Mercury (planet)

**Mercury** is the first  planet from the Sun. It is the second hottest planet, and the smallest in the Solar System. It is also the closest planet to the Sun. It makes one trip around the Sun once every 87.969 days.

Mercury is bright when we can see it from Earth. It has an apparent magnitude ranging from −2.0 to 5.5. It cannot be seen easily because it is usually too close to the Sun. Because of this, Mercury can only be seen in the morning or evening twilight or when there is a solar eclipse.

Less is known about Mercury than about other planets of our Solar System. Even with telescopes<nowiki/> only a small, bright crescent can be seen. It is also hard to put a satellite in orbit around it. Two spacecraft have visited Mercury. The first one was Mariner 10. It only made a map of about 45% of the Mercury's surface from 1974 to 1975. The second is the MESSENGER spacecraft, which finished mapping Mercury in March 2013.

Mercury looks like Earth's Moon. It has many craters and smooth plains. It has no moons and little atmosphere as we know it. However, Mercury does have an extremely thin atmosphere, known as an exosphere.  Mercury has a large iron core. Because of this Mercury has a magnetic field about 1% as strong as that of the Earth. It is a very dense planet because its core is large.

Because of it's thin atmosphere, temperature at the surface can be anywhere from about 90 to  (−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: The one that they were only able to see at sunrise, they called Apollo; the other one that they were only able to see at sunset, they called Hermes. The English name for the planet is from the Romans, who named it after the Roman god Mercury. The symbol for Mercury is based on Hermes' staff.

Even though Mercury is the closest planet to the Sun, it is not the hottest. This is because it has no greenhouse effect. The heat that the Sun gives it, quickly escapes into space. The hottest planet is Venus.

## Inside Mercury

Mercury is one of four inner planets in the Solar System. It is a terrestrial planet like Earth. It is the smallest planet in the Solar System, with a radius of . Mercury is even smaller than some of the largest moons in the solar system, such as Ganymede, the largest moon of Jupiter and Titan, the largest moon of Saturn. However, it has in 2.2 times greater mass than Ganymede and around 2 times heavier than Titan. Mercury is made of about 70% metallic and 30% silicate material. Mercury has the second highest density in the Solar System at 5.427 g/cm³, only slightly less than Earth’s.

## Surface of Mercury

Mercury's surface resembles the surface of the Moon. It has plains that look like mares and has lots of craters. Mercury was hit by a multitude of comets and asteroids 4.6 billion years ago. Mercury was also hit during a period called the Late Heavy Bombardment. Mercury has many craters because its atmosphere is too faint to slow foreign objects down. Images from _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 a long time. It does have a thin exosphere that is made up of hydrogen, helium, oxygen, sodium, calcium, potassium. This exosphere is blown away and replenished from lots of sources. Hydrogen and helium may come from the solar wind. Radioactive decay of elements inside the crust of Mercury provide another source of helium, as well as sodium and potassium.

## Orbit and rotation

Mercury has the most eccentric orbit of all the planets in the Solar System. It has an eccentricity of 0.21. It ranges from 46,000,000 to 70,000,000 km (29,000,000 to 43,000,000 mi) away from the Sun. Mercury takes 87.969 Earth days to go around the Sun. Mercury's axial tilt is 0.027 degrees. While most of Mercury's precession is caused by the pull of other planets, the second-largest cause is the warping of space-time around the Sun.

In the future, because Mercury's orbit's is very eccentric and Jupiter's huge gravity, its orbit may become unstable and the following things may happen:

- It crashes into the Sun
- It enters the Sun's Roche limit slowly and is torn apart
- It crashes into Venus
- It crashes into Earth
- It is flung out of the Solar System and becomes a rogue planet

## List of satellites sent to Mercury

Few 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 to 1975. Mariner 10 took the first close-up pictures of Mercury's surface. It showed many features, such as the craters. Unfortunately, the same side of Mercury was day each time Mariner 10 flew close to Mercury. This made observing of both sides of Mercury impossible. In the end, less than 45% of the Mercury's surface was mapped.

Mariner 10 came close to Mercury three times. At the first time, it found a magnetic field, which surprised planetary geologists because Mercury's rotation was too slow to create a magnetic field. The second time was mainly used to take pictures of Mercury's surface. At the third time, it got more information about the magnetic field. It showed that the Mercury's magnetic field is like the Earth's magnetic field.

On March 24, 1975, eight days after its last close fly by, Mariner 10 ran out of fuel. Because its orbit could no longer be controlled, mission controllers shut down the probe . Mariner 10 is thought to still be orbiting the Sun.

### _MESSENGER_

The second satellite to visit 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. It made a map of most of Mercury that _Mariner 10_ didn't map. 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, if 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 made and launched a spacecraft 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.

## Related pages

- List of planets

## Other websites

- SolarViews.Com
- www.planetfacts.net

## Infobox (planet)

- **bgcolour**: #D8BBA6
- **name**: Mercury
- **symbol**:
- **image**: Mercury in color - Prockter07 centered.jpg
- **caption**: Mercury photographed by MESSENGER (spacecraft), MESSENGER spacecraft in 2008
- **epoch**: J2000
- **aphelion**: 69,816,900 km
0.466 697 Astronomical unit, AU
- **perihelion**: 46,001,200 km
0.307 499 AU
- **semimajor**: 57,909,100 km
0.387 098 AU
- **eccentricity**: 0.205 630
- **period**: 87.969 1 day, d
(0.240 846 julian year (astronomy), a)
- **synodic period**: 115.88 d
- **avg speed**: 47.87 km/s
- **inclination**: 7.005° to Ecliptic
3.38° to Ecliptic#Ecliptic and planets, Sun’s equator
6.34° to Invariable plane
- **asc node**: 48.331°
- **arg peri**: 29.124°
- **mean anomaly**: 174.796°
- **satellites**: None

diameter = 4,880 km
- **mean radius**: 2,439.7 ± 1.0 km
0.3829 Earths
- **flattening**: < 0.0006
- **surface area**: 7.48 km²
0.147 Earths
- **volume**: 6.083 km³
0.054 Earths
- **mass**: 3.3022 kg
0.055 Earths
- **density**: 5.427 g/cm³
- **surface grav**: 3.7 Acceleration, m/s²
0.38 g-force, g
- **escape velocity**: 4.25 km/s
- **sidereal day**: 58.646 day
1407.5 hour, h
- **axial tilt**: 2.11′ ± 0.1′
- **right asc north pole**: 18 h 44 min 2 s
281.01°
- **declination**: 61.45°
- **albedo**: 0.119 (Bond albedo, bond)

0.106 (Geometric albedo, geom.)
- **magnitude**: up to −1.9
- **angular size**: 4.5" – 13"
- **temp name1**: 0°N, 0°W
- **min temp 1**: 100 K
- **mean temp 1**: 340 K
- **max temp 1**: 700 K
- **temp name2**: 85°N, 0°W
- **min temp 2**: 80 K
- **mean temp 2**: 200 K
- **max temp 2**: 380 K
- **adjectives**: Mercurian,
- **atmosphere composition**: 42% Molecular oxygen
29.0% sodium
22.0% hydrogen
6.0% helium
0.5% potassium
Trace amounts of argon, nitrogen, carbon dioxide, Water, water vapor, xenon, krypton, & neon