Title: Earth volcanoes craters mountains riverbeds
1Earthvolcanoescratersmountainsriverbeds
2Venusvolcanoesfew craters
Radar view of a twin-peaked volcano
3Marssome cratersvolcanoesriverbeds?
4Mercurycraterssmooth plains,cliffs
5Mooncraterssmooth plains
67.3 Mars A Victim of Planetary Freeze-drying
- Our Goals for Learning
- What geological features tell us that water once
flowed on Mars? - Why did Mars change?
7Mars vs. Earth
- 50 Earths radius, 10 Earths mass
- 1.5 A.U from the Sun
- Axis tilt about the same as Earth.
- Similar rotation period.
- Orbit is more elliptical than Earths seasons
more extreme in the south than the north. - Thin CO2 atmosphere little greenhouse
8Main Difference seems to be
9What geological features tell us water once
flowed on Mars?
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11Eroded crater
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14Volcanoesas recent as 180 million years ago
15Past tectonic activity
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19- 2004 Opportunity Rover provided strong evidence
for abundant liquid water on Mars in the distant
past. - How could Mars have been warmer and wetter in the
past?
20Today, most water lies frozen underground (blue
regions) Some scientists believe accumulated
snowpack melts to carve gullies even today
21Why did Mars change?
22Would terraforming Mars work?
23What have we learned?
- What geological features tell us that water
once flowed on Mars? - Dry river channels, rock-strewn floodplains, and
eroded craters all show that water once flowed on
Mars, though any periods of rainfall seem to have
ended at least 3 billion years ago. Mars today
still has water ice underground and in its polar
caps, and could possibly have pockets of
underground liquid water.
24What have we learned?
- Why did Mars change?
- Marss atmosphere must once have been much
thicker with a much stronger greenhouse effect,
so change must have occurred due to loss of
atmospheric gas. Much of the lost gas probably
was stripped away by the solar wind, which was
able to reach the atmosphere as Mars cooled and
lost its magnetic field and protective
magnetosphere. Water was probably also lost
because ultraviolet light could break apart water
molecules in the atmosphere, and the lightweight
hydrogen then escaped to space.