| Themes > Science > Earth Sciences > Geology > Earth > Earth's Origin and Structure > Comparative Planetology | ||||||||||||||||||||||||||||||
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| property | Venus | Earth | Mars |
| pressure | 92 bar | 1.013 bar | 0.007 bar |
| average Temperature | 482°C | 15°C | -63°C |
| atmosphere (%) | |||
| CO2 | .96 | .00360 | .9532 |
| N2 | .03+ | .78 | .027 |
| Ar2 | trace | .01 | .016 |
| O2 | 0 | .201 | .0013 |
The atmosphere of Venus includes trace amounts of Sulfur dioxide(SO2), water vapor (H2O gas), carbon monoxide (CO), argon (Ar2), helium (He), neon (e), hydrogen chloride (HCl), and hydrogen fluoride (HF).
The atmosphere of Mars contains smaller amounts of:
Carbon Monoxide (CO) = 0.07%
Water (H2O) = 0.03%
Neon (Ne) = 0.00025%
Krypton (Kr) = 0.00003%
Xenon (Xe) = 0.000008%
Ozone (O3) = 0.000003%
Jovian Planets and moons
The moons of Saturn and Jupiter include some bodies which have been proposed as possible sites of prebiotic chemistry.
Origin of the Moon. is complicated by the Moon's composition which is somewhat similar to that of Earth's mantle, but not it's average composition.
Information provided by: http://www2.bc.edu