ASTR 1210 (O'Connell) Study Guide
17. FROM THE SURFACE OF MARS
View of the Martian surface from the Mars
Pathfinder lander (1997)
This Guide continues the discussion of Mars begun in
Guide 16 and covers the five
successful Martian lander missions and the tantalizing but
still marginal evidence for an early biosphere on Mars.
F. Viking Lander Missions (1976)
- Viking was the most ambitious robot space mission to that time.
It consisted of two separate, nearly identical spacecraft, each
containing an orbiter and a lander component. The orbiters mapped
some 99% of Martian surface
- The Viking landers were very sophisticated experiments (though they
did not "rove"), taking weather & soil samples at two
sites and analyzing these with laboratory precision.
- Viking's primary goal was to perform a series
tests for organisms in the Martian soil. The basic technique for
the three experiments other than the mass spectrometer was to expose
Martian soil to nutrients or gases labeled with radioactive tracers.
If these were utilized by microorganisms in the soil, that could be
detected by subsequent tests.
- Test for the presence of organic molecules using a mass spectrometer
- Test for metabolism (solid ===> gas)
- Test for photosynthesis (gas ===> solid)
- Test for respiration (gas ===> gas)
- Iron-rich minerals; iron oxides (rust) produce the red soil
- No organic molecules detected by the mass spectrometer
- A positive result from the "labeled release" metabolism
experiment, which detected tagged carbon dioxide emitted from the
soil. But this result was ultimately attributed to the "strange"
chemistry of iron-oxide rich material, not to biological activity.
over the interpretation here, and some scientists argue that the
Viking experiments did indeed provide evidence of
microorganisms on Mars.
- Soil samples were taken only about 10-cm deep. They may not be
representative because the surface may be sterilized by solar UV.
Artist's concept of Mars Pathfinder Rover
G. Mars Pathfinder Mission (1997)
- Twenty years after Viking, MPF was the first of a new series of
moderate-cost Martian orbiters and landers intended to culminate in
robot missions to return soil & rock samples to Earth.
- Novel airbag cushions
permitted landing without usual powerful (& heavy) retro-rockets. Here
is an animation of how these work.
- MPF studied the atmosphere, soil, and rocks on Ares Vallis,
a floodplain region.
- MPF carried the first robot
"rover" to sample rocks/soil within a few 10's of yards from
- The rover used an Alpha-Proton-X-ray Spectrometer to determine
the mineral content of rocks by firing "alpha particles" (the nuclei
of helium atoms) into the rocks and detecting the resulting emitted
- Results: pebble & rock shapes give strong evidence
for catastrophic floods in the distant past but only wind
erosion (without water) since those. Some rocks appear to be
sedimentary, forming during a long "wet-era" with stable liquid water
on surface. Most of the rocks are "andesites"---lava deposited molten
but allowed to cool slowly or re-heated at a later time; similar to
terrestrial rocks from Iceland. From precision measurements of
Pathfinder's radio signal, there is dynamical evidence for an iron
core in the Martian interior, implying (as expected) a hot,
geologically active phase at early times.
H. Mars Exploration Rover Mission (2004)
- The MER mission consisted of two landers with rovers, "Spirit" and
"Opportunity," launched in mid-2003, which landed on Mars in January
Click here for QuickTime
animations of the launch and landing sequences of the MER mission.
- Landing sites were both chosen for their potential to demonstrate
the presence of water on Mars in the past: Gusev Crater (Spirit) is a possible ancient lake bed;
Meridiani Planum (Opportunity) is a plain with signs
of a water-deposited mineral (hematite).
- The rovers were very robust, and traveled (slowly!) for large
distances over the surface, a combined total of 13 miles. Opportunity
spent almost two years exploring the Victoria crater and six months
exploring Endurance crater.
- Both sites have yielded strong evidence of a watery past
on Mars by detecting traces of
specific minerals, such as "jarosite," "goethite,"
blueberries," which are only produced in a water-rich environment,
and layering which is expected for sedimentary rocks laid down at
the edge of a lake or ocean. Rover "Spirit" also discovered deposits
of silica, the product of igneous rocks exposed to hot water or steam,
which is considered an excellent medium to host microbial life.
The wall of Victoria Crater as seen by the Opportunity Rover
I. Mars Phoenix Lander (2008)
- The Phoenix site is closer to the north Martian pole than any other
lander. Phoenix did not carry a rover but was able to sample the soil and
determine its chemical composition and change of properties with temperature.
