Mercury

Click for larger image Mercury is the closest planet to the Sun, and for this reason it has a very short year. Its days are quite long, though, because the planet revolves around its own axis very slowly. Due to both these factors, Mercury has just one day for each two years. It was named after the Greek god of commerce and travel, most likely because of its orbital velocity. The planet has a high temperature range, varying between -180°C to 530°C, and is the highest temperature range for any body in the Solar System. Despite this, radar observations of Mercury have shown signs that water and ice may be evident on some craters at the North Pole, which are shaded from the Sun.

The atmosphere of Mercury is very thin, and is largely made up of atoms blasted off by solar wind. These atoms escape the atmosphere very fast due to Mercury's hot surface, and create a significant drop in temperature. The planet is predominantly made up of a large iron core, approximately 3700km in diameter, which contributes to Mercury's high density and is also the reason why Mercury is some times referred to as the "Iron planet". Mercury is similar to the Moon in that it has a number of rather old craters, and it has no plate tectonics.� Mercury's surface is very irregular, as it has numerous cliffs and pits lining it. These were created when Mercury's core cooled and shrank and the effect of this was buckling of the planet's crust. Mercury has no known satellites.

Diameter

4,880 km

Mass

3.3 × 1023 kg

Mean Distance from sun

57,910,000 km

Mean Density

5.43 g/cm3

Rotational Period

59 Earth days

Orbital Period

88 Earth days

Mean Orbital Velocity

48 km/s

Atmosphere

50% oxygen, 30% sodium,
10% helium, 10% others

Average Surface Temperature

179°C

Equatorial Surface Gravity

3.7 m/s2

Copyright owned by the State of Victoria (Department of Education and Early Childhood Development). Used with Permission.

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