Return to WNC Home Page Skip Navigation A-Z IndexMapsFaculty and Staff DirectoryContact Us

Jack C. Davis Observatory Planetary Walkway
Mercury


Previous: SunWalkway OverviewNext: Venus
Dedication: SBC is a proud partner of Western Nevada Community College. SBC is dedicated to its customers and to the communities in which we live.

SBC
Named after the Roman messenger of the gods, Mercury has almost no atmosphere and its surface is scarred by thousands of impact craters resulting from collisions with meteors.
Named after the Roman messenger of the gods, Mercury has almost no atmosphere and its surface is scarred by thousands of impact craters resulting from collisions with meteors.
Mean Distance from Sun
57.9 milion kilometers
Orbital Period
88 days
Rotational Period
58 days 39 minutes
The smallest of the 4 terrestrial (rocky) planets and the planet that is most similar in its outer appearance to Earth's Moon. Mercury is very close to the Sun and never exceeds an angular distance of 28° from the direct line of sight of the Sun. Mercury can only be seen at most 2 hours on any given night or morning that is favorable for viewing.

Mercury less than 1/3 of the distance the Earth is from the Sun (0.31 A. U.). The planet can reach a scorching 700 K (800°F) during the day to 100 K (-280° F) at night.

Mercury rotates on its axis very slowly. The orbital period of Mercury is equivalent to 88 Earth days and its rotation rate is 59 Earth days. Mercury is considered speedy because it moves quickly around the Sun (less than ¼ of an Earth year) and Mercury was named after the Roman god of commerce and thievery. Although the entire surface of Mercury has not been observed yet it has many craters one of which is the result of a major impact of an asteroid that sent shock waves through the core of the planet. This impact formed the Caloris Basin that eventually filled with lava from below.
Previous: SunWalkway OverviewNext: Venus
The Image Processing Lab at NASAs Jet Propulsion Laboratory produced this photomosaic using computer software and techniques developed for use in processing planetary data. The Mariner 10 spacecraft imaged the region during its initial flyby of the planet. Image courtesy NASA Jet Propulsion Laboratory (NASA-JPL).
The Image Processing Lab at NASA's Jet Propulsion Laboratory produced this photomosaic using computer software and techniques developed for use in processing planetary data. The Mariner 10 spacecraft imaged the region during its initial flyby of the planet. Image courtesy NASA Jet Propulsion Laboratory (NASA-JPL).

Return to WNC Home Page © 2007 Western Nevada College
Privacy Policy | Site Policies | WNC en Español | Home
Information: 775-445-3000
General Questions: info_desk@wnc.edu