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BY SPACEFLIGHT NOW February 28, 2001 -- Follow the conclusion of NASA's NEAR Shoemaker exploration mission after the craft's unprecedented landing on an asteroid. Reload this page for the very latest.
WEDNESDAY, FEBRUARY 28, 2001
FRIDAY, FEBRUARY 23, 2001
WEDNESDAY, FEBRUARY 14, 2001
2300 GMT (6:00 p.m. EST) As announced earlier today, NEAR's mission has been extended for up to 10 days to gather data from the spacecraft's gamma-ray spectrometer, a scientific instrument that could provide unprecedented information about the surface and subsurface composition of Eros. Mission controllers at the Johns Hopkins University Applied Physics Laboratory (APL) in Laurel, Md., have configured the instrument to begin collecting and recording this information. NEAR Mission Operations Manager Robert Nelson said the team is also sending commands to prevent the rest of the spacecraft from sending data to its onboard recorder, since the only reliable telemetry link is through NEAR Shoemaker's low-gain antenna. "Now that we have landed, collection and recovery of critical gamma-ray data is our primary objective," he said.
2100 GMT (4:00 p.m. EST)
1740 GMT (1:40 p.m. EST) The NEAR Shoemaker spacecraft's historic soft landing on asteroid 433 Eros Feb. 12 turned out to be a mission planner's dream - providing NEAR team members with more scientific and engineering information than they ever expected from the carefully designed series of descent maneuvers. "We put the first priority on getting high-resolution images of the surface and the second on putting the spacecraft down safely - and we got both," says NEAR Mission Director Dr. Robert Farquhar of the Johns Hopkins University Applied Physics Laboratory in Laurel, Md., which manages the Near Earth Asteroid Rendezvous (NEAR) mission for NASA. "This could not have worked out better." Two days after a set of five de-orbit and braking maneuvers brought it to the surface of Eros, NEAR Shoemaker is still communicating with the NEAR team at the Applied Physics Lab. The spacecraft gently touched down at 3:01:52 p.m. EST on Monday, ending a journey of more than 2 billion miles (3.2 billion kilometers) and a full year in orbit around the large space rock. Yesterday the NEAR mission operations team disabled a redundant engine firing that would have been activated had it been necessary to adjust the spacecraft's orientation in order to receive telemetry from it. But because NEAR Shoemaker landed with such a favorable orientation, and telemetry has already been received, it was no longer necessary to move the spacecraft from its resting place. Mission operators say the touchdown speed of less than 4 miles per hour (between 1.5 and 1.8 meters per second) may have been one of the slowest planetary landings in history. They also have a better picture of what happened in the moments after the landing: What they originally thought was the spacecraft bouncing may have been little more than short hop or "jiggle" on the surface; the thrusters were still firing when the craft hit the surface, but cut off on impact; and NEAR Shoemaker came down only about 650 feet (200 meters) from the projected landing site. "It essentially confirmed that all the mathematical models we proposed for a controlled descent would work," says Dr. Bobby Williams, NEAR navigation team leader at NASA's Jet Propulsion Laboratory. "You never know if they'll work until you test them, and this was like our laboratory. The spacecraft did what we expected it to do, and everyone's real happy about that." NEAR Shoemaker snapped 69 detailed pictures during the final three miles (five kilometers) of its descent, the highest resolution images ever obtained of an asteroid. The camera delivered clear pictures from as close as 394 feet (120 meters) showing features as small as one centimeter across. The images also included several things that piqued the curiosity of NEAR scientists, such as fractured boulders, a football-field sized crater filled with dust, and a mysterious area where the surface appears to have collapsed. "These spectacular images have started to answer the many questions we had about Eros," says Dr. Joseph Veverka, NEAR imaging team leader from Cornell University in Ithaca, N.Y., "but they also revealed new mysteries that we will explore for years to come." NEAR Shoemaker launched on Feb. 17, 1996 - the first in NASA's Discovery Program of low-cost, scientifically focused planetary missions - and became the first spacecraft to orbit an asteroid on Feb. 14, 2000. The car-sized spacecraft gathered 10 times more data during its orbit than originally planned, and completed all the mission's science goals before Monday's controlled descent. "NEAR has raised the bar," says Dr. Stamatios M. Krimigis, head of the Applied Physics Laboratory's Space Department. "The Laboratory is very proud to manage such a successful mission and work with such a strong team of partners from industry, government and other universities. This team had no weak links - not only did we deliver a spacecraft in 26 months, we were ready to launch a month early, and that efficiency continued through five years of operations. This is what the Discovery Program is designed to do."
