[meteorite-list] The Opportunity Rover Has Its Eye on Martian Bedrock
From: Ron Baalke <baalke_at_meteoritecentral.com>
Date: Thu Apr 22 10:31:19 2004 Message-ID: <200402021559.HAA09068_at_zagami.jpl.nasa.gov> http://www.aviationnow.com/avnow/news/channel_awst_story.jsp?id=news/02024top.xml The Opportunity Rover Has Its Eye on Martian Bedrock By Craig Covault Aviation Week & Space Technology February 1, 2004 Sobered by a near-death experience with Spirit and still reeling from the landing of Opportunity at a location with scientific potential "beyond their wildest dreams," Mars Exploration Rover controllers are this week preparing to restart science operations with the first rover, while 6,000 mi. away they plan to drive Opportunity onto the Martian surface for a first taste of the bizarre terrain and soil at its Meridiani Planum landing site. Rover drivers here will then steer Opportunity onto Martian bedrock--possibly 3-4 billion years old--that researchers rate as one of the best finds ever made by the storied Jet Propulsion Laboratory planetary exploration team. The chance landing of a scientifically potent rover within 25 ft. of exposed Martian bedrock ranks as significant in the annuals of JPL as the 1979 Voyager 1 discovery of volcanoes on Jupiter's moon Io, said Larry Soderblom of the U.S. Geological Survey, one of the world's most experienced planetary scientists. This is because bedrock, normally deeply buried but here remarkably exposed by meteorite impact, is a fundamental planetary building block formed directly where it is found. The rover's ability to sample it will allow scientists to make fundamental judgments about Martian processes, rather than infer these processes from material deposited perhaps hundreds of miles from where it was formed. The Rover's powerful Panoramic Camera already shows the rocks have intricate layers as if formed by sedimentary deposits in water, a possibility given the strong potential for past water at Meridiani. But volcanic ash also remains a viable hypothesis. The Mini-TES infrared spectrometer will begin to provide compositional data on the outcrop this week, and during the next month the rover will park over the site to use its Alliance Spacesystems Inc. arm carrying spectrometers and a microscopic imager to decipher the nature of the bedrock better than a lesser equipped human geologist on Earth could. "We are going to beat on it with everything we have got," said Steve Squyres, MER principal investigator from Cornell University. Rock layers are like the pages in a history book, and Opportunity has now found that book on Mars, said Andrew Knoll, a science team member from Harvard University. In the span of just a month, human exploration of the solar system has changed fundamentally. With two new surface rovers and the highly capable European Mars Express orbiting Mars along with two other U.S. orbiters, suddenly there are several hundred people--both U.S. and European--literally working "on Mars." And that is especially evident here at JPL where the MER science and operations team is split into distinct groups, about half working on the Spirit rover on Gusev Crater time, the other half working with a 12-hr. time-zone difference for Meridiani. In the meantime, hundreds of support personnel for both missions are working on Pasadena time. It can be 1 p.m. PST in Pasadena, 5 p.m. Gusev time and 5 a.m. Meridiani time. People passing in the congenial central JPL plaza will extend both "good morning" and "good evening" greetings simultaneously, when it's neither here at JPL. THE TWO SURFACE teams are working out of different floors of the Building 264 Surface Mission Support Area (SMSA) here. Controllers for both rovers and the Gusev science team operate out of the fourth floor, colored red, while the Opportunity/Meridiani science team is on the fifth floor, colored blue, so managers and scientists can remember which Martian time zone they are in--critical for rover decision timing. This editor visited the SMSA on Jan. 29 as it was linked to Spirit at Gusev just as the team reinitiated Pancam science operations. I then observed the Spirit anomaly team led by Jennifer Trosper meeting in an adjoining room as they decided that the tactical science operations process for Spirit could be reinitiated on Feb. 1, its 29th day on Mars. It is a remarkable comeback from a week ago when Ed Weiler, head of Space Science for NASA in Washington, said he feared he was returning to JPL "for a funeral" for Spirit (see story p. 36). Meanwhile