Extreme Planet Takes Its Toll on the Mars Rovers
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baalke@earthlink.net - 14 Jun 2007 16:40 GMT http://marsrovers.jpl.nasa.gov/spotlight/20070612.html
Extreme Planet Takes Its Toll Jet Propulsion Laboratory June 12, 2007
Like Sun Belt retirees who complain about cold weather, NASA's Mars rovers are becoming less tolerant of temperature changes with age.
Near the martian equator, where the rovers are exploring opposite sides of the red planet, highs and lows make Earth temperatures look downright tropical. Temperatures often differ by more than 100 degrees Celsius. That's a change of 180 degrees Fahrenheit -- the equivalent of having the temperature drop from a high of 70 degrees F. at midday to minus 110 degrees F. the same night. That would be like going from a beach in Hawaii to the South Pole in mid-winter ... every day!
Air Temperatures -- Spirit Temperatures in the shade for Spirit ranged from highs of about 35 degrees C. (95 degrees F.) in summer to lows of -90 degrees C. (-130 degrees F.) in winter. In the background is a panoramic camera image of sunset <http://marsrovers.jpl.nasa.gov/gallery/press/spirit/ 20050610a.html> on Mars. Image courtesy: NASA/JPL-Caltech/Cornell/NMMNH
[chart] This chart shows degrees C. on the left-hand axis and degrees F. on the right-hand axis. The horizontal x-axis at the bottom shows the number of sols, or Martian days, on the surface. <http://marsrovers.jpl.nasa.gov/images/ 20070612/20070612_Spirit_LFHzczm_plot.jpg>
Extreme Planet
Though both rovers are exploring Mars well beyond their initial 90-day missions, electrical connections and moving parts are showing signs of temperature-related fatigue.
"Every day we have a huge thermal cycle," notes Jake Matijevic, chief of the rover engineering team. "That causes the solder in electrical connections to expand and contract until it breaks."
Air Temperatures -- Opportunity Temperatures in the shade for Opportunity ranged from about 30 degrees C. (86 degrees F.) in summer to minus 80 degrees C. (-112 degrees F.) in winter. The background panorama shows a false-color view of dunes <http://photojournal.jpl.nasa.gov/catalog/PIA06753> at the bottom of Endurance Crater. Credit: NASA/JPL-Caltech/Cornell/NMMNH
[chart] This chart shows degrees C. on the left axis and degrees F. on the right-hand axis. The horizontal x-axis at the bottom shows the number of sols, or Martian days, on the surface. <http://marsrovers.jpl.nasa.gov/images/ 20070612/20070612_Opportunity_LFHzczm_plot.jpg>
Seasonal Change
During their exploration of Mars, the rovers have recorded temperatures ranging from midday highs of about 35 degrees C. (95 degrees F.) in spring and summer to nighttime lows of about minus 110 degrees C. (minus 166 degrees F.) in winter. Spirit has experienced greater swings in temperature because its location is farther from the martian equator, which puts it seasonally closer to or farther from the Sun than Opportunity.
Solar Panel Temperatures -- Spirit Summer temperatures on Spirit's solar arrays have reached summertime highs of more than 30 degrees C. and winter lows of about minus 110 degrees C. The image in the background shows the rover's view of "Husband Hill" <http://photojournal.jpl.nasa.gov/catalog/PIA01907> after cliimbing down from the top. Image courtesy: NASA/JPL-Caltech/Cornell/NMMNH
[chart] This chart shows degrees C. on the left-hand axis and degrees F. on the right-hand axis. The horizontal x-axis at the bottom shows the number of sols, or Martian days, on the surface. <http://marsrovers.jpl.nasa.gov/images/ 20070612/20070612_Spirit_SA4_plot_2.jpg>
Three Years of Data
Rover engineer Dan Porter has been tracking temperatures recorded by 50 or so sensors on each of the rovers since shortly after they landed on Mars in January 2004. The results are not only of interest to scientists, they're a favorite of human audiences as well.
