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  Jump to: Intro, Swift Mercury, About the Rock, Conditions of the Surface

INTRO:
A mosiac of Mercury as the Mariner 10 was approaching it. Courtesy of NSSDC/NASA.      Mercury is the closest planet to the sun. Mercury's mean distance from the sun is 36 million miles (57.9 million kilometer) which is about half the distance from the sun to Venus. Mercury runs around the sun in a tight little elliptical path (eccentricity of 0.2056). The Earth's own eccentricity is only 0.0167, much more circular than Mercury's. At it's closest to the Sun, Mercury is 28.6 million miles (46 million km) away. At it's farthest it is 43.4 million miles (69.8 million km) away. Mercury is pretty small being only 3,031 miles (57.9 km) in diameter which is three-eighths of Earth's diameter.

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SWIFT MERCURY:
     Mercury moves faster than any other planet around the sun. Mercury travels 47.87 kilometers per second compared to Earth's speed 29.79 kilometers per second. One time around the sun for Mercury is only 88 earth-days, only about 3 months only. Astronomers up to 1965, thought that Mercury only rotated once in every 88 earth-days, which is the same time it takes to go around the sun once. That would mean that one side of Mercury would always face the sun. The side that would always face the sun be extremely hot, while the other side would be very dark and very cold. In 1965 they found out that Mercury rotates once every 59 earth-days. They found out by bouncing radar beams off of Mercury. The signals returned from one side of Mercury were different from another side. They measured and analyzed the movements of the different sides of Mercury and found that Mercury rotated once every 59 earth-days. So Mercury did not have one sizzling hot side and one cold dark side. Mercury rotates on its axis at a tilt of about 0.1 degrees.

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ABOUT THE ROCK:
     On the outside, Mercury is very much like our moon. It has little air or atmosphere, small, gray, reflects only 6% of the light it receives, and has craters, steep cliffs, and flat plains. The craters were caused by comets and meteorites colliding with the planet. Without a thick atmosphere to slow down and burn up incoming comets and meteoroids, Mercury and the moon are battered pieces of rock. All the lighter materials with lower boiling points have boiled off the surface since the creation of Mercury, because it is so hot leaving rocks and metal. An intriguing feature found on Mercury is the presence of several 3 km high cliffs as if Mercury's skin had cracked at some time in the past. An impact crater larger than France, called the Caloris Basin, was created by a shock-wave so great it created a mountain range on the other side of the planet. The first feature to be recorded on Mercury was name Kuiper Crater after Gerard Kuiper, the pioneer veteran planetary scientist who died while the Mariner 10 was on the way to Mercury.

Courtesy of NASA/JPL The very bright crater towards the top and left on the edge of  a  larger older crater is called the Kuiper Crater. 

      The core of Mercury is appears to be made of iron and other heavy elements. The Mariner 10 detected a magnetic field which indicates Mercury has a large iron core like the Earth. The Mariner 10 also found that Mercury has a metal core larger in proportion to its overall size than any other planet. This was suspected to be caused by the numerous catastrophic collisions that sent most of the planet's crust into space.

      The density of Mercury is only slightly less than Earth, at 5427 kg per cube meter compared to Earth's density which is 5520 kg per cube meter. Scientists suspect that Earth and Mercury are made of similar materials, because of their similar densities.

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CONDITIONS ON THE SURFACE:
     Since Mercury is the closest planet to the sun, it gets very hot on Mercury. Temperatures skyrocket to 801 Fahrenheit (427 Celsius) and dive to -279 F (-173 C) at night. The sun's rays are 7 times stronger on Mercury and the sun seems 2 ½ times bigger in Mercury's sky. That could cause one bad sunburn! Mercury doesn't have enough gases to reduce the heat and light it receives from the sun.

      The little atmosphere that Mercury does have consists of  small amounts of helium, hydrogen, oxygen and sodium. Combined, the little amount of gases on Mercury make a possible atmospheric pressure of 0.00000000003 pounds per square inch (or approximately 10^-10 Pascals). Also because of the lack of atmosphere, the Mercurial sky is black and the stars can be seen in broad daylight. 

 

 
Mercury's South Pole as taken by the Mariner 10. Ice is thought to exist at the poles in deep craters. To read more about Ice on Mercury click on the link below. Picture courtesty of NASA/JPL.

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Complete Fact Sheet

Observing Mercury

Ice on Mercury

Mariner 10

Sources for Mercury
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