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Exploring the surface of Mars

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Exploring the surface of Mars ... well-known geological history of Earth with a speculative history of Mars The Mars Exploration Rovers (MER) are mobile, ... – PowerPoint PPT presentation

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Title: Exploring the surface of Mars


1
Exploring the surface of Mars
What can we learn about the ancient past of Mars
from measurements and observations on the surface?
2
Where we ended last time
  • Liquid water cannot be present on the surface of
    Mars at the present time
  • Nonetheless, pictures from orbit show water
    channels going through ancient landscapes on Mars
    (2 types of channels)
  • Perhaps the climate of Mars 3-4 billion years ago
    was conducive to the presence of bodies of
    standing water

3
To see what people have in mind, lets compare
the (relatively) well-known geological history of
Earth with a speculative history of Mars
4
A sketchy history of the planet Earth
5
An even sketchier history of the planet Mars
6
Prior to 2004 2 theories about the geological
history of Mars
  • warm, wet Mars early in solar system history,
    a dense atmosphere permitted higher temperatures
    and pressure, and existence of bodies of liquid
    water. Early Mars might have been similar to
    early Earth.
  • cold, dry Mars Mars has been about the same
    as now for all of its history. The valley
    networks and outflow channels show water flows,
    but they were short duration floods rather than
    long lasting bodies of water
  • An argument in favor of cold, dry Mars the
    apparent absence of carbonate rocks on the
    surface of Mars.

7
To resolve this required (and requires)
geological measurements, studies of minerals in
Martian rocks
  • Some minerals (hematite) form in presence of
    standing water. Others, (olivine) are destroyed
    by water.

8
The Mars Exploration Rovers (MER) are mobile,
geological laboratories sent to see if Martian
rocks are lava flows (e.g. basalts) or minerals
formed in the presence of water.
9
The launch, interplanetary journey, and arrival
at Mars of an MER spacecraft
The journey to Mars of "Spirit"
10
Spirit and Opportunity on the Surface of Mars
11
Gusev Crater the view from the surface
12
On a hill in Gusev crater
13
The Opportunity landing site
14
Sedimentary rocks on Mars
15
Opportunity finds hematite spheresminerals that
condensed from water
16
Opportunity explores ancient sedimentary rocks in
Victoria Crater and other craters
A panorama of Victoria Crater from the MER
"Opportunity"
17
Take advantage of the marvelous images in your
textbook
  • Figure 11.29overhead view of Opportunity at
    Victoria crater
  • 11.28panorama of Endurance crater
  • 11.32evidence of water waves (ripples) in
    ancient streambeds
  • 11.20water gullies formed in a space a few years

18
What have we learned from the MERs and Mars
Phoenix
  • It now seems clear that there were standing
    bodies of water for long periods of time early in
    Martian history
  • Evidence is presence of hematite, jarosite, and
    other minerals that form in lakes or oceans
  • Relative absence of carbonate rocks is due to
    alternative chemistry in acidic water
  • But, apparently oldest rock strata do contain
    carbonate rocks and clay (montmorillonite)

19
In the futureMars Science Laboratory
  • Launch in fall, 2011, arrival fall 2012. Will
    make tests for organic chemicals, biological
    molecules

20
The El Dorado of future missions Mars Sample
Return
rom Earth) in 2014.
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