2. Historical background of Mars.
Evidences of water existence on the surface
of Mars:
(1) - Water vapour .
- Mars atmosphere.
- Over the polar cap.
- Over the four big volcanoes.
(2) - Water-ice.
- Polar ice cap.
- Glaciers.
- Frozen Lake in Crater.
- Water- ice cloud.
(3)- The Flowing the water on Mars surface.
3. Mars
Table 1: the difference between the Earth and Mars .
Planets Distance from Period of Period of
the sun (AU) revolutio rotation
n
Earth 1 365 days 24 hours
Mars 1.52 687 days 25 hours
4. North pole
Craters
South pole
Valley
Olympus volcano
6. about (27°C) at morning
to about (-73°C) at
midnight.
humidity on Mars is very
high.
The pressure cause flow
the water (Heldmann et
al.,2009).
http://web.ics.purdue.edu/~nowack/geos105/lect14-dir/lecture14.htm
7. H2O column density at high northern latitudes for Ls = 93–
100. H2O column density at high northern latitudes for
The maximum column density is 70 pr-um. Ls = 111–115. The maximum column density is 70 pr-um.
H2O column density at high northern latitudes for H2O column density at high northern latitudes for
Ls ¼ 101–105. The maximum column density is 70 pr-um. Ls ¼ 116–120. The maximum column density is 70 pr-um.
8. Olympus
Water
vapour
Olympus Ascraeus Mons
Pavonis Arsia
15. Malin, M, Calvin, W, Cantor, B, Clancy, R, Haberle, R,
James, P, Thomas, P, Wolff, M, Bell, J & W.Lee, S 2008,
‘Climate, weather, and north polar observations from the
Mars Reconnaissance Orbiter Mars Color Imager’, Icarus,
vol.194, no. , pp501-512, accessed in 20-01-2011.
The Jackson School of Geosciences, 2008, Glaciers on
Mars: Scientists Discover Concealed Glaciers on Mars at
Mid-Latitudes, The University of Texas at Austin, accessed
in 24-01-2011,
http://geology.com/research/glaciers-on-mars.shtml
Seiff, A. and Kirk, D. (1977).
"Structure of the atmosphere of Mars in summer at mid-latitudes"
(abstract only). Journal of Geophysical Research,
82(28):4364–4378.