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Mercury's surface closely resembles the Moon's. It is covered by impact craters, ancient lava flows, and quake fault lines. Mile-high cliffs stretch for hundreds of miles across the planet's surface. The huge Caloris impact basin, 800 miles (1,300 km) wide, decorates one side of the planet.
Mercury is only about six percent as massive as Earth, but it is about the same density. It is dominated by its iron core, which makes up 70 percent of its mass. The core may be partly molten, which would explain the presence of Mercury's weak magnetic field, which is just one percent as strong as Earth's. Above the core, Mercury has a thin mantle and crust.
A thin but strong wind from the Sun blasts particles off of Mercury's hard surface, creating a thin atmosphere around the planet. The particles rapidly escape into space, even as the never-ending solar wind blasts more material from the surface.
Mercury speeds around the Sun faster than any other planet. Its 88-day, highly elliptical orbit brings it within 29 million miles (47 million km) of the Sun, and then swings it out to 44 million miles (70 million km).
In the 1800s, astronomers realized that the physics of the day could not correctly predict Mercury's orbital path. The reason remained a mystery until 1915, when Albert Einstein used his new theory of gravity, General Relativity, to correctly predict Mercury's orbit -- and explained the reason for previous errors: Mercury is so close to the Sun that its orbit is affected by the "warp" in space created by the Sun's powerful gravitational field.
From Earth, we view the same side of Mercury each time it passes closest to our planet. For a long time, this caused astronomers to think that the planet was tidally locked with the Sun -- that is, its day and year were of equal length. Not so; in 1965, radar observations showed that Mercury completes three spins on its axis for every two orbits around the Sun.
The planet's surface swings through extremes of temperature. In the daytime, it can reach 700 degrees Fahrenheit (315 C). At night, the temperature drops to –300 F (–183 C). Radar observations suggest that water ice might inhabit shadowed craters at Mercury's poles. These regions never see the Sun, so the ice would not vaporize into space.
Mercury's distance and proximity to the Sun make it difficult to study with ground-based telescopes. It's only visible just after sunset or just before sunrise, forcing astronomers to view it through a thick, turbulent layer of Earth's atmosphere.
Only two spacecraft have visited Mercury. Mariner 10 flew by the planet three times in 1974 and 1975, and mapped about half of Mercury's surface. NASA's MESSENGER spacecraft made three passes of its own more than three decades later. In March 2011 it became the first spacecraft to orbit Mercury. It is scheduled to end its mission in early 2015.
☿The Sun’s closest planet is at its best this year in the dawn sky in mid- September, and in the evening sky in early April.
Only two spacecraft have visited Mercury. Mariner 10 flew by the planet three times in 1974 and 1975, and mapped about half of its battered, Moon-like surface, which is dominated by impact craters. Mariner found that Mercury's interior consists of a large iron-rich core, which generates a weak magnetic field around the planet. Messenger flew by Mercury three times in the early 2000s, and entered orbit around the planet in March 2011. More »
At a Glance
|Known since antiquity|
|Roman messenger god|
|Average distance from Sun|
0.387 Astronomical Unit
|0.055 times Earth's mass|
|Length of Day|
|58.65 Earth days|
|Length of Year|
|0.24 Earth years
88 Earth days
|0.38 that of Earth (If you weigh 100 pounds, you would weigh about 38 pounds on Mercury.)|
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The Astro Guides for the Solar System and Beyond the Solar System are supported by the National Aeronautics and Space Administration under Grant Nos. NNG04G131G and NAG5-13147, respectively.