"People ask about this all the time," says New Mexico geologist Larry Crumpler, a member of the Mars rover science team who created the charts showing monthly average temperatures superimposed on panoramic-camera images from each of the rovers. "These plots of daily temperature are destined to become an important part of all my public outreach talks."
Solar Panel Temperatures -- Opportunity Nighttime temperatures on Opportunity's solar panels fell within a fairly stable range of about minus 90 degrees C. (-130 degrees F.) to minus 100 degrees C. (-148 degrees F.) most nights. Daytime temperatures reached a high of around 30 degrees C. (86 degrees F.) in the summer. In the background of the chart is an outcrop known as "Cape St. Mary" <http://pancam.astro.cornell.edu/pancam_instrument/ 1037B_bottomless_bay.html> in Victoria Crater. Credit: NASA/JPL-Caltech/Cornell/NMMNH
[chart] This chart shows degrees C. on the left-hand axis and degrees F. on the right-hand axis. The horizontal x-axis at the bottom shows the number of sols, or Martian days, on Mars. <http://marsrovers.jpl.nasa.gov/images/ 20070612/20070612_Opportunity_SA4_plot.jpg>
Cold vs. Colder
Just as on Earth, temperatures on Mars are not uniform everywhere. Objects exposed to direct sunlight are apt to be warmer than those in the shade. Some objects retain heat better than others. A source of relative warmth on Mars is rocky terrain, because it retains heat better than sandy terrain.
A solar panel is sort of like a "warm wall in mid-winter," says Crumpler. Components beneath the solar panels, such as the hazard avoidance cameras, are closer in temperature to the martian air. Unlike Earth, Mars does not have a thick, atmospheric blanket to seal in warmth by night or minimize the Sun's heat by day.
Colder in the Shade On Mars as on Earth, surfaces shaded from sunlight are more likely to develop a veneer of frost. This pair of images taken by the Compact Reconnaissance Imaging Spectrometer for Mars, on board the Mars Reconnaissance Orbiter, shows water frost in shaded areas and carbon dioxide frost in only the coldest of those. Image courtesy: NASA/JPL-Caltech/JHU APL
[Image] The top image of this stacked pair of images is a false-color image showing white frost covering alluvial fans beneath a cliff. The bottom image is an infrared view of the same surfaces, showing blue areas covered by frozen water vapor interspersed with aqua patches covered by an even colder coating of frozen carbon dioxide. <http://photojournal.jpl.nasa.gov/catalog/PIA09101>
Wear and Tear
Engineers have traced stalls in a shoulder joint on Opportunity's robotic arm to a broken electrical wire. The shoulder motor has experienced greater temperature swings than other parts because of its location beside a heater that has been stuck in the "on" position since shortly after landing.
Notes Matijevic, "Our theory is that one of the wires in the electrical coil broke free and disabled the motor."
Frost on Mars Rover Opportunity discovered frost <http://marsrovers.jpl.nasa.gov/gallery/press/opportunity/ 20041213a.html> on the rover's calibration target in October 2004. Credit: NASA/JPL-Caltech/Cornell
[Image] This photo shows shiny black rocks shaped like masses of thick rope piled atop each other. In the distance are the rugged cliffs that make up the slopes of Kilauea, rising gently in elevation from right to left. <http://photojournal.jpl.nasa.gov/catalog/PIA07108>
Mechanical Problems
Extremely cold temperatures have also caused mechanical problems. Recently, Opportunity's right front wheel began drawing excess electrical current, reminiscent of Spirit's right front wheel in 2004. The demand for more electrical current suggests that the wheel motor is working harder than usual. Engineers suspect that, like motor oil that can't handle freezing temperatures on Earth, gelid lubricant failed to flow properly and caused Spirit's right front wheel to fail. This black-and-white orbital image shows circular sprays of lighter-colored rocks ejected from within craters onto darker background materials. <http://photojournal.jpl.nasa.gov/catalog/PIA03739>
Warmer vs. Colder
[Image} NASA's Mars Odyssey spacecraft mapped surface changes in nighttime temperatures on Mars. Lighter areas are warmer than darker areas and correspond to rock exposures.
