Mercury is the
nearest planet to the sun. It has the most extreme contrast in temperature between
day (430°C) and night (-180°C) in the solar system. Daytime temperatures are high
enough to melt zinc and tin. Mercury has virtually no atmosphere, meaning life as
we know it is impossible.
Mercury was the Roman god of trade and commerce, in the
same vein as Hermes of the Greeks, the messenger.
Mercury's orbit is highly eccentric, meaning it's path
is elliptical. Also, mercury rotates three times for every two orbits of the sun.
Mercury has no satellites.
|
Semimajor axis (km) |
57.91x106 |
|
Perihelion (km) |
46.00x106 |
|
Aphelion (km) |
69.82x106 |
|
Mean orbital speed (km s-1) |
47.87 |
|
Sidereal orbit period (days) |
87.969 |
|
Tropical orbit period (days) |
87.968 |
|
Synodic period (days) |
115.88 |
|
Length of day (hours) |
4222.6 |
|
Sidereal rotation period (hours) |
1407.6 |
|
Obliquity to orbit (deg) |
0.01 |
|
|
Semimajor axis (AU) |
0.38709893 |
|
Eccentricity |
0.20563069 |
|
Inclination (deg) |
7.00487 |
|
Longitude of ascending node (deg) |
48.33167 |
|
Longitude of perihelion (deg) |
77.45645 |
|
Mean longitude (deg) |
252.25084 |
|
Discoverer |
Unknown |
|
Date of Discovery |
Classical |
J2000 Data from
NSSDC
|
Only one spacecraft has been to mercury, Mariner 10, passing
three times in 1974-75. However NASA's Messenger is on the way, launched in August
2004, and will fly by three times and then enter mercury orbit in March 2011. Then
in 2012, ESA/ISAS's BepiColombo will be launched, also into mercurian orbit. Because
of mercury's proximity to the sun, it cannot safely be photographed by the Hubble
Space Telescope.
Mercurian atmosphere is thin enough to be described as
an exosphere, meaning the constituent atoms never collide. The identified elements
in the exosphere are sodium, potassium, hydrogen, oxygen and neon. Ions and high
frequency electromagnetic radiation from the sun are responsible for dislodging
the atoms in the exosphere.
|
Mass (kg) |
3.302x1023 |
|
Equatorial radius (km) |
2439.7 |
|
Polar radius (km) |
2439.7 |
|
Mean density (kg m-3) |
5427 |
|
Equatorial surface gravity (m s-2) |
3.70 |
|
Escape Velocity (km s-1) |
4.3 |
|
Black-body temp (K) |
442.5 |
|
Solar intensity (W m2) |
9127 |
|
Natural satellites |
0 |
The surface of mercury is splattered with craters, the
majority being formed in the early days of the solar system when rocky bodies moving
at high speeds around the sun collided with the planet. The nonexistence of atmosphere
meant that there was nothing to cushion the incoming bodies. Flat plains suggest
possible volcanic activity. Earth based radar observations hint at possible water
ice in the pole craters, possible only because of permanent shadow. The Caloris
Basin is a notable landmark, a giant crater having a 650 km radius and is similar
to the lunar basins.
Mercury is the second most dense planet after earth. The
earth has more mass and so part of this density is attributable to gravitational
compression. We can only speculate at the core composition of mercury, but it has
a very high density for its radius so it is likely to have a large metallic core
accounting for most of its mass. In this, mercury differs from the other terrestrial
planets. Possible explanations are that mercury formed in an iron rich part of the
early solar system, the sun's rays have reduced the metal oxides to solid metals
which are denser, collisions or energy from the sun may have removed part of a less
dense crust.
Mercury's point of perihelion was noticed to rotate the
sun faster than predicted by Newton's laws of gravitation and proved to be strong
evidence for Einstein's gravitational model; general relativity.
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