Surface Temperature

Two Mercury years

Ls = 0 degrees
Ls = 180 degrees
Ls = 0 degrees
Ls = 180 degrees
Ls = 0 degrees

Perihelion
Noon at 0o Longitude

Aphelion
Noon at 90o Longitude

Perihelion
Noon at 180o Longitude

Aphelion
Noon at 270o Longitude

Perihelion
Noon at 0o Longitude

Temperature animation

Mercury experiences extreme temperature variations on its surface because, like out Moon, Mercury lacks a substantial atmosphere to buffer surface temperatures. Without the moderating effects of an atmosphere or oceans like the Earth, the intense solar radiation (the sun appears about 2½ times larger in Mercury's sky) results in surface temperatures reaching an extreme 700 K (801 oF or 427 oC) at the subsolar point (local noon time). The nights on Mercury are long due to its slow rotation. Since there is no atmosphere to trap heat, it radiates from the surface directly into space at night and the surface gets very cold, about 90 K (-297 oF or -183 oC). Such temperature extremes do not occur on planets with atmospheres due to the insulating effects of the atmospheres that moderate temperature extremes and maintain a warmer temperature at night (the greenhouse effect).

Special thanks to David Paige at UCLA Earth and Space Sciences for the Mercury surface temperatures (http://diviner.ucla.edu)

See References for details:
(1) Paige D. A., S. E. Woods and A. R. Vasavada, "The thermal stability of water ice at the poles of Mercury", Science 258, 643–646, 1992.
(2) Vasavada, A. R., D. A. Paige and S. E. Wood, "Near-surface temperatures on Mercury and the Moon and the stability of polar ice deposits", Icarus 141, 179–193, 1999.