Image courtesy: NASA/JPL-Caltech/ASU
Adjusting Expectations
Rover drivers have compensated for Spirit's stuck wheel by driving on the other five wheels. They have compensated for Opportunity's stalled shoulder joint by unstowing it before going to sleep at night. This way, if the motor fails during the night, when temperatures are at their lowest, they would still have limited use of the arm by operating the remaining working joints. Each rover has lost a few temperature sensors as well, while dozens more continue operating.
[Image] This black-and-white image shows a narrow column of light dust rising from a dark Martian surface. <http://photojournal.jpl.nasa.gov/catalog/PIA09260>
Warm Air Currents
[Image] Dust devils form when the surface heats up and creates warm air that rises in a spinning column. Spirit produced a movie <http://marsrovers.jpl.nasa.gov/gallery/press/spirit/20070412a.html> of this dust devil in February, 2007.
Image courtesy: NASA/JPL-Caltech
Time Will Tell
"How long will it take for us to see other sorts of things related to temperature swings? We don't know," says Matijevic. "We know it matters over time, but we don't know how many of these swings we'll see before we lose a component.
"Meanwhile, we're applying for a fifth extended mission for both rovers."
Surface Frost
[Image] In the 1970s, NASA's Viking landers took images of seasonal ice coating rocks and soil on Mars. Image courtesy: NASA/JPL-Caltech
Robert Clark - 14 Jun 2007 18:49 GMT This page discusses that at the MER rover landing sites the maximum Summer-time air temperatures can exceed 30 C, 86 F, while the temperature swings from day to night reach a 100 C , 180 F, change:
Extreme Planet Takes Its Toll. June 12, 2007 Like Sun Belt retirees who complain about cold weather, NASA's Mars rovers are becoming less tolerant of temperature changes with age. http://marsrovers.jpl.nasa.gov/spotlight/20070612.html
On this same page is discussed the observations of frost on the Opportunity rover. It had been known for some time that daytime, Summer temperatures can exceed the melting point of water at equatorial locations on Mars but it was believed the equator was desiccated. We now have visual evidence that the equator on Mars is not desiccated, in addition to the GRS/HEND instrument readings on Mars Odyssey showing this. The errors of the report of "puddles" at the Opportunity rover site have been legitimately criticized. But the observation of frost on the Opportunity rover occurred 3 years ago. Is not the refusal to investigate the possibility of liquid water at the Opportunity site when the environmental conditions suggest it should be possible an even greater error of omission by the scientific community at large?
Bob Clark
Robert Clark - 10 Jul 2007 20:27 GMT > This page discusses that at the MER rover landing sites the maximum > Summer-time air temperatures can exceed 30 C, 86 F, while the [quoted text clipped - 22 lines] > > Bob Clark Linked below is a graph I use that shows the dates for solar longitude on Mars from 1997 to 2007. I copied this from some online report but now can't remember which one it was. Solar longitude tells the position of Mars in its orbit, 0?-90? is northern Spring; 90?-180? is northern Summer; 180?-270?, northern Autumn; and 270?-360?, northern Winter. It is notable that Spirit landed in January, 2004 at the end of the period that the HEND instrument on Mars Odyssey indicates is the highest period of H2O deposition, Ls=270?-330?, which is early to mid Summer in the southern hemisphere:
47 - EVIDENCE OF THE SEASONAL REDISTRIBUTION OF WATER IN THE SURFICIAL MARTIAN REGOLITH BASED ON ANALYSIS OF THE HEND MAPPING DATA. R.O. Kuzmin, E.V. Zabalueva, I.G. Mitrofanov, M.L.Litvak, A.V. Parshukov, V.Yu.Grin'kov, W. Boynton, R.S. Saunders. "As it well seen from fig.1b,c,d, two distinctive "hollows" of neutrons flux reduction have been appeared in the northern hemisphere during northern summer at Ls=130?-170? and in first half of northern winter at Ls=270?-330?, being extended from high to low latitudes. At that, later "hollow" (Ls=270?-330?) is characterized by much stronger reduction of the neutrons flux and it traces from northern polar region up to low latitudes in the southern hemisphere. The first "hollow" is related with periods of the northern middle summer, while the second one - with of the southern middle summer. In both case the residual polar caps serve as main source of the water in the Martian atmosphere." p. 2 http://www.geokhi.ru/~planetology/theses/47_kuzmin_et_al.pdf
