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|Diameter||389 km (242 mi)|
|Eponym||Sea of Moisture|
It was not sampled by the Apollo program, so a precise age has not been determined. However, geological mapping indicates that it is intermediate in age between the Imbrium and Nectaris Basins, suggesting an age of about 3.9 billion years. Humorum Basin is filled with a thick layer of mare basalt, believed to exceed 3 kilometers in thickness at the center of the basin.
A mass concentration (mascon), or gravitational high, was identified in the center of Mare Humorum from Doppler tracking of the five Lunar Orbiter spacecraft in 1968. The mascon was confirmed and mapped at higher resolution with later orbiters such as Lunar Prospector and GRAIL.
Gravity map based on GRAIL
Like most of the other maria on the Moon, Mare Humorum was named by Giovanni Riccioli, whose 1651 nomenclature system has become standardized. Previously, the 17th century astronomer Pierre Gassendi had named it Anticaspia ('opposite to the Caspian', referring to Mare Crisium, which he had named after the Caspian Sea), and Michael Van Langren had labelled it the Mare Venetum ("Venetian Sea") in his 1645 map. Johannes Hevelius called it Sinus Sirbonis ("Bay of Serbonis", after the lake of Serbonis, now Lake Bardawil, in Egypt) in his 1647 map.
- "Moon Mare/Maria". Gazetteer of Planetary Nomenclature. USGS Astrogeology. Retrieved 2010-08-20.
- D. Ben J. Bussey et al., "Humorum Basin Geology from Clementine Data," Lunar and Planetary Science Conference XXVIII (1997)
- P. M. Muller, W. L. Sjogren (1968). "Mascons: Lunar Mass Concentrations". Science. 161 (3842): 680–684. doi:10.1126/science.161.3842.680.
- Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.61.
- Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.33
- Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p.41, 198.
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