at least some information about the start of the burn, its progress and its termination. This graphic shows Cassini's track as it enters orbit around Saturn. Credit: NASA/JPL"So we went back and scrambled then," Barber said. "We had a compromise solution. We could have pointed the high-gain antenna to Earth during the whole burn and have telemetry but there was a large delta V (fuel) penalty to do so. So the plan is to switch to a low gain antenna and that will allow us to maintain Doppler during the burn." While no actual data will be transmitted to Earth, analysis of the Doppler shift of a carrier signal from the spacecraft will tell engineers when the burn started, the precise deceleration it produces and when it stops. "There were two key things we wanted to be sure we could differentiate between," Mitchell said. "One was in the event we just lost it entirely and never saw it again, we wanted to be able to differentiate between whether we had a problem going through the ring plane or whether we did that successfully and had a problem during the course of the burn itself. So with the data we have, we will know that quite well." After re-orienting itself for SOI, Cassini will begin transmitting a carrier signal. Six minutes later, the burn will begin, showing up on computer screens at the Jet Propulsion Laboratory as a change in the slope of the carrier frequency. Thirty minutes later, the signal is expected to fade out for 25 minutes or so as Cassini passes behind Saturn's A ring as viewed from Earth. Engineers then expect six minutes of carrier through the Cassini division before another 28-minute communications blackout while the spacecraft passes behind the broad B ring. Closest approach to Saturn - 12,400 miles from the planet's cloud tops - is expected at 12:03 a.m. EDT (0403 GMT) July 1, nine minutes before the SOI burn comes to an end. The first images and other data from the orbit insertion maneuver are expected around 8:39 a.m. EDT (1239 GMT). Here is an edited timeline of critical events in the SOI maneuver for the evening of June 30 through the morning of July 1 (all times in EDT): "We turn off of Earth line shortly prior to the ring plane crossing," Mitchell explained. "We turn to point the high-gain antenna in the direction we need to be in to shield the rest of the spacecraft and then there's a period of about an hour where we don't have any contact. "Then when we turn back to go to the burn attitude, at about the time we get to that attitude, which is six minutes prior to the burn start, we will crank up a signal that comes from one of the low gain antennas. There's no telemetry, it's just a carrier. "But that carrier will allow us to get Doppler and that'll tell us if the spacecraft is operating fine and has not had any safing events. And then during the course of the burn, that Doppler will let us see quite accurately what the acceleration levels are. So if the system is performing nominally or over performing or under performing, the Doppler will show that very well." The day after orbit insertion, Cassini will pass within 205,000 miles of Titan, the first official Titan encounter of the mission and one that could prove, one way or the other, whether the spacecraft's cameras will be able to penetrate the hazy atmosphere as scientists hope. Between July 4 and 11, Cassini will be out of contact with Earth as Saturn passes behind the sun. The SOI sequence will end on July 30 as tour sequence No. 3 begins. Sometime around Aug. 23, Cassini's main engine is scheduled to fire in what will be the last fully helium-regulated burn of the mission: a 51-minute maneuver that will change the spacecraft's velocity by 877 mph. The Perigee Raise Maneuver, or PRM, will raise the low point of Cassini's orbit and set up the first close flyby of Titan in October. After another flyby in December, the Huygens probe will be released for atmospheric entry during the mission's third Titan encounter in January. Cassini's initial orbits around Saturn are illustrated in this graphic. Credit: NASA/JPLThe SOI maneuver is one of only three so-called "critical sequences" built into Cassini's mission software. A critical sequence is one that simply must execute properly to ensure mission success. The launch to Venus was one such sequence and the only other one is the Huygens data relay sequence. SOI is "the only maneuver that we will do throughout the entire course of the mission where we just absolutely have to do this burn right now," Mitchell said at a news briefing. "If this burn doesn't work, then we would have a Saturn flyby and that's not what we're here about. So we have designed what we refer to as a critical sequence where no matter what fault might occur, the spacecraft will not let the burn halt. Now in some modes it will stop the burn, swap to the other engine and then continue on with the burn. But the burn will continue even in the presence of faults." During normal operations, a problem with a spacecraft system would trigger fault-protection software that would shut down unnecessary activity, a condition known as safe mode. There are numerous variations, depending on the nature and timing of the fault and whether the spacecraft still knows its orientation in space. The end result, however, is the same: Cassini shuts down, finds