Mercury has a year of only 88 Earth days and, because it spins more slowly than the Earth, one day on Mercury takes up to two thirds of its year. During one of Mercury’s long days, the Sun makes a complete loop in the sky due to changes in the planet’s speed around the Sun.
The surface of Mercury is covered in craters, as it has no atmosphere to protect it from meteorite impacts and no surface water, weather systems or volcanic activity to erode or cover them.
The surface of Mercury facing the Sun can reach temperatures of above 400 °C, while at night temperatures plummet to below -170 °C.
From Earth, because of its proximity to the Sun, Mercury can only be seen for about one hour before sunrise or after sunset, or during a total solar eclipse. Because, like Venus, Mercury’s orbit is inside that of the Earth, Mercury can be observed in transit as it passes across the disc of the Sun and exhibits phases similar to those of Venus or the Moon.
Warning: Never look through a telescope, or binoculars, pointed anywhere near the Sun, unless it is equipped with a specially designed solar filter. Also, do not look in the direction of the Sun without wearing eye protection such as safety glasses designed for observing a solar eclipse. Note that the Sun’s image can also be safely projected though a telescope onto a white screen behind the eyepiece, in order to observe transits of Mercury and Venus, although great care should be taken.
To find Mercury’s current position in the sky from your location, visit our Night Sky Simulator.
- Type: Terrestrial
- Diameter: 4,878 km (0.38 Earths)
- Mass: 3.3011×1023 (0.055 Earths)
- Distance from Sun: 0.466 to 0.307 AU
- Sidereal period (day length): 58.646 Earth days
- Orbital period (year length): 87.969 Earth days or 0.241 years
- Number of Moons: 0
- Symbol: ☿ (HTML code: ☿)