Mare Humboldtianum

Mare Humboldtianum /hʌmboʊltiˈeɪnəm/ (Latin humboldtiānum, the "Sea of Alexander von Humboldt") is a lunar mare located just to the east of Mare Frigoris, in the center of Humboldtianum basin. It is located along the northeastern limb of the Moon, and continues on to the far side. Due to its location, the visibility of this feature can be affected by libration, and on occasion it can be hidden from view from Earth.

Mare Humboldtianum
Mare Humboldtianum is the smooth dark patch. The upper right is occupied by the walled plain Bel'kovich. Clementine image.
Coordinates56.9°N 81.5°E / 56.9; 81.5
Diameter230 km (140 mi)[1]
EponymSea of Alexander von Humboldt
Elevation map of Humboldtianum basin
Oblique view from Apollo 16

The basin material is of the Nectarian epoch,[2] with the mare material being of the Upper Imbrian epoch (3.4–3.7 Ga).[3] The lighter gray area to the southeast of the dark mare material is a region of hills within the basin. The rim of this basin forms a mountain range that can be seen under oblique lighting conditions.

This mare is centered at 56.9° N, 81.5° E, and its maximal size is 230 km. However the surrounding basin extends for a diameter of over 600 km. The walled plain Bel'kovich spills over the northwestern portion of Mare Humboldtianum, and the flooded crater Bel'kovich A lies across the southwestern rim of Bel'kovich and part of the floor of the mare.

At the center of the Humboldtianum basin is a mascon, or gravitational high. The mascon was first identified by Doppler tracking of the Lunar Prospector spacecraft.[4]

This mare is situated between near (visible) and far sides of the Moon, like a link between known and unknown. That's why Johann Mädler named it after Alexander von Humboldt, a prominent explorer of unknown lands.[5] It is one of only two lunar maria that are named after people, the other being Mare Smythii (named after British astronomer William Henry Smyth), and is located along the eastern lunar limb.

References
  1. "Mare Humboldtianum". Gazetteer of Planetary Nomenclature. USGS Astrogeology. Retrieved 2015-05-19.
  2. Fassett, C. I.; Head, J. W.; Kadish, S. J.; Mazarico, E.; Neumann, G. A.; Smith, D. E.; Zuber, M. T. (2012). "Lunar impact basins: Stratigraphy, sequence and ages from superposed impact crater populations measured from Lunar Orbiter Laser Altimeter (LOLA) data" (PDF). Journal of Geophysical Research. 117 (E12): n/a. Bibcode:2012JGRE..117.0H06F. doi:10.1029/2011JE003951. hdl:1721.1/85892.
  3. Hiesinger H., Head J. W., Wolf U., Jaumann R., Neukum G. (2011). "Ages and stratigraphy of lunar mare basalts: A synthesis" (PDF). In W. A. Ambrose, D. A. Williams (ed.). Recent Advances and Current Research Issues in Lunar Stratigraphy. Geological Society of America Special Paper 477. 477. Geological Society of America. pp. 30–31. doi:10.1130/2011.2477(01). ISBN 978-0-8137-2477-5.CS1 maint: multiple names: authors list (link)
  4. A. S. Konopliv; A. B. Binder; L. L. Hood; A. B. Kucinskas; W. L. Sjogren & J. G. Williams (1998). "Improved Gravity Field of the Moon from Lunar Prospector". Science. 281 (5382): 1476–1480. Bibcode:1998Sci...281.1476K. doi:10.1126/science.281.5382.1476. PMID 9727968.
  5. Rükl A. (2004). G. Seronik (ed.). Atlas of the Moon. Cambridge, Massachusetts: Sky Publishing Corp. pp. 40–41. ISBN 978-1-931559-07-2.
This article is issued from Wikipedia. The text is licensed under Creative Commons - Attribution - Sharealike. Additional terms may apply for the media files.