at Meridiani, Opportunity was being put through multiple milestones related to standup and wheel deployment and alignment. But that was being done cautiously. "We are trying to make sure we are not accidentally duplicating what caused Spirit to have its problems," said Jim Erickson, Opportunity mission manager. Opportunity had been planned to roll off its forward ramp directly facing the bedrock as early as Jan. 31, its eighth Martian day (Sol) on the surface. The Opportunity team was working one rover problem unrelated to standup and roll-off. A thermostat in the elbow joint of its manipulator arm was continuously cycling heater power at that location on and off. A periodic drain of up to 15 watts, which if it were to persist for 3-4 months from now, could limit mission life, depending upon solar array dust buildup. Of the two rover landing sites, Opportunity's Meridiani site on the equator about 0 deg. Long. was the highest priority. This is because of the detection there by Mars Global Surveyor (MGS) of a formation the size of Oklahoma of gray hematite, an iron oxide mineral that normally indicates the past presence of water. Since the overall MER missions are to study the permanency of water as habitats for ancient life forms, this was the highest priority target. To get to the 46 X 4-mi. landing ellipse required extremely precise work by the MER Navigation Team led by Louis D'Amario. Launched on July 7, nearly a month after Spirit, Opportunity flew a shorter 280-million-mi. circuit to Mars compared with Spirit's 300-million-mi. trajectory. But Opportunity intercepted the planet at about 124 million mi. from earth--about 20 million mi. farther away than when Spirit landed. This resulted in a one-way light time signal travel time to Earth of 11 min. for Opportunity during landing compared with 9.5 min. for Spirit's descent. The effect the extra difference had on signal strength and viewing angle for the Deep Space Network antennas at Goldstone, Calif., and Canberra, Australia, indicated that maintaining signal lock at landing would be more difficult than for Spirit. But this proved not to be the case. On Jan. 17, JPL commanded a third and final cruise stage trajectory correction burn of only 0.25 mph. using 120 grams of propellant. This was just the maximum amount of energy contained in your average hamburger, said Erickson. But it had the effect of changing the surface arrival location by 380 km. (224 mi.) and adjusting arrival time by 36 sec. The maneuver targeted Opportunity about one third of the way down the 46-mi.-long landing ellipse with a touchdown planned slightly north of center, based on intensive overhead imaging of the site. A 10-15-km. downrange error was also likely, given atmospheric characteristics at Meridiani, a forecast that proved close to accurate. WEATHER MONITORING of Meridiani was absolutely critical to final entry, descent and landing (EDL) updates, said Rob Manning, EDL manager. This monitoring was done by JPL and Goddard Space Flight Center teams using MGS and other data. A critical parameter was the dust level in the atmosphere over the landing site, given that a dust storm had swept through the area in December. The dust affected atmospheric heating and therefore reduced atmospheric density--a critical factor for calculating performance of the 47-ft.-dia. nylon Pioneer parachute. This was especially critical at Meridiani, the highest Martian landing site ever attempted--about 1,500 ft. higher than Gusev. The dust, in effect, forced the chute to function for a time in a higher, thinner atmosphere than at Gusev. These calculations resulted in updating Opportunity's computer to open the chute 2 sec. earlier than planned--a 1-2% difference in chute performance that would equate to 5% extra margin at the deceleration rocket firing and airbag-release altitude, Manning said. In the days before landing, these calculations were verified by thousands of computer simulations using expected atmospheric density and various dispersions. The plunge to the surface by Opportunity, encased in its aeroshell, took it at night directly over Valles Marineris, the solar system's largest canyon, and just abeam of Olympus Mons, the solar system's largest volcano. The vehicle heat shield pointed into the direction of flight slammed into the atmosphere at 12,187 mph. and 73 mi. altitude about 440 mi. from the landing site to begin its 6-min. descent. The chute deployed as planned with the vehicle still supersonic above 25,000 ft. At 5.4-km. altitude, with the