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% |
|