|caption=Reprocessed Mariner 10 data was used to produce this image of Mercury. The smooth band is an area of which no images were taken.
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|caption=Reprocessed Mariner 10 data was used to produce this image of Mercury. The smooth band is an area of which no images were taken.
|discname=Known to ancients
|discname=Known to ancients
|origname=Roman messenger god<br>and prince of thieves
|origname=Roman messenger god<br>and prince of thieves
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:''For information about the NASA project, see [[Project Mercury]].''
:''For information about the NASA project, see [[Project Mercury]].''
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[[Mercury]] is the smallest planet in the [[Solar System]], and it is the closest to the [[Sun]]. It orbits the [[Sun]] in 88 (Earth) days. It rotates on its axis every 58.6 days,<ref>"The theory that Mercury is in [[synchronous rotation]] with its orbital motion was shattered in 1965. Astronomers Gordon Pettengill and Rolf Dyce used a radio telescope to make radar observations of Mercury’s spin rate. They found that Mercury’s rotation period is only 58.6 Earth days, not the 88 days accepted for nearly a century." [http://btc.montana.edu/messenger/elusive_planet/modern_times.htm]</ref> which is 3 rotations for every two orbits (called "3:2 resonance"). It can be seen from [[Earth]] only at sunrise and sunset.<ref name="spacemag">[http://www.space.com/spacewatch/mercury_view_030404.html Seeing Mercury at sunset], April 2003</ref>
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[[Mercury]] is the smallest planet in the [[Solar System]] and the closest to the [[Sun]]. It orbits the [[Sun]] in 88 Earth days and rotates on its axis every 58.6 Earth datesdays,<ref>"The theory that Mercury is in [[synchronous rotation]] with its orbital motion was shattered in 1965. Astronomers Gordon Pettengill and Rolf Dyce used a radio telescope to make radar observations of Mercury’s spin rate. They found that Mercury’s rotation period is only 58.6 Earth days, not the 88 days accepted for nearly a century." [http://btc.montana.edu/messenger/elusive_planet/modern_times.htm]</ref> which is 3 rotations for every two orbits (called "3:2 resonance"). It can be seen from [[Earth]] only at sunrise and sunset.<ref name="spacemag">[http://www.space.com/spacewatch/mercury_view_030404.html Seeing Mercury at sunset], April 2003</ref>