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TUESDAY, FEBRUARY 13, 2001 We will provide a live streaming video broadcast of the briefing and provide updates on this page as details become available. Meanwhile, a statement released from Johns Hopkins University Applied Physics Laboratory on Tuesday said the NEAR Shoemaker mission operations team had disabled a redundant engine firing command that would have been activated if it became necessary to adjust the spacecraft's orientation in order to receive telemetry from the ground. But because NEAR Shoemaker landed with a favorable orientation, and telemetry has already been received, it is no longer necessary to move the spacecraft from its resting-place on the surface of Eros.s
1945 GMT (2:45 p.m. EST)
MONDAY, FEBRUARY 12, 2001 NASA's Deep Space Network -- a collection of powerful communications antennas around the world -- have been able to successfully "lock on" to NEAR Shoemaker. This is an improvement over the simple beacon signal that was heard at the time of landing. There has not been any telemetry transmission from the craft's systems, however. The DSN plans to continue monitoring the spacecraft until Wednesday when NEAR Shoemaker's remarkable mission officially ends. There was speculation earlier today about NEAR Shoemaker performing one final feat -- launching from the surface of Eros. But there are currently no plans to do so. "We are down and happy and expect to stay that way," project spokeswoman Helen Worth says. Also on Wednesday there will be a wrap-up news conference with project officials and scientists. We will cover it live!
2200 GMT (5:00 p.m. EST)
2125 GMT (4:25 p.m. EST) The mission has two days remaining on the Deep Space Network tracking system to receive data from the probe before the 5-year voyage of NEAR Shoemaker officially concludes.
2030 GMT (3:30 p.m. EST) We will pause our coverage now, and will provide further information as it becomes available.
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2010 GMT (3:10 p.m. EST) And on Wednesday, officials will hold a post-landing news conference, which we will cover live.
2006 GMT (3:06 p.m. EST) NASA had said there was less a one-percent chance of contacting the probe upon landing.
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1958 GMT (2:58 p.m. EST) The camera will now provide blurring photos, along with the craft's laser ranging instrument giving range measurements and Doppler tracking to determine when NEAR Shoemaker touches down.
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1901 GMT (2:01 p.m. EST) Mission controllers also report the probe has been oriented for the upcoming braking burn now 15 minutes away. There are no problems being reported as NEAR heads for its impact on Eros.
1840 GMT (1:40 p.m. EST)
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1809 GMT (1:09 p.m. EST) Meanwhile, the navigation team is converging on a 16-minute timing update that will be uplinked to the craft. This will shift the spacecraft's onboard timing sequence for the upcoming maneuvers based upon imagery showing NEAR's position following the de-orbit burn this morning.
1757 GMT (12:57 p.m. EST)
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1750 GMT (12:50 p.m. EST) The difference between the craft's location as predicated vs. the actual status following the de-orbit burn is currently just 6 seconds, which is reported as "good" by controllers. Further pictures will examined before mission control decides to adjust the timing.
MONDAY, FEBRUARY 12, 2001
1728 GMT (12:28 p.m. EST)
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1605 GMT (11:05 a.m. EST) The next thruster firing is expected around 2:16 p.m. EST (1916 GMT) when the first of four braking maneuvers will occur to slow NEAR's descent. Our continuous live coverage of the landing will begin at 1:30 p.m. EST (1830 GMT).
1532 GMT (10:32 a.m. EST) It will be a little while yet before mission controllers can confirm the burn occurred and was performed correctly. Mission navigators plan to examine images taken by NEAR Shoemaker after this maneuver to calculate the spacecraft's location and altitude, and set the timing on the satellite for the final thruster firings upcoming in the next couple of hours.
