Mercury |
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| The planet Mercury |
category : planets |
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| Mercury is
the planet the closest to the sun and the smallest planet in the solar
system. Its size is about identical to our moon and their craters of
surface have really very in common. Mercury travels around the sun more
quickly than any other planet. She can only see itself of the earth just
before the sunrise or just after the sunset. Mercury never deviates from
more than 27 degrees of the Sun (it is the angle of the needles of a
watch when it is one o'clock). Mercury is a mysterious planet among
which only 45 percent of its surface was seen in the detail. It
possesses no satellite. Mercury has a very eccentric orbit which makes
vary its beam from 46 to 70 million kilometers. Its name comes from the
Roman god
Mercury Mercury (Roman) / Hermes ( Greek) is the god of the
Business, journeys and the messenger of the other gods in the Ancient
Rome and the empire Roman. His traditional attributes are the
scholarship, mostly held the hand, the winged Pégase or not, the
caduceus, the winged sandals as well as the cock and\or the billy goat..
The iron important proportion of Mercury intrigues the scientists. Three
hypotheses were proposed to explain the high content in metal of Mercury
and its gigantic nucleus. |
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- The rate of
heavy elements, as the iron, present in the solar nebula was more
important for the neighborhood of the Sun, even that these heavy
elements were gradually distributed around the Sun (the more we went
away from it, the less there was of heavy elements). Mercury, close to
the Sun, would thus have amassed more heavy materials than the other
planets to form its nucleus. |
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| Lower planet: Mercury |
category : planets |
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Mercury is a lower planet, thus included in the space of the orbit Earth Sun. Of this fact it presents phases as the Moon. Dense and rich iron, Mercury practically has no atmosphere. Mercury is easily visible with binoculars or even in the bare eye, but as it is always very close to the sun, it is difficult to see it in a enlightened sky. There are numerous Web sites which show the current position of Mercury (and the other planets) in the sky. We can observe the planets that because of the solar light which they reflect. Mercury, |
because of the strong percentage of variation of its
distance with the Earth, presents a strong variation of its visible
size. For Mercury the visible diameter of the disk varies between 4,8"
and 13,3". |
Because of the nearness of the Sun, the planet seems low on the horizon in the rise and in the sunset. Mercury is known since the period Sumerian (3000 years before J.C.). it received 2 names by Greek: Apollo for its appearance as morning star and Hermes as evening star. However, the Greek astronomers knew that it was about the one and only body. Greek Heraclius even believed that Mercury and Venus orbited around the Sun, but not the Earth. |
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| The orbit of Mercury |
category : planets |
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The orbit of Mercury is strongly eccentric; its perigee places it in only 46 million km of the Sun while its aphelia is 70 million km. Curiously, it crosses its orbit corresponding to its perigee in a very weak speed. The astronomers of the 19th century made very precise observations of the parameters orbital of Mercury but were able to explain them by basing itself on the mechanics Newtonians. |
The small difference between the observed values and
those predicted constituted a minor but disturbing problem during of
numerous decades. It was suggested that another planet (sometimes called
Red admiral) was able to exist in an orbit close to that of Mercury to
explain this difference. The true answer is given by the theory onto the
General Relativity of Einstein. |
The exactness of its prediction of the movement of Mercury was moreover a factor very important for the credibility of this theory. |
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| The day "Mercurial" |
category : planets |
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Until 1962, we believed that the day "Mercurial" had the same duration as its "year", so that Mercury had to present the same in front of Sun as the fact the Moon in front of the Earth. But in 1965, this was contradicted thanks to radar observations Doppler. We know from now on that Mercury makes 3 rotations on itself there 2 of its years. Mercury is the only body in the solar system known to have an echo orbit / rotation of a ratio other than 1:1. |
This echo and the eccentricity of its orbit would produce a strange spectacle for a possible observer on the surface of Mercury: in certain latitudes, the observer would see the Sun getting up then gradually increasing in visible size while he moves slowly towards the top. So the Sun would stop, would briefly backtrack, would stop again before taking back its road towards the horizon by decreasing in size. |
During all this time, stars would move 3 times as fast
in the sky. Observers situated in the other places of Mercury would see
different but so bizarre movements. |
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| The surface of Mercury |
category : planets |
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The images of the surface of Mercury look like the images of the moon; lava flows and varied craters of dimension harmonize to indicate us that Mercury as the Moon is a celestial body died since several billion years. Furthermore there is no atmosphere what forbids any aqueous and wind erosion. There is however a weak magnetic field. By many aspects, Mercury is very similar to the Moon: |
its surface is covered with craters and very former; it has no tectonic plate. On the other hand, Mercury is denser than the Moon (5,43 gm / cm3 against 3,34). Mercury is the densest 2nd planet in the solar system after the Earth. The density of the Earth is partially due to the gravitational compression; or, Mercury would be denser than it. This explains by the fact that the iron nucleus of Mercury is |
relatively bigger than that of the Earth, representing probably the majority of the planet. As a consequence, Mercury has a coat / crust of relatively fine silicates. Mercury has a big iron nucleus of a beam of 1800 in 1900 km. The envelope of silicates (similar to the coat and in earth's crusts) is only from 500 to 600 km. |
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| The atmosphere of Mercury |
category : planets |
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Mercury has a very fine atmosphere of atoms lifted by its surface by the solar wind. As Mercury is very warm, these atoms quickly escape in the space. The atmosphere of Mercury is permanently reconstituted. The surface of Mercury reveals enormous steep slopes, some making up to hundreds kilometers wide on 3000 m of height. Certain cuts in the rings of craters and other peculiarities of the relief of the same kind, show that |
these steep slopes were formed by compression. One of the biggest reliefs of the surface of Mercury, the basin Calorisin is one diameter of about 1300 km. It is known to be similar to the big basin (Maria) de la Lune). As for the lunar ponds, it was credibly caused by an enormous impact of meteorite. Besides its numerous craters, Mercury also has relatively flat plains. Some people could be the result of a volcanic activity and the |
others the consequence of a deposit of ejected stemming
from craters of impact. Curiously, radar observations of the North Pole
of Mercury (a region not mapped to Marinade 10) reveal the existence of
ice-cold water hidden in the shadow defender of certain craters. |
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Related subjects |
category: planets |
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Astronomy - october 15th 2007 |