By testing for water vapor and watching changes as temperatures rose
above the melting point of water ice, Phoenix confirmed the presence of
large amounts of water frozen in the Martian soil. Liquid droplets,
probably water, formed and then evaporated from Phoenix's landing
J. Mars Science Laboratory/Curiosity Lander (2012)
- The MSL rover Curiosity, which successfully landed in
August 2012, is a one-ton roving laboratory, the most ambitious
experiment yet sent to Mars. Getting it safely to ground
involved a complex
set of equipment and maneuvers.
- Curiosity carries the most elaborate set
equipment yet sent to Mars to study the geology and
- Curiosity landed in Gale Crater and will study the sedimentary
deposits on the slope of "Mount Sharp" in the middle of the crater.
The unusual geology of Gale Crater arises from the fact that after the
crater was formed by a meteoroid impact, it was flooded with
sedimentary debris. The outer parts of the crater were subjected to
weathering by winds, which left a sedimentary mountain 18,000 feet
high in its center.
- In its early explorations, Curiosity has used a drill to remove
samples from inside a Martian rock lying in a ancient stream bed.
Analysis with its on-board laboratory detected the presence of
clays, sulfates, and other materials favorable to primitive lifeforms.
The water content of soil minerals is estimated to be about 2%, which
is substantial. Curiosity has ruled out a significant component
of methane (CH4) in the Martian atmosphere, which
would be expected if certain types of bacteria thrived in the soil.
K. "SNC" Meteorites
- "SNC" meteorites are a rare class of meteorite (only 99 of 53000
fall in this group) found on Earth.
- By matching their composition to data from the Martian
landers, geologists realized that the SNC's
are fragments of the Martian surface, ejected
by asteroid impacts,
which have happened to travel to Earth and survive passage through the
- They are about 1 Byr old. (Typical meteorite remnants
of the solar nebula would be much older, at about 4.5 Byr.)
- Their Argon isotope ratios match results from the Viking and Curiosity
landers and are very different from Earth or Jupiter ratios, indicating
a major loss of atmospheric gases from Mars at some time in the past.
- Analysis of the SNC minerals shows that Mars was once
very wet, with a global water layer perhaps several 100 meters
deep. The SNC results support the
extensive imaging and other
evidence for massive water flows in the past on Mars.
L. Microscopic Life on Mars??
84001 is a SNC meteorite recovered from an
Antarctic meteorite field. It is over 3.5 Byr old
- It contains several features which are suggestive of the presence
of ancient microorganisms
- Carbonate inclusions. "PAH" molecules, which may imply
- Microfossils (0.0001 mm) (see image at right; click for
an enlarged view)
- The implication is that bacterial life may have existed on Mars
during the "wet era", 1-4 Byr ago
- But this interpretation is controversial.
See the Lunar & Planetary Institute web site for links
discussing various sides of the debate.
M. Martian Satellites
- Mars has two satellites: Phobos & Deimos, discovered in 1877.
- These are both small (10-17 mi) and irregular in shape.
- They are captured asteroids. Viking images of them afforded us our
first close-up view of asteroids.
N. Expeditions to Mars
Serious proposals for human expeditions to Mars have been around for
over 50 years. Many prelminary conceptual designs have been
considered (for details,
article). In January 2004, President Bush proposed a long term
commitment (20+ years) to a program that would send expeditions back
to the Moon and ultimately to Mars, but funding has never been
committed for a project of this scale.
Human space missions are much more costly than the robot craft we have
used for all previous studies of Mars because of the life support
systems needed (both during the trip and once on Mars' surface).
However, many people are eager to go---for both scientific and
personal reasons---and are exploring the various necessary
technologies. There is much discussion of "terraforming" Mars---i.e.
making it suitable for human colonies by releasing trapped water onto
its surface and generating oxygen for a breathable atmosphere.
Artist's concept of a human expedition to Valles Marinaris.
Reading for this lecture:
Study Guide 17
Bennett textbook, p. 206, Sec. 9.4.
Reading for next lecture:
H. G. Wells War of the Worlds
Study Guide 18
November 2013 by rwo
Text copyright © 1998-2013 Robert W. O'Connell. All
rights reserved. These notes are intended for the private,
noncommercial use of students enrolled in Astronomy 1210 at the
University of Virginia.