Physics
Scientific paper
Jun 1975
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1975jgr....80.2415k&link_type=abstract
Journal of Geophysical Research, vol. 80, June 10, 1975, p. 2415, 2416.
Physics
3
Mariner Venus-Mercury 1973, Mercury (Planet), Planetary Rotation, Planetary Surfaces, Spaceborne Photography, Error Analysis, High Resolution, Orbital Elements, Synchronism, Time Measurement
Scientific paper
The rotation period of Mercury has been determined to be 58.661 days by using high-resolution photography from the Mariner 10 mission. This value matches the period required for 3/2 synchronism with the orbital period (58.6462 days) within the 1-sigma errors assigned and is consistent with the latest values derived from radar and earth-based telescopic observations.
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