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Mercury at 0.4 AU (57,910,000 km) is the [[planet]] closest to our Sun and it is the smallest of the eight planets in our solar system with only a 0.055 Earth mass (3.30e23 kg) and a diameter of 4,880 km.  
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[[Image:Mercury JPL-NASA.jpg|right|thumb|350px|{{#ifexist:Template:Mercury JPL-NASA.jpg/credit|{{Mercury JPL-NASA.jpg/credit}}<br/>|}}mosaic of Mariner 10 photos of Mercury taken between 1974 and 1976]]
{{dambigbox|Mercury (planet)|Mercury}}
'''Mercury''' at 0.4 AU (57,910,000 km) is the [[planet]] closest to our Sun, and it is the smallest of the eight planets in our solar system, with only a 0.055 Earth mass (3.30e23 kg) and a diameter of 4,880 km.  
{{Image|Mercury JPL-NASA.jpg|right|350px|Mosaic of Mariner 10 photos of Mercury taken between 1974 and 1976}}
 
==Parameters for classification as a planet==
==Parameters for classification as a planet==
Mercury is classified as a planet by the International Astronomical Union for meeting the following criteria:<ref>[http://www.nasa.gov/vision/universe/solarsystem/planetsf-20060824.html Honey, I Shrunk the Solar System] NASA. “The International Astronomical Union has decided that, to be called a planet, an object must have three traits. It must orbit the sun, be massive enough that its own gravity pulls it into a nearly round shape, and be dominant enough to clear away objects in its neighborhood.”</ref>
Mercury is classified as a planet by the [[International Astronomical Union]] for meeting the following criteria:<ref>[http://www.nasa.gov/vision/universe/solarsystem/planetsf-20060824.html Honey, I Shrunk the Solar System] NASA. “The International Astronomical Union has decided that, to be called a planet, an object must have three traits. It must orbit the sun, be massive enough that its own gravity pulls it into a nearly round shape, and be dominant enough to clear away objects in its neighborhood.”</ref>
*Orbits the sun;
*Orbits the sun;
*Has mass sufficient for its gravity to form a nearly round shape;
*Has mass sufficient for its gravity to form a nearly round shape;
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==Rotational characteristics==
==Rotational characteristics==
Mercury’s surface temperature fluctuates from more than 400°C to -180°C . Planetary rotation means that alternating areas are exposed to the sun’s heat, with the result that the surface of a planet will heat and cool in alternating periods. However, while Mercury does in fact rotate about its axis, Mercury’s rotational and orbital periods are coupled, that is, nearly the same. This means that some places on Mercury’s surface receive 2.5 times more solar radiation than other areas.<ref name=NMMRotation>[http://www.nmm.ac.uk/server/show/conWebDoc.272/viewPage/8 The effect of rotation] National Meritime Museum</ref> As the planet closest to the sun it receives the highest ratio of solar radiation. Solar radiation decreases by the inverse square law as it reaches further away from the sun. The Moon, by comparison, which also has no atmosphere but is much further from the sun that Mercury reaches temperatures of only about 110°C<ref>[http://www.nmm.ac.uk/server/show/conWebDoc.272/viewPage/3 What happens to the Sun's radiation when it reaches a planet?]NMM</ref>
Mercury’s surface temperature fluctuates from more than 400°C to -180°C . Planetary rotation means that alternating areas are exposed to the Sun’s heat, with the result that the surface of a planet will heat and cool in alternating periods. However, while Mercury does in fact rotate about its axis, Mercury’s rotational and orbital periods are coupled, that is, nearly the same. This means that some places on Mercury’s surface receive 2.5 times more solar radiation than other areas.<ref name=NMMRotation>[http://www.nmm.ac.uk/server/show/conWebDoc.272/viewPage/8 The effect of rotation] National Maritime Museum</ref> As the planet closest to the Sun it receives the highest ratio of solar radiation. Solar radiation decreases by the inverse square law as it reaches further away from the Sun. The Moon, by comparison, which also has no atmosphere but is much further from the Sun than Mercury, reaches temperatures of only about 110°C<ref>[http://www.nmm.ac.uk/server/show/conWebDoc.272/viewPage/3 What happens to the Sun's radiation when it reaches a planet?]NMM</ref>


==Orbital characteristics==
==Orbital characteristics==
Mercury's sidereal period is 87.97 days per year.<ref> A sidereal period is the time it takes a planet to return to an orbital position relative to the stars</ref> Mercury's distance from Sun is 0.31 AU at perihelion (the closest approach to the sun), 0.47 at aphelion (its nearest approach and it has an orbital inclination of 7.0° relative to the solar plane.<ref>[http://www.nmm.ac.uk/server/show/conWebDoc.393 The orbits of the planets] National Maritime Museum</ref>
Mercury's sidereal period is 87.97 days per year.<ref> A sidereal period is the time it takes a planet to return to an orbital position relative to the stars</ref> Mercury's distance from Sun is 0.31 AU at perihelion (the closest approach to the sun), 0.47 AU at aphelion (its most distant point) and it has an orbital inclination of 7.0° relative to the solar plane.<ref>[http://www.nmm.ac.uk/server/show/conWebDoc.393 The orbits of the planets] National Maritime Museum</ref>


