astronomy 340 fall 2007
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Astronomy 340 Fall 2007. 2 October 2007 Class #9. Salient Martian Features. R Mars = 3396 km (R Earth = 6378 km) Higher surface area to mass ratio More efficient cooling Lower internal heat flow, less volcanism No plate tectonics Atmospheric Composition 95% CO 2 (same as Venus) - PowerPoint PPT PresentationTRANSCRIPT
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ASTRONOMY 340FALL 20072 October 2007Class #9
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Salient Martian Features RMars = 3396 km (REarth = 6378 km)
Higher surface area to mass ratio More efficient cooling Lower internal heat flow, less volcanism No plate tectonics
Atmospheric Composition 95% CO2 (same as Venus) Pressure = 0.006 bar (Earth = 1, Venus = 89)
TSurface hey, it’s cold! Mean solar constant 0.431 (Earth =1) Summer T ~ 273K (max) Winter (polar) T ~ 150K ground is permanently
frozen to 1 km
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Soil Composition
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Mars Missions Current Missions
Spirit and Opportunity (rovers) 2001 Mars Odyssey (orbiter) Mars Global Surveyot (orbiter) Mars Express (polar orbit) Mars Reconnaissance Orbiter (just launched)
Planned Phoenix Mars Science Laboratory
Past Mariner flybys/orbiters Viking landers Pathfinder
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NASA Mars Missions -- Goals Determine whether life ever arose on
Mars Characterize the Climate of Mars Characterize the Geology of Mars Prepare for Human Exploration
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Where to land? Equatorial maximum solar radiation Low elevation maximum atmosphere
to slow descent, low shear Relatively flat to preserve airbag Radar-reflective, hard surface for rovers
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Where to land? Parachute to slow descent, followed by
bouncing airbag….
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Gusev Crater
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Spirit Landing SiteGolombek et al 2005 Nature 436 44
Nice and flat….
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Opportunity landing site – and some space junk
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Rock size distribution on landing sites
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Surface CompositionBibring et al. 2005 Science 307 1576
Ices/Frosts CO2 veneers over polar ice caps H2O ice w/ dust
Hydrated Minerals/Ferric Oxides Significant presence – detected via 3μm
feature Primarily in older craters (younger craters
lack hydrated minerals) Igneous Rocks
Standard olivines
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Water on Mars Canals? Background origin of H2O on Earth
Outgassing via internal processes volcanic Formation via accretion of hydrated protoplanetary material
External origin via hydrated impactors (comets?) Maintaining liquid H2O on surface….
Temperature Liquid H2O unstable at 150 K < T < 220 K But ice on stable at poles
Pressure Sublimation of polar ice atmospheric pressure insufficient to maintain
water in atmosphere Dissociation of H2O, loss of H
Current conditions not favorable for liquid H2O on Martian surface or significant H2O in atmospere
But…..
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Water on Mars Polar Ice Caps Mariner 9 (1972)
images of obvious channels that look like river beds major amounts of surface water in past
Atmospheric chemistry Trace H2O content via
outgassed volatiles 80-160m of water
outgassedNorth Polar Ice Cap in summer
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Water on Mars Water channels
Outflow channels Catastrophic floods (108 m3 s-1 vs 104 m3 s-1) “sudden” appearance Volcanism, internal pressure, ???
Valley networks Look like river systems groundwater
Fretted channels Remote sensing/imaging
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Possible water flow as seenby Global Surveyor.
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Gusev Crater Haskin et al 2005 Nature 436 66 Gusev plain an old
lake bed? Primarily igneous
rock (olivine basalt) Veins/plugs aqeous
solutions plausible Composition
measured via near-IR spectrometer
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Gusev crater Haskin et al 2005
Note inclusions – need water to form
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Gusev Crater Haskin et al 2005 Nature 436 66 Veins/plugs aqeous
solutions plausible Composition measured via
near-IR spectrometer Various geochemical
effects of aqeous solutions E.g. ratio of Al2O3 vs SO3 Increased ratio of salts,
oxidation of Fe2+
Conclusions: running water, but no pools/oceans
Inverse correlation – mixing with evaporative component with high S content
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Gusev Crater Haskin et al 2005 Nature 436 66
Gusev plain an old lake bed? Primarily igneous rock (olivine basalt)
Veins/plugs aqeous solutions plausible Composition measured via near-IR
spectrometer Various geochemical effects of aqeous
solutions E.g. ratio of Al2O3 vs SO3 Increased ratio of salts, oxidation of Fe2+
Conclusions: running water, but no pools/oceans
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Frozen Equatorial Sea?Murray et al. 2005 Nature 434 352 What are these
cracked “plates”? Lava? The authors think not…
Edges much younger than rest of plate – lava doesn’t do this
Crater density suggests age ~ 5Myr
Resemblance of plates to pack-ice in Arctic
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a. Mars 13.7m resolution b. Antarctica c. Martian ice raft?
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But is there water there now?
Diagram showing possible fossil water flow from subsurface source. Images from Global Surveyor. See handout.
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Phobos & Deimos Low inclination,
equatorial orbits
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