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							Mercury
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								| Imaged in enhanced 
								color by MESSENGER in 2008. |  
 Mercury is the smallest planet in the Solar System. It 
						is the closest planet to the sun. It makes one trip 
						around the Sun once every 87.969 days. Mercury is bright 
						when it is visible from Earth, ranging from −2.0 to 5.5 
						in apparent magnitude. It cannot be easily seen as it is 
						usually too close to the Sun. Because Mercury is 
						normally lost in the glare of the Sun, Mercury can only 
						be seen in the morning or evening twilight or during a 
						solar eclipse.
 
 Less is known about Mercury than about other planets of 
						our Solar System. Telescopes on the Earth show only a 
						small, bright crescent, and putting a satellite in orbit 
						around it is difficult. The first of two spacecraft to 
						visit the planet was Mariner 10, which mapped only about 
						45% of the planet’s surface from 1974 to 1975. The 
						second is the MESSENGER spacecraft, which finished 
						mapping the planet in March 2013.
 
 Mercury looks like Earth's Moon. It has many craters and 
						areas of smooth plains, no moons around it and no 
						atmosphere as we know it. However, Mercury does have an 
						extremely thin atmosphere, known as an exosphere. Unlike 
						Earth's Moon, Mercury has a large iron core, which gives 
						off a magnetic field about 1% as strong as that of the 
						Earth. It is a very dense planet due to the large size 
						of its core. Surface temperatures can be anywhere from 
						about 90 to 700 K (−183 °C to 427 °C, −297 °F to 801 
						°F), with the subsolar point being the hottest and the 
						bottoms of craters near the poles being the coldest.
 
 Known sightings of Mercury date back to at least the 
						first millennium BC. Before the 4th century BC, Greek 
						astronomers thought that Mercury was two different 
						objects: one able to be seen only at sunrise, which they 
						called Apollo; the other that was only able to be seen 
						at sunset, which they called Hermes. The English name 
						for the planet is from the Romans, who named it after 
						the Roman god Mercury, which they thought to be the same 
						as the Greek god Hermes. The symbol for Mercury is based 
						on Hermes' staff.
 
 Even though Mercury is the closest planet to the Sun, it 
						is not the warmest. This is because it has no greenhouse 
						effect, so any heat that the Sun gives to it quickly 
						escapes into space. The hottest planet is Venus.
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						| Inside Mercury 
 Mercury is one of four inner planets in the Solar 
						System, and has a rocky body like the Earth. It is the 
						smallest planet in the Solar System, with a radius of 
						2,439.7 km (1,516.0 mi). Mercury is even smaller than 
						some of the largest moons in the solar system, such as 
						Ganymede and Titan. However, it has a greater mass than 
						the largest moons in the solar system. Mercury is made 
						of about 70% metallic and 30% silicate material. 
						Mercury's density is the second highest in the Solar 
						System at 5.427 g/cm³, only a little bit less than 
						Earth’s.
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							Surface of Mercury
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								| Mercury's internal 
								structure and magnetic field. |  
 Mercury's surface looks similar to the surface of the 
						Moon. It has plains that look like mares and has lots of 
						craters. Mercury have been hit by a lot of comets and 
						asteroids 4.6 billion years ago. Mercury have also been 
						hit during a period called the Late Heavy Bombardment. 
						Mercury has lots of craters because it does not have any 
						atmosphere to slow objects down. Images gotten by 
						MESSENGER have shown that Mercury may have shield 
						volcanoes.
 
 The surface temperature of Mercury ranges from 100 to 
						700 K (−173 to 427 °C; −280 to 800 °F) at the most 
						extreme places. Even though the temperature at the 
						surface of Mercury in the day is very high, observations 
						suggest that there is frozen water on Mercury.
 
 Mercury is too small and hot for its gravity to keep any 
						thick atmosphere for long a long time. It does have a 
						thin exosphere that contains hydrogen, helium, oxygen, 
						sodium, calcium, potassium. This exosphere is lost and 
						replenished from lots of sources. Hydrogen and helium 
						may come from the solar wind. Radioactive decay of 
						elements inside the crust of Mercury is another source 
						of helium, and also sodium and potassium.
 
 Orbit and rotation
 
 Mercury has the most eccentric orbit of all the planets; 
						its eccentricity is 0.21. Its distance from the Sun 
						ranges from 46,000,000 to 70,000,000 km (29,000,000 to 
						43,000,000 mi). It takes 87.969 Earth days to go around 
						the Sun. Mercury's axial tilt is 0.027 degrees which is 
						best measurement of the axial tilt.
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							List of satellites sent to 
						Mercury
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								| MESSENGER being 
								prepared for launch. |  
 Many man-made satellites have been sent to Mercury to 
						study it. They are:
 
 Mariner 10
 
 The first spacecraft to visit Mercury was NASA's Mariner 
						10. It stayed in Mercury's orbit from 1974–1975. Mariner 
						10 provided the first close-up pictures of Mercury's 
						surface. It showed many types of geological features, 
						such as the craters. Unfortunately, the same face of the 
						planet was day at each time Mariner 10 flew close to 
						Mercury. This made close observation of both sides of 
						the planet impossible. In the end, less than 45% of the 
						planet's surface was mapped.
 
 The Mariner 10 came close to Mercury three times. At the 
						first time, instruments found a magnetic field, which 
						surprised planetary geologists because Mercury's 
						rotation was too slow to generate a magnetic field. The 
						second time was mainly used to take pictures of 
						Mercury's surface. At the third time, more information 
						about the magnetic field were obtained. It showed that 
						the planet's magnetic field is much like Earth's.
 
 On March 24, 1975, just eight days after its final close 
						approach, Mariner 10 ran out of fuel. Because its orbit 
						could no longer be controlled, mission controllers 
						instructed the probe to shut down. Mariner 10 is thought 
						to still be orbiting the Sun.
 
 MESSENGER
 
 The second satellite to reach Mercury is NASA's 
						MESSENGER. It stands for MErcury Surface, Space 
						ENvironment, GEochemistry, and Ranging. It was launched 
						on August 3, 2004. It made a fly-by of Earth in August 
						2005. It made another fly-by of Venus in October 2006. 
						It made its first fly-by of Mercury happened on January 
						14, 2008, a second on October 6, 2008, and a third on 
						September 29, 2009. Most of the hemisphere not mapped by 
						Mariner 10 was mapped during these fly-bys. The 
						satellite entered an elliptical orbit around the planet 
						on March 18, 2011. The first image of Mercury orbiting 
						the Sun was gotten on March 29, 2011.
 
 MESSENGER was made to study Mercury's high density, the 
						history of Mercury's geology, its magnetic field, the 
						structure of its core, whether it has ice at its poles, 
						and where its thin atmosphere comes from. MESSENGER 
						crashed into Mercury's surface on April 30, 2015.
 
 Bepicolombo
 
 The European Space Agency and the Japanese Space Agency 
						developed and launched a joint mission called 
						BepiColombo. It will orbit Mercury with two probes: one 
						to map the planet and the other to study its 
						magnetosphere. It was launched on October 20, 2018. 
						BepiColombo is expected to reach Mercury in 2025. It 
						will release the probe that will study the magnetosphere 
						into an elliptical orbit. It will then release the probe 
						the will make a map of Mercury into a circular orbit.
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						|  Kiddle: 
					Mercury Wikipedia: Mercury
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