lander now hanging below the chute on a bridle, the critical landing radar altimeter locked up on the surface, enabling the vehicle to compute retrorocket ignition at about 121 meters (397 ft.) altitude. At about 2 km. the first of three images was taken by the Descent Image Motion Estimation Subsystem (Dimes) camera as input for any lateral velocity corrections needed. Unlike on Spirit, none was needed. Initial data showed that as the lander hung on its 65-ft. bridle under the parachute, it had a drift of 10 meters/sec. north combined with a 2.7 meter/sec. component to the west. The three 1,124-lb. thrust Alliant retrorockets fired for 2.8 sec., providing 25 meter/sec. deceleration. This also provided 7.7 meters/sec. of southern velocity that tended to cancel out the other two values as the bridle holding the airbags was separated at about 12-meter altitude. The lander experienced only about 3g at touchdown and is designed for up to 40. The vehicle bounced, all the while transmitting data to Earth in the western sky. It was during these bounces that the lander plopped fortuitously into a shallow crater where it dribbled like a basketball, then rolled like a marble in a soup bowl, coming to rest in the center of the 20-ft. wide depression. That was extremely good luck because the object that created the crater had also excavated the bedrock. The airbag's bouncing also proved to be an excellent first science experiment, leaving such detailed impressions that the airbag stitches sewn into the bag by the staff at ILC in Dover, Del., have now been sharply imprinted on Mars. The vehicle came to rest 24 km. downrange from its formal target area, but in a more scientifically rich spot than had it been on target. The lander settled on a side petal, which also was fortunate, because unlike with Spirit, it allowed the airbags on the preferred forward drive-off direction to be fully reeled in before the rover was flipped onto its base petal. So far the crater in which the spacecraft landed shows signs of what geologists expected--that if hematite is there, it is on top of a 200-300-meter stack of sedimentary deposits, visible when excavated by erosion or meteorite impact. The question is whether the hematite was formed by water or volcanic-related processes. As expected, the site, with a reflectance ratio of only 10-15%, has the darkest material ever seen on Mars--totally unlike the two Viking, Pathfinder or Spirit sites (see front cover). A FIRST ORDER of business this week is to use the instruments on the arm to look for hematite in the soil. But Squyres believes the rover will have to drive out of the crater to more likely find it on the slightly higher terrain. That will come in a month or so when this second rover in effect makes its second landing on Mars by driving out of the crater and looking around at what again will be a whole new world not clearly visible from inside the 3-ft.-deep depression. At JPL I also visited their In Situ Instrument Laboratory where an engineering rover was climbing a dirt slope similar to the crater where Opportunity landed as a technician carefully monitored rover angles. The soil, as first indicated by the airbag impact, is an extra surprise that will keep the rover almost as busy as the bedrock. Soderblom noted that when disturbed by the airbags it looks as if it has become a nicely sculptured "Japanese rock garden." "The soil and physical properties group is going wild. . . . Everybody is having a wonderful time arguing about it," Squyres said. "When you look at this soil and you try and interpret what the heck you are looking at, there are two schools of thought," he said. "One, that we have soil with two distinct components. That there are coarse grayish grains and much finer reddish stuff. And when the airbags hit it and push the coarse gray grains into the red stuff, then all you see is red stuff. The other idea is that we have aggregates of grains that appear grayish but when impacted they somehow turn red." But researchers are also beginning to see pebbles with multiple colors. What they may be, nobody has figured out yet. And there are some innovative ideas on what could cause such a unique powdery soil that changes character when compressed. One idea is a "flash water" phenomenon where liquid water may have existed briefly on the surface--perhaps just a second or two in some wide area event, which altered electrical charges in the soil. Received on Mon 02 Feb 2004 10:59:36 AM PST |
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