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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.
:   They did not announce who they were or why they were there, and no search
:   warrants were displayed. "When I asked if they had a search warrant, their
[quoted text clipped - 9 lines]
:   deliberately stomped to death a cherished Manx kitten, and kicked it under
:   a tree.

*   "1984", author George Orwell, 1949, ISBN 0-679-41739-7
*  
*   There was a gasp and thump behind Winston, and he received a violent
*   kick on the ankle which nearly flung him off balance.
*
*   One of the men had smashed his fist into Julia's solar plexus,
*   doubling her up like a pocket ruler. She was thrashing about
*   on the floor, fighting for breath.
*
*   Winston dared not turn his head by even a millimeter, but sometimes her
*   livid, gasping face came within the angle of his vision.

:   The BATF agent slammed Kimberly Katona, then several month
 
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