Summary
Lacus Mortis /ˈleɪkəs ˈmɔːrtɪs/ (Latin mortis, "Lake of Death"[1]) is a hexagonal-shaped plain of basaltic lava flows in the northeastern part of the Moon's near face. It was formed as a floor-fractured crater during the pre-Imbrian epoch, then flooded during the late Imbrian period.[2] This feature lies just to the south of the elongated Mare Frigoris, being separated by a slender arm of rugged ground and linked at the eastern extreme. To the south is the Lacus Somniorum, separated from this mare by the joined craters Plana and Mason, and a strip of uneven surface.
 Lacus Mortis with crater Bürg | |
| Coordinates | 45°08′N 27°19′E / 45.13°N 27.32°E[1] |
|---|---|
| Diameter | 158.78 km[1] |
| Eponym | Lake of Death |
The name of this feature originated with the lunar nomenclature of Giovanni Riccioli, published in 1651 with the Almagestum Novum.[3] It was officially adopted by the IAU in 1935. The selenographic coordinates of the Lacus Mortis are 45.13° N, 27.32° E, and it has a diameter of 158.78 km (98.66 mi). The feature is positioned between lunar latitudes 42.5° to 47.75° north, and longitudes 23.61° to 31.03° east.[1]
The western edge of this mare forms a straight line, while the eastern edge is heavily eroded with open gaps.[4] Located prominently just to the east of the midpoint of this feature is the 40 km diameter impact crater Bürg.[5] This was formed during the Copernican period around 800 million years ago.[2] A pair of low ridges run north and south from Bürg crater to the mare rim.[4] The mare basalts, including those in the neighboring region of Mare Frigoris, are found to be richer in magnesium oxide (MgO) and aluminium oxide (Al2O3) compared to typical mare regions of the Moon, while iron oxide (FeO) is comparatively low in abundance.[6] A section of mare to the east of Bürg crater includes low concentrations of titanium oxide; less than 1.5% by concentration. It was likely delivered here as ejecta from a crater impact.[7]
The western part of the Lacus Mortis contains an extensive system of criss-crossing rilles collectively designated Rimae Bürg, spanning a length of 140 km.[8] The rilles are suspected to have formed from lava tubes.[5] There is a collapsed pit crater to the west of Bürg, at 44.96°N, 25.62°E, which may be an opening into a lava tube or cave.[9] This is the largest mare pit found as of 2012, measuring 100 × 150 m, with a floor about 90 m below the surrounding mare. The eastern wall of this pit appears to have collapsed, leaving a ramp with a ~22° slope extending from the mare to the floor.[10] Two small volcanoes are positioned along the southwest border of the mare with the highlands, to the south of a linear rille. They have a diameter of about 1.5 km and are similar in appearance to cinder or scoria cones on the Earth.[11]
Gallery edit
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Clementine mosaic of the Lacus Mortis region -
Oblique view from Apollo 16 -
This pit on Lacus Mortis has a collapsed eastern wall that could serve as a ramp -
The arrow points to lava domes to the south of a linear rille -
Closeup view of lava domes
See also edit
References edit
- ^ a b c d "Lacus Mortis". Gazetteer of Planetary Nomenclature. IAU. October 18, 2010. Retrieved 2021-01-06.
- ^ a b Clark, Mardi (February 2007). "Posidonius Area" (PDF). The Lunar Observer. Retrieved 2021-01-07.
- ^ Whitaker, Ewen A. (1999). Mapping and Naming the Moon. Cambridge University Press. pp. 60–61, 216. ISBN 0-521-62248-4.
- ^ a b Wilkinson, John (November 19, 2010). The Moon in Close-up: A Next Generation Astronomer's Guide. Springer Berlin Heidelberg. ISBN 9783642148057.
- ^ a b Hong, Ik-Seon; Yi, Yu; Yu, Jaehyung; Haruyama, Junichi (June 2015). "3D Modeling of Lacus Mortis Pit Crater with Presumed Interior Tube Structure". Journal of Astronomy and Space Science. 32 (2): 113–120. Bibcode:2015JASS...32..113H. doi:10.5140/JASS.2015.32.2.113.
- ^ Kramer, G. Y.; et al. (October 2015). "The basalts of Mare Frigoris". Journal of Geophysical Research: Planets. 120 (10): 1646–1670. Bibcode:2015JGRE..120.1646K. doi:10.1002/2014JE004753.
- ^ Rehfuss, D. E.; et al. (March 1978). "Delivery of VLT Basalt to Taurus-Littrow". Lunar and Planetary Science. 11: 952–954. Bibcode:1978LPI.....9..952R.
- ^ Lucchitta, B. K.; Watkins, J. A. (1978). Age of graben systems on the moon. Lunar and Planetary Science Conference, 9th, Houston, Tex., March 13–17, 1978, Proceedings. Vol. 3. New York: Pergamon Press, Inc. pp. 3459–3472. Bibcode:1978LPSC....9.3459L.
- ^ Urbancic, N.; et al. (March 2015). Exploring Lunar Sub-Surface Objects Using Surface Gravimetric Surveys. 46th Lunar and Planetary Science Conference, held March 16–20, 2015 in The Woodlands, Texas. LPI Contribution. Vol. 1832. p. 1616. Bibcode:2015LPI....46.1616U.
- ^ Wagner, R. V.; Robinson, M. S. (December 2012). Computer-Assisted Detection of Collapse Pits in LROC NAC Images. American Geophysical Union, Fall Meeting 2012. Bibcode:2012AGUFM.P53A2042W. P53A-2042.
- ^ "Volcanoes in Lacus Mortis". Lunar Reconnaissance Orbiter. NASA. August 10, 2010. Retrieved 2021-01-07.