The Solar System

Mercury

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Mercury

 

It would appear that Mercury could not support water in any form. It has very little atmosphere and is blazing hot during the day, but in 1991 scientists at Caltech bounced radio waves off Mercury and found an unusual bright return from the north pole. The apparent brightening at the north pole could be explained by ice on or just under the surface. But is it possible for Mercury to have ice? Because Mercury's rotation is almost perpendicular to its orbital plain, the north pole always sees the sun just above the horizon. The insides of craters would never be exposed to the Sun and scientists suspect that they would remain colder than -161 C. These freezing temperatures could trap water outgassed from the planet, or ices brought to the planet from cometary impacts. These ice deposits might be covered with a layer of dust and would still show bright radar returns.

Mercury Statistics

Mass (kg) 3.303e+23
Mass (Earth = 1) 5.5271e-02
Equatorial radius (km) 2,439.7
Equatorial radius (Earth = 1) 3.8252e-01
Mean density (gm/cm^3) 5.42
Mean distance from the Sun (km) 57,910,000
Mean distance from the Sun (Earth = 1) 0.3871
Rotational period (days) 58.6462
Orbital period (days) 87.969
Mean orbital velocity (km/sec) 47.88
Orbital eccentricity 0.2056
Tilt of axis (degrees) 0.00
Orbital inclination (degrees) 7.004
Equatorial surface gravity (m/sec^2) 2.78
Equatorial escape velocity (km/sec) 4.25
Visual geometric albedo 0.10
Magnitude (Vo) -1.9
Mean surface temperature 179°C
Maximum surface temperature 427°C
Minimum surface temperature -173°C
Atmospheric composition
Helium
Sodium
Oxygen
Other

42%
42%
15%
1%

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Made by Iain, Matt and James!!!