Difference between revisions of "Mercury (planet)"
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== Explanation == | == Explanation == | ||
[[File:Flyby_color_photo_of_Mercury_from_MESSENGER.png|thumb|right|300px|A full-color composite image taken by MESSENGER spacecraft from its first Mercury [[planetary flyby|flyby]].]] | [[File:Flyby_color_photo_of_Mercury_from_MESSENGER.png|thumb|right|300px|A full-color composite image taken by MESSENGER spacecraft from its first Mercury [[planetary flyby|flyby]].]] | ||
| − | Mercury is the first [[planet]] in the [[solar system]], which is closest to the [[sun]]. It is also the smallest planet with the shortest [[orbital period]] among the other planets, lasting only 88 earth days. Mercury was initially thought to be [[tidal locking|tidally locked]] to the sun. But it was later discovered that Mercury indeed rotates, but slowly. The planet is tidally locked at a [[resonance]] due to its elliptic [[orbit]]. A day on Mercury is 58 Earth days, 15 hours, and 30 minutes. For every two orbital rotations around the Sun, Mercury rotates on its axis thrice. The other interesting fact about Mercury is its [[apsidal precession|orbital precession]] about 43 arc seconds per century, which proves [[general relativity]] more practically. | + | Mercury is the first [[planet]] in the [[solar system]], which is closest to the [[sun]]. It is also the smallest planet with the shortest [[orbital period]] among the other planets, lasting only 88 earth days. Mercury was initially thought to be [[tidal locking|tidally locked]] to the sun. But it was later discovered that Mercury indeed rotates, but slowly. The planet is tidally locked at a [[resonance]] due to its elliptic [[orbit]]. A [[sidereal time|sidereal day]] on Mercury is 58 Earth days, 15 hours, and 30 minutes. A [[solar day]] on Mercury is 176 Earth days. For every two orbital rotations around the Sun, Mercury rotates on its axis thrice. The other interesting fact about Mercury is its [[apsidal precession|orbital precession]] about 43 arc seconds per century, which proves [[general relativity]] more practically. |
Mercury is the second densest planet in the solar system, with a molten iron core that would make about 1800 km in radius.<ref> Finley, Dave (May 3, 2007). "Mercury's Core Molten, Radar Study Shows". National Radio Astronomy Observatory.</ref> For comparison, the total radius of Mercury is about 2440 km with a crust about 400 km thick. This molten core generates a strong magnetic field due to the [[dynamo theory|dynamo effect]], forming a [[magnetosphere]] around the planet. | Mercury is the second densest planet in the solar system, with a molten iron core that would make about 1800 km in radius.<ref> Finley, Dave (May 3, 2007). "Mercury's Core Molten, Radar Study Shows". National Radio Astronomy Observatory.</ref> For comparison, the total radius of Mercury is about 2440 km with a crust about 400 km thick. This molten core generates a strong magnetic field due to the [[dynamo theory|dynamo effect]], forming a [[magnetosphere]] around the planet. | ||
Revision as of 06:57, 11 January 2017
Contents
Explanation
Mercury is the first planet in the solar system, which is closest to the sun. It is also the smallest planet with the shortest orbital period among the other planets, lasting only 88 earth days. Mercury was initially thought to be tidally locked to the sun. But it was later discovered that Mercury indeed rotates, but slowly. The planet is tidally locked at a resonance due to its elliptic orbit. A sidereal day on Mercury is 58 Earth days, 15 hours, and 30 minutes. A solar day on Mercury is 176 Earth days. For every two orbital rotations around the Sun, Mercury rotates on its axis thrice. The other interesting fact about Mercury is its orbital precession about 43 arc seconds per century, which proves general relativity more practically.
Mercury is the second densest planet in the solar system, with a molten iron core that would make about 1800 km in radius.[1] For comparison, the total radius of Mercury is about 2440 km with a crust about 400 km thick. This molten core generates a strong magnetic field due to the dynamo effect, forming a magnetosphere around the planet.
Frequently Asked Questions
Why does the orbit of Mercury precess?
Almost all the orbits of the planets precess gradually due to the gravitational perturbation of the other planets. In the case of Mercury, the eccentricity of the orbit is different from other planets and Newton's theorem of revolving orbits could not explain it. Newton's theorem could account for the perturbation, Sun's little quadrupole moment and come up with a precession of 5557 arc seconds per century. But the observed precession is 5600 arc seconds per century and was higher by 43 arc seconds. It is proposed that there could be a planet or an asteroid belt beyond Mercury that could be contributing to the eccentricity. Later, as Einstein was able to predict the extra 43 arc seconds with general relativity, it is clear that Mercury is following the curved spacetime around the massive Sun, which results in the observed precession.
References
- ↑ Finley, Dave (May 3, 2007). "Mercury's Core Molten, Radar Study Shows". National Radio Astronomy Observatory.