Mercury (planet)

Mercury Astronomical symbol of mercury
File:Mercury in color - Prockter07 centered.jpg
Pronunciation/ˈmɜrkjəri/ (Audio file "en-us-Mercury.ogg " not found)
Orbital characteristics[4]
Epoch J2000
Aphelion69,816,900 km
0.466 697 AU
Perihelion46,001,200 km
0.307 499 AU
57,909,100 km
0.387 098 AU
Eccentricity0.205 630[2]
87.969 1 d
(0.240 846 a)
115.88 d[2]
47.87 km/s[2]
Inclination7.005° to Ecliptic
3.38° to Sun’s equator
6.34° to Invariable plane[3]
Known satellitesNone diameter = 4,880 km
Physical characteristics
Mean radius
2,439.7 ± 1.0 km[5][6]
0.3829 Earths
Flattening< 0.0006[6]
7.48×10Script error: No such module "Gapnum". km²
0.147 Earths[5]
Volume6.083×10Script error: No such module "Gapnum". km³
0.054 Earths[5]
Mass3.3022×10Script error: No such module "Gapnum". kg
0.055 Earths[5]
Mean density
5.427 g/cm³[5]
3.7 m/s²
0.38 g[5]
4.25 km/s[5]
58.646 day
1407.5 h[5]
Equatorial rotation velocity
10.892 km/h (3.026 m/s)
2.11′ ± 0.1′[7]
North pole right ascension
18 h 44 min 2 s
North pole declination
Albedo0.119 (bond)
0.106 (geom.)[2]
Surface temp. min mean max
0°N, 0°W 100 K 340 K 700 K
85°N, 0°W 80 K 200 K 380 K
up to −1.9[2]
4.5" – 13"[2]
Composition by volume42% Molecular oxygen
29.0% sodium
22.0% hydrogen
6.0% helium
0.5% potassium
Trace amounts of argon, nitrogen, carbon dioxide, water vapor, xenon, krypton, & neon[2]

Mercury is the smallest planet in the Solar System.[8][9][10] It is the closest planet to the sun.[11] It makes one trip around the Sun once every 87.969 days.[2][12] 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[13] 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,[14] 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.[11] 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.[15] 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),[16] 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.[17] 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.[18]

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.[19]

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).[2] 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.[20] Mercury's density is the second highest in the Solar System at 5.427 g/cm³, only a little bit less than Earth’s.[2] alot of the planets we see today have the same simularty then other planets so it reallly does not make a difffernce

Related pages


  1. "Mercurian". Oxford University Press. Retrieved 2016-12-15.
  2. 2.00 2.01 2.02 2.03 2.04 2.05 2.06 2.07 2.08 2.09 2.10 2.11 "Mercury Fact Sheet". NASA Goddard Space Flight Center. November 30, 2007. Retrieved 2008-05-28.
  3. "The MeanPlane (Invariable plane) of the Solar System passing through the barycenter". 2009-04-03. Retrieved 2009-04-03. (produced with Solex 10 written by Aldo Vitagliano; see also Invariable plane)
  4. Yeomans, Donald K. (April 7, 2008). "HORIZONS System". NASA JPL. Retrieved 2008-04-07.
  5. 5.0 5.1 5.2 5.3 5.4 5.5 5.6 5.7 Munsell, Kirk; Smith, Harman; Harvey, Samantha (May 28, 2009). "Mercury: Facts & Figures". Solar System Exploration. NASA. Retrieved 2008-04-07.CS1 maint: Multiple names: authors list (link)
  6. 6.0 6.1 Seidelmann, P. Kenneth; Archinal, B. A.; A’hearn, M. F.; et al. (2007). "Report of the IAU/IAGWorking Group on cartographic coordinates and rotational elements: 2006". Celestial Mechanics and Dynamical Astronomy 90: 155–180. doi:10.1007/s10569-007-9072-y. Retrieved 2007-08-28. 
  7. Margot, L.J. (2007). Peale, S.J.; Jurgens, R.F.; Slade, M.A.; Holin, I.V.. "Large Longitude Libration of Mercury Reveals a Molten Core". Science 316: 710–714. doi:10.1126/science.1140514. PMID 17478713. 
  8. "Mercury  l  Mercury facts, pictures and information". 2011 [last update]. Retrieved 7 March 2012.
  9. "BBC Solar System - Mercury: A tortured world close to our blazing Sun". 2012 [last update]. Retrieved 7 March 2012.
  10. Pluto was once thought to be the smallest, but, as of 2006, Pluto is now known as a dwarf planet.
  11. 11.0 11.1 Murchie, Scott L.; Vervack Jr., Ronald J.; Anderson, Brian J. (March 2011), "Space Science: Journey to the Innermost Planet", Scientific American, New York, 304 (3), pp. 26–31
  12. [1]
  13. Template:Cite book
  14. [2]
  15. "Mercury magnetic field". C. T. Russell & J. G. Luhmann. Retrieved 2007-03-16.
  16. "Background Science". European Space Agency. Retrieved 2008-05-23.
  17. Template:Cite book
  18. Template:Cite book
  19. "CBBC Newsround". British Broadcasting Corporation. Retrieved February 04, 2012. Check date values in: |accessdate= (help)
  20. Template:Cite book

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