This is important because shortly after landing the Spirit rover observed material that might have been liquid water related, the famous "magic carpet":
Mystery at Gusev Crater. By Leonard David Senior Space Writer posted: 01:35 pm ET 16 January 2004 "PASADENA, Calif. -- Scientists are puzzled about a patch of soil near the Mars rover Spirit lander that they now call "Magic Carpet". The intrigue has been stirred up by how soil behaved when the landers airbags scraped across the martian soil. That soil appears to have been peeled away." ... "Sand and brine? I think were seeing, already, preliminary evidence for a variety of materials, just within the soil," said David Des Marais, an astrobiologist from NASAs Ames Research Center. He is also a lead member of the long-term planning group that is charting future use of the Mars rovers, Spirit and the yet-to-land Opportunity. Finer grain material is seemingly globally uniform on Mars, Des Marais told SPACE.com. But then more coarse material is available locally too, he said. "That darker stuff thats beneath the fines is a step in that direction. This funny peeling thats occurred, he added, could be, as hypothesized, the result of very fine grain material. "But another thing that could do something like that, in my opinion, is a mixture of sand and brine," Des Marais explained." http://www.space.com/missionlaunches/spirit_gusev_040116.html
Another possibility for what it could be is clay, since both Spirit and Opportunity made detections of clays with the mini-TES instrument. Since we are coming into southern Summer perhaps the night time temperatures will be within the range that the rover can make some minimal movements. Geoffrey Landis explained the constraints on what the rover was allowed to do according to the Winter temperatures in his report on the detection of frost on Opportunity:
OBSERVATION OF FROST AT THE EQUATOR OF MARS BY THE OPPORTUNITY ROVER. Geoffrey A. Landis1 and the MER Athena Science Team, 1NASA John Glenn Research Center, 21000 Brookpark Road, mailstop 302-1, Cleveland OH 44135; ****@nasa.gov Lunar and Planetary Science XXXVIII (2007) http://www.lpi.usra.edu/meetings/lpsc2007/pdf/2423.pdf
This detection of frost was correlated to the observation of clouds over the rover site. It would be a good idea to estimate the time of evening the greatest deposition occurs according to when the nighttime clouds are densest. The idea now would be to emulate how the airbag retraction discovered the "magic carpet" material. The period of highest water/ice deposition at Ls=270?-330? occurs this year from July to October. We would try to lay down a large flat rock over an area around the time of day the airbags were laid down, and uncover the area around the same time of day the airbags were retracted. Ideally this flat rock or perhaps a shard of cemented sulfate would be as thin as possible to allow penetration of heat as happened with the airbag material to cause melting. Note also an important consideration often not mentioned about liquid water occurring in the low pressure on Mars is that an over cover of low porosity soil or a rock could supply sufficient over pressure to allow liquid water over a wider temperature range than normally happens on the Martian surface. This could well have been what happened with the airbags. Other things we might want to emulate is similar thermal inertia properties of the area we wanted to cover to that of the "magic carpet" area. Or we might want to use an area consisting of salts or sulfates so that it would absorb large amounts of water vapor. Still another consideration is that we might want to use areas that approximate the thermal properties of the solar panels on the rovers since that was where deposition occurred on Opportunity.
Bob Clark
Mars Solar Longitude Chart. http://uplink.space.com/attachments//745003-solarlongitudechartls_chartcompr2.JPG
Robert Clark - 14 Aug 2007 06:32 GMT Harry's face.
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: The BATF agent slammed Kimberly Katona, then several month
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