0501 GMT (12:01 a.m. EST) Launched on February 17, 1996 and orbiting Eros since February 14, 2000, the 5-year, 2-billion mile voyage of NEAR Shoemaker is wrapping up because the project is out of money and the probe's fuel reserve is almost gone. "We've been having a lot of fun over the last few years and we've fulfilled all the primary science goals of the mission. But all good things must come to an end, and the mission is scheduled to end (today)," said Dr. Robert Farquhar, the NEAR mission director at Johns Hopkins University Applied Physics Laboratory. Officials decided to attempt the first-ever asteroid landing in an effort to collect "bonus" science by capturing pictures of the ancient space rock with more detail than NEAR Shoemaker has been able to see from its higher orbital perch. And the hoped-for "controlled descent" will give ground controllers a challenging opportunity to see if they can land the satellite -- even though it wasn't designed to do so -- now that it has finished its useful life. "We're trying to find some way that we can end the mission on a high note, and we've come up with a way to do some bonus science, and also do some things with the spacecraft that have never been done before," Farquhar said. "Of course, when you try to do something like this there is always a little risk involved. But since we're trying to get bonus science and the primary goals have been satisfied, in my view, the only risk is not taking one at this point in the mission." Scientists hope the close-up pictures will be 5 to 10 times better than those collected so far, with the craft snapping about two images every minute during the descent and beaming them back to Earth in almost real time. "The secondary goal is to try to impact on the surface in a relatively soft way -- a soft landing -- about somewhere between 1 to 3 meters per second, which is about 2 to 7 miles per hour," Farquhar explained. "Now 7 miles per hour may not sound very fast, but I have personal experience with this kind of velocity. When I was in the paratroopers and we were jumping with World War 2 parachutes you would hit the ground at about 7 miles per hour if after swinging back and forth, so I know it's a fairly hard landing." Farquhar describes today's descent: "We are going to de-orbit with the first engine burn about 4 1/2 hours before we would impact on the surface. As it comes down there is a kink in the orbit close to the surface; it takes about 4 hours to get there and not too much is happening, we're just drifting down. At that point, about 5 kilometers above the surface, is where we do our final controlled descent. "That first burn, which I call brake number one, lasts about 3 minutes and is followed a bit later by another engine burn, brake two, which takes about 5 minutes, then another one that lasts 6 minutes, then a final one at about 4 minutes. "You can see we're doing a whole series of these engine burns and we've never done this before on the mission. So this is rather complicated, but I have full confidence that we have very experienced teams both at the Applied Physics Laboratory and the Jet Propulsion Laboratory that will be in charge of planning and implementing this. "The engines will fire and we come out of orbit; the sun is facing the right side of the solar panels and we're getting power. The thrusters fire as it gets closer; we do a roll to position ourselves properly for the final engine firing. "All the way down we stay on the high-gain antenna; it points toward Earth, and about 20 degrees off of that is the sun, so were getting full solar power on the panels on the way down, and the imager is pointing down. "When the spacecraft actually hits it could roll, or we could go into what we call the ostrich mode (tipped over on its top). We don't want to do that because it's hard to communicate with it. We are going to try to communicate with the low-gain antenna, but the chances of contacting it are probably less than one percent." The satellite was never meant to land and the odds of successfully receiving communications from the craft once on Eros are extremely remote. "The unknown nature of the surface makes it hard to predict what will happen to the spacecraft, especially since it wasn't designed to land. The most we can hope for is a beacon from NEAR Shoemaker that says it's still operating (on the surface)," Farquhar said. NEAR Shoemaker descent is scheduled to start at 10:31 a.m. EST (1531 GMT) with a maneuver moving it out of its current orbit 22 miles (35 kilometers). Touchdown is expected at 3:04 p.m. EST (2004 GMT) on the surface of Eros more than 196 million miles (316 million kilometers) from Earth. The planned landing site is the outer edge of the saddle-shaped depression called Himeros. The last clear pictures from the telescopic camera, taken in the final minutes before landing from approximately 1,650 feet (500 meters), could show surface features as small as four inches (10 centimeters) across. "NEAR Shoemaker has set a high standard for low-cost planetary exploration," said Dr. Edward Weiler, Associate Administrator for Space Science at NASA Headquarters, Washington, D.C. "This mission has provided answers to a range of fundamental science questions, and it has excited the public with its exploration and great images. The team at Johns Hopkins University Applied Physics Laboratory and its many partner institutions are to be congratulated for achieving this historic first in space exploration." "If you're not thrilled by the science and the basic exploration we accomplished, and you ask why we spent $223 million on this program, which is about a dollar per American over the life of the mission, let me tell you why it might be important," Weiler told reporters at a recent news conference. "This marks the first time we really began the in-depth reconnaissance of the so-called class of asteroids, near-Earth objects. These are objects that in the past have caused some bad days for species on the Earth, namely the dinosaurs. "We are not the agency that has the responsibility for protecting the Earth, but we do consider it a responsibility to learn as much as we can about these objects, and what you're going to hear today is the beginning of that process. During its mission, according to NASA, NEAR Shoemaker gathered 10 times more data than originally planned. The data include a detailed shape model culled from more than 11 million laser pulses; radar and laser data on Eros' weak gravity and solid but cracked interior; X-ray, gamma-ray and infrared readings on its composition and spectral properties; and about 160,000 images covering all of the 21-mile-long asteroid's bouldered, cratered, dusty terrain. Spaceflight Now will have continuing live updates throughout the day on Monday during the historic descent on this page. We will also provide a streaming video Webcast of the mission control room.
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