ASTR 1210, O'CONNELL. Study Guide 17 [Spring 2013]

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
- Click here for a Viking Project fact sheet.
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 of lab 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.
- Identify any organic molecules using a mass spectrometer
- Test for metabolism (solid ===> gas)
- Test for photosynthesis (gas ===> solid)
- Test for respiration (gas ===> gas)
Results:
- Iron-rich minerals; iron oxides (rust) produce the red soil color
- 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. There is still controversy over the interpretation here, and some scientists argue that Viking did indeed detect microorganisms on Mars.
- Soil samples were taken only about 10cm 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 lander.
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 X-rays.
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 2004.
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," and "hematite 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 struts.

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 of diagnostic equipment yet sent to Mars to study the geology and environment.
Curiosity landed in Gale Crater and will study the sedimentary deposits on the slope of "Mount Sharp" in the middle of the crater.
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.

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 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 atmosphere.
- They are about 1 Byr old. (Typical meteorite remnants of the solar nebula would be much older, at about 4.5 Byr.)
- Their isotope ratios match Viking results
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??

ALH 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 biosynthesis.
- 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.