the sun (Earth will never be more than six degrees away), switches to low-data-rate communications and awaits instructions from Earth. Because of Saturn's great distance and the slow-speed radio link used in safe mode, engineers would need at least 48 hours to restore Cassini to normal operations. Such a fault during the SOI maneuver would shut the main engine down, interrupting the all-important rocket firing and possibly dooming the mission. But in critical sequence mode, that will not be allowed to happen. "In critical mode, if the spacecraft detects a fault - we get a glint in the eye of the star scanner or the thrusters don't like what they're doing or a piece of hardware doesn't work right - the spacecraft will detect a fault," said Julie Webster, lead spacecraft engineer. "The sequence will halt and the spacecraft is allowed through its autonomous fault protection to go off and fix the fault. "And then it will come back and say I've detected a fault, I've fixed the fault. And then it'll come back and say OK, critical sequence, you can restart. And the critical sequence will say Oh, but I've gotta remember where I was. We have what we call a mark and rollback strategy. So it'll roll back to the last good mark point and it will resend all the commands necessary to execute the next states that it needs to be in. It'll recommend all of those and continue on. And so, if there's a fault anytime during the critical sequence, it'll stop, halt, detect the fault, correct the fault and then restart the sequence." That's where Cassini's second main engine comes in. If a fault of any kind interrupts the SOI sequence, the computer will fire up Rocket Engine Assembly B and continue the burn. Cassini's two engines are seen in this pre-launch photo. Credit: NASA/JPL"In the burn, we have already disabled any fault protection activity that's not necessary to complete the burn," Webster said. "So we've got fault monitors, say, on the CDS (command and data system) computer and on the radio. Well, the radio's not necessary to complete a burn. Neither is the CDS, ironically, because the attitude and articulation control system also has its own computer and once the CDS has told it to go do a burn, it takes over and says I don't need you anymore, I'll complete this burn and I'll let you know when I'm done. So only the fault protection that's necessary to complete the burn is active. "It would detect a fault in where it's pointing or the propulsion system wasn't acting right, maybe under thrusting or over thrusting. If there's a fault during the burn, then we terminate the burn. We try to fix the fault and then we mark and roll back, pick up where we did, restart but we're going to restart on the second engine. It takes at least two hours to cool down one engine. So 10 minutes later, we can restart on engine B and minimize our overall cost." But any safe mode that would necessitate firing REA-B also would terminate priceless SOI science operations, a small price to pay if survival of the mission is at stake. Cassini has a seven-hour window in which to complete the SOI maneuver and "as long as we got the correct amount of burn at any time in that seven-hour period, we would get into orbit," Webster said. "We might not like the orbit, but we'd get into orbit." While outwardly confident, many project officials are naturally anxious going into the make-or-break maneuver. But not Carolyn Porco. To her, the real issue is collecting the science required to meet Cassini's enormously challenging objectives. "Everything's working very well. Cassini is a very robust spacecraft, the instruments are working very well and I have personally no worries about Saturn orbit insertion at all," she said. "That's not what worries me about Cassini. What worries me about Cassini is the magnitude of the job. It's absolutely enormous. "What needs to be conveyed to people is the magnitude of this mission. It is not a Discovery-class mission. The breadth of its scientific objectives is tremendous. What we are going to do at Saturn will ultimately reach well beyond Saturn itself. It will teach us about the behavior of disk systems all throughout the universe. The processes going on in the disks of material from which planets are forming around other stars, it will tell us about what's going on in spiral galaxies, because the kind of things we find in Saturn's rings are directly applicable to what we find in galaxies. "The study of Titan, it's the place to go in the solar system to find a body that is the most Earth-like. And so what we find at Titan will inform us about many aspects of the Earth and the behavior of its atmosphere, possibly processes that were part of the run up to the origin of life on Earth. On and on. It is really, truly the flagship mission of our time."MISSION PREVIEWStargaze II DVDThe Stargaze II DVD has arrived! It features over 65 minutes of all new videos of the universe with newly-composed dolby digital and DTS 5.1 Channel surround sound music. Choose your store: - - - Solar system poster This new poster is popular for classrooms and children's bedrooms. It includes interesting facts and figures about the planets and their moons. Choose your store: - - - Apollo 15 DVD Relive on DVD the journey of Apollo 15, one of the great explorations of our time. This