==References==
==References==
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<references/>
</div>
</div>
==External links==
* [http://solarsystem.nasa.gov/index.cfm NASA's Solar System Exploration site]
* [http://space.jpl.nasa.gov NASA's Solar System Simulator]
* [http://www.jpl.nasa.gov/solar_system NASA/JPL Solar System main page]
* [http://www.nineplanets.org/ The <strike>Nine</strike>8 Planets - Comprehensive solar system site by Bill Arnett]
* [http://www.krysstal.com/solarsys_planets.html Planetary data]
* [http://www.solstation.com/habitable.htm SolStation: Stars and Habitable Planets]
* [http://www.space.com/solarsystem/ SPACE.com: All About the Solar System]
*[http://www.classzone.com/books/earth_science/terc/content/visualizations/es2701/es2701page01.cfm?chapter_no=27 Illustration of the distance between planets]
*[http://www.co-intelligence.org/newsletter/comparisons.html Illustration comparing the sizes of the planets with each other, the sun, and other stars]
[[Category:Astronomy Workgroup]]
[[Category:CZ Live]]

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This editable Main Article is under development and subject to a disclaimer.
This article is about Mercury (planet). For other uses of the term Mercury, please see Mercury (disambiguation).

Mercury at 0.4 AU (57,910,000 km) is the planet closest to our Sun, and it is the smallest of the eight planets in our solar system, with only a 0.055 Earth mass (3.30e23 kg) and a diameter of 4,880 km.

Mosaic of Mariner 10 photos of Mercury taken between 1974 and 1976

Parameters for classification as a planet

Mercury is classified as a planet by the International Astronomical Union for meeting the following criteria:[1]

  • Orbits the sun;
  • Has mass sufficient for its gravity to form a nearly round shape;
  • Has mass sufficient for gravity to clear a path in its orbit.

Physical characteristics

Mercury has no natural satellites, and its only known geological features besides impact craters are "wrinkle ridges", probably produced by a period of contraction early in its history.[2] Mercury's almost negligible atmosphere consists of atoms blasted off its surface by the solar wind.[3] Its relatively large iron core and thin mantle have not yet been adequately explained. Hypotheses include that its outer layers were stripped off by a giant impact, and that it was prevented from fully accreting by the young Sun's energy.[4][5]

Rotational characteristics

Mercury’s surface temperature fluctuates from more than 400°C to -180°C . Planetary rotation means that alternating areas are exposed to the Sun’s heat, with the result that the surface of a planet will heat and cool in alternating periods. However, while Mercury does in fact rotate about its axis, Mercury’s rotational and orbital periods are coupled, that is, nearly the same. This means that some places on Mercury’s surface receive 2.5 times more solar radiation than other areas.[6] As the planet closest to the Sun it receives the highest ratio of solar radiation. Solar radiation decreases by the inverse square law as it reaches further away from the Sun. The Moon, by comparison, which also has no atmosphere but is much further from the Sun than Mercury, reaches temperatures of only about 110°C[7]

Orbital characteristics

Mercury's sidereal period is 87.97 days per year.[8] Mercury's distance from Sun is 0.31 AU at perihelion (the closest approach to the sun), 0.47 AU at aphelion (its most distant point) and it has an orbital inclination of 7.0° relative to the solar plane.[9]

References

  1. Honey, I Shrunk the Solar System NASA. “The International Astronomical Union has decided that, to be called a planet, an object must have three traits. It must orbit the sun, be massive enough that its own gravity pulls it into a nearly round shape, and be dominant enough to clear away objects in its neighborhood.”
  2. Schenk P., Melosh H.J. (1994), Lobate Thrust Scarps and the Thickness of Mercury's Lithosphere, Abstracts of the 25th Lunar and Planetary Science Conference, 1994LPI....25.1203S
  3. Bill Arnett (2006). Mercury. The Nine Planets. Retrieved on 2006-09-14.
  4. Benz, W., Slattery, W. L., Cameron, A. G. W. (1988), Collisional stripping of Mercury's mantle, Icarus, v. 74, p. 516-528.
  5. Cameron, A. G. W. (1985), The partial volatilization of Mercury, Icarus, v. 64, p. 285-294.
  6. The effect of rotation National Maritime Museum
  7. What happens to the Sun's radiation when it reaches a planet?NMM
  8. A sidereal period is the time it takes a planet to return to an orbital position relative to the stars
  9. The orbits of the planets National Maritime Museum