Mean distance from the Sun | 57.9 millions of Km (36 millions of miles) |
Revolution period | 87.969 days |
Rotational period | 58.6461 days |
Diameter | 4878 Km (3031 miles) |
Mass (Earth=1) | 0.055 |
Volume (Earth=1) | 0.056 |
Gravity (Earth=1) | 0.38 |
Number of satellites | 0 |
Mean temperature | +350 °C (day)
-170 °C (night) |
Minimum distance from the Earth | about 90 millions Km (56 millions of miles) |
Maximum distance from the Earth | about 200 millions Km (124 millions of miles) |
Generalities:
it is the planet nearest to the Sun. It has rather small dimensions
and it is a rocky planet.
It
is the thickest planet of the Solar System and for this reason its
metallic nucleus is supposed to occupy great part of the ray of the planet.
It is practically deprived of atmosphere: the presence of helium has been
noticed, probably captured by the solar wind in extremely small quantity.
Because of its proximity to the Sun, its diurnal temperatures are extremely
high. The lack of atmosphere exposing the planet to solar radiations
during the day, enables the heat to be quickly dispersed across
the space during the night, making the temperature fall toward
very low values. This procedure is helped by the slow rotation of the planet.
The proximity to the Sun also exposes Mercury to the bombardment
of the meteorites attracted by the strong solar gravity. For this reason
the small planet has a surface very rich in craters.
Observation: Mercury is a very elusive object in the terrestrial sky . The difficulty of observation lies in the fact that its permanence in the sky not illuminated by the Sun is limited to brief times after sunset or before dawn. For this reason Mercury cannot be ever observed in a completely dark sky. Being next to the sunset, or being risen by a little time it must then be observed when it is rather low in the sky. Its magnitude is very varied, since Mercury shows phases. Unlike Venus, which varies its distance from the Earth a lot, even if it shows phases,compensating, as far as brightness is concerned, the small phase with the greatest proximity to the Earth, Mercury, which varies less its distance from the Earth, is more influenced by the phase, showing different brightness. The magnitude can overcome -2 at the superior conjunction (completely illuminated, but not observable for the perspective proximity to the Sun) and go down beyond the value of +4 at the inferior conjunction (it shows the dark hemisphere). The visibility interval of interest (next to the maximum elongations) varies from -1 to +1. Because of its quick motion the observation periods last few days, but they are shown more times a year.
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Visibility
of planets during this month