unique six-disc DVD set contains all the available television and 16mm film footage from the mission.Choose your store: - - - Shuttle patchesCollect the official mission patches for the first ten space shuttle flights and save off the regular price. Introducing the Space Shuttle Patch Collection.Choose your store: - - - | | | | 2014 Spaceflight Now Inc.Spaceflight Now +Premium video content for our Spaceflight Now Plus .Cassini previewThe Cassini spacecraft's arrival at Saturn is previewed in this detailed news conference from NASA Headquarters on June 3. (50min 01sec file)Saturn arrival explainedCassini's make-or-break engine firing to enter orbit around Saturn is explained with graphics and animation. Expert narration is provided by Cassini program manager Robert Mitchell. (3min 33sec file)Cassini mission scienceThe scientific objectives of the Cassini mission to study the planet Saturn, its rings and moons are explained by Charles Elachi, director of the Jet Propulsion Laboratory. (4min 54sec file)Huygens mission scienceAfter entering orbit around Saturn, the Cassini spacecraft will launch the European Huygens probe to make a parachute landing on the surface of the moon Titan. The scientific objectives of Huygens are explained by probe project manager Jean-Pierre Lebreton. (3min 14sec file)Saturn's moon Iapetus as you've never seen it CASSINI PHOTO RELEASEPosted: December 8, 2004New details on Iapetus are illuminated by reflected light from Saturn in this revealing Cassini image. Never-before-seen features on the Saturn-facing part of Iapetus' bright trailing hemisphere are visible for the first time, including many dark spots, and a sharper view of a dark, circular structure that was first seen at very low resolution by NASA's Voyager 1 in 1980. Iapetus diameter is 1,436 kilometers (892 miles). Credit: NASA/JPL/Space Science InstituteThe image shows mainly the night side of Iapetus; part of the far brighter sunlit side appears at the right and is overexposed due to the long integration time of 180 seconds. Despite this long exposure time, almost no blurring due to the spacecraft's motion is apparent. This technique for imaging the night side of Iapetus will be used again during a flyby on Jan. 1, 2005, when Cassini will pass 13 times closer to the icy moon. The image was taken in visible light with the Cassini spacecraft narrow angle camera on Oct. 22, 2004, at a distance of 1.6 million kilometers (994,000 miles) from Iapetus, and from a Sun-Iapetus-spacecraft, or phase, angle of 161 degrees. The view is centered on 0.4 degrees north latitude, 317 degrees west longitude on Iapetus. The image scale is 9.4 kilometers (5.8 miles) per pixel. Credit: NASA/JPL/Space Science InstituteDownload larger image version IMAGE 2 These spectacular Cassini images of Saturn's moon Iapetus show an enticing world of contrasts. These are the sharpest views of Iapetus from Cassini so far, and they represent better resolution than the best images of this moon achieved by NASA's Voyager spacecraft. Images obtained using ultraviolet (centered at 338 nanometers), green (568 nanometers) and infrared (930 nanometers) filters were combined to produce the enhanced color views at left and center; the image at the right was obtained in visible white light. The images on the bottom row are identical to those on top, with the addition of an overlying coordinate grid. These views show parts of the moon's anti-Saturn side--the side that faces away from the ringed planet--which will not be imaged again by Cassini until Sept., 2007. In the central view, part of the moon's eastern edge was not imaged and appears to be cut off. With a diameter of 1,436 kilometers (892 miles), Iapetus is Saturn's third largest moon. It is famous for the dramatic contrasts in brightness on its surface--the leading hemisphere is as dark as a freshly-tarred street, and the trailing hemisphere and poles almost as bright as snow. Many impact craters can be seen in the bright terrain and in the transition zone between bright and dark, and for the first time in parts of the dark terrain. Also visible is a line of mountains that appear as a string of bright dots in the two color images at left, and on the eastern limb in the image at right. These mountains were originally detected in Voyager images, and might compete in height with the tallest mountains on Earth, Jupiter's moon Io and possibly even Mars. Further observations will be required to precisely determine their heights. Interestingly, the line of peaks is aligned remarkably close to the equator of Iapetus. The large circular feature rotating into view in the southern hemisphere is probably an impact structure with a diameter of more than 400 kilometers (250 miles), and was first seen in low-resolution Cassini images just two months earlier. Theses images were taken with the Cassini spacecraft narrow angle camera between Oct, 15 and 20, 2004, at distances of 1.2, 1.1 and 1.3 million kilometers (746,000, 684,000 and 808,000 miles) from Iapetus, respectively. The Sun-Iapetus-spacecraft, or phase, angle changes from 88 to 144 degrees across the three images. The image scale is approximately 7 kilometers (4.5 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.Saturn's moon Phoebe likely born in outer solar system BY WILLIAM HARWOOD