Mercury

Mercury
Number of Sattelites	None
Atmospheric Makeup	41.5% molecular oxygen; 29% sodium; 22% hydrogen; 6% helium; 0.48% potassium
Distance from Sun	48 million miles (from Earth) 57.91 million km (from The Sun)
Diameter	3032 miles; 4880 kilometers
Volume	6.083×1010 km3 0.056 Earths
Axial tilt	2.11 degrees
Orbit	88 Earth days 59 days axis
Position in Solar System	First planet from Sun
Surface Features	Cratered surface
Albedo	(geometric) 0.142; (bond) 0.068
Aphelion	43.64 million miles
Perihelion	28.75 million miles
Mass of Planet	3.302 x 10^23 kg
Escape Velocity	4.25 kilometers/second

Mercury

Even though Mercury is the closest planet to the Sun, it is not the hottest (which the title belongs to Venus) but that doesn't mean its temperature is bland. A day on Mercury is 430 degrees Celsius in temperature and a night on Mercury can freeze at a temperature of -180 degrees Celsius. Why does Mercury have an extremely large temperature range? That's because of its atmosphere. Mercury's atmosphere is so thin that it's barely a metric ton dense. The thin atmosphere allows most of the space radiation, heat, and coldness from the Sun to arrive at the surface.

Formation[]

There are two theories of Mercury being formed.

Mercury could have been a gas giant (most likely a hot jupiter) that orbited too close to the Sun and its atmosphere vaporized, leaving only its rocky core behind.

2. Mercury formed just like all the other terrestrial planets, as first a volcanic clump of asteroids and particles. It was the third planet from the Sun but its orbit was disturbed by the Sun's gravity and was placed as the first planet.

Atmosphere[]

As you saw in the introduction, Mercury only has 2200 pounds of atmosphere. It is made up of about forty percent oxygen, about twenty percent sodium, about twenty two percent hydrogen, and about ten percent helium. The last one percent is made up of trace gases. The atmosphere of Mercury is produced from the heat within the planet.

Surface[]

The surface of Mercury is heavily cratered. The best known of these craters is the Caloris Basin, which is about one thousand miles in width. Ancient volcanoes show signs that volcanism was once present on this planet. The rest of the surface include cliffs and plains that became solid, which is a process called solidification. This solidification created these volcanoes.

Structure[]

The core is thought to consist of iron, which happened due to the amount of accretion the nebula received when it created the Solar System. Around that is a silicate mantle, where the convection currents occur, shifting tectonic plates. The last is the crust, which suffers from asteroid impacts and volcanism.

Observation[]

Mercury can be easily seen during twilight or just after the sunset. The visibility cannot remain for long due to its speedy orbit around the Sun. The elongation, or the point at which a celestial object is at its farthest point from a solar remnant, of Mercury from the Sun is the best time to view it, though this event only occurs seven times a year.