Astronomy:Mare Imbrium

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Short description: Vast lunar mare filling a basin on Earth's Moon
Mare Imbrium
Imbrium location.jpg
A map showing the location of Mare Imbrium
Diameter1,146 km (712 mi)[1]


LRO mosaic of Mare Imbrium
Detail map of Imbrium's features
Detail of basaltic lava flow fronts within Mare Imbrium, located north of Euler crater. (Mosaic of Apollo 17 images.)

Mare Imbrium /ˈɪmbriəm/ (Latin imbrium, the "Sea of Showers" or "Sea of Rains", "Sea of Tears") is a vast lava plain within the Imbrium Basin on the Moon and is one of the larger craters in the Solar System. The Imbrium Basin formed from the collision of a proto-planet during the Late Heavy Bombardment. Basaltic lava later flooded the giant crater to form the flat volcanic plain seen today. The basin's age has been estimated using uranium–lead dating methods to approximately 3.9 billion years ago, and the diameter of the impactor has been estimated to be 250 ± 25 km.[2] The Moon's maria (plural of mare) have fewer features than other areas of the Moon because molten lava pooled in the craters and formed a relatively smooth surface. Mare Imbrium is not as flat as it was originally thought, because later events have altered its surface.

Origin

Mare Imbrium formed when a proto-planet from the asteroid belt collided with the Moon during the Late Heavy Bombardment.[3] The impact is dated to approximately 3922 ± 12 million years ago, based on radiometric dating techniques. Ejecta from the impact covers large areas of the near side of the Moon.[4][5]

Characteristics

With a diameter of 1145 km, Mare Imbrium is second only to Oceanus Procellarum in size among the maria, and it is the largest mare associated with an impact basin.

The Imbrium Basin is surrounded by three concentric rings of mountains, uplifted by the colossal impact event that excavated it. The outermost ring of mountains has a diameter of 1300 km and is divided into several different ranges; the Montes Carpatus to the south, the Montes Apenninus to the southeast, and the Montes Caucasus to the east. The ring mountains are not as well developed to the north and west, and it appears they were simply not raised as high in these regions by the Imbrium impact. The middle ring of mountains forms the Montes Alpes and the mountainous regions near the craters Archimedes and Plato. The innermost ring, with a diameter of 600 km, has been largely buried under the mare's basalt leaving only low hills protruding through the mare plains and mare ridges forming a roughly circular pattern.

Selenochromatic Image (Si) of Mare Imbrium

The outer ring of mountains rise roughly 7 km above the surface of Mare Imbrium. The Mare material is thought to be about 5 km deep, giving the Imbrium Basin a total depth of 12 km; it is thought that the original crater left by the Imbrium impact was as much as 100 km deep, but that the floor of the basin bounced back upwards immediately afterwards.

Oblique view of Imbrium Sculpture, with the crater Ukert right of center

Surrounding the Imbrium Basin is a region blanketed by ejecta from the impact, extending roughly 800 km outward. Also encircling the basin is a pattern of radial grooves called the "Imbrium Sculpture", which have been interpreted as furrows cut in the Moon's surface by large projectiles blasted out of the basin at low angles, causing them to skim across the lunar surface ploughing out these features. The sculpture pattern was first identified by Grove Karl Gilbert in 1893.[6] Furthermore, a Moon-wide pattern of faults which run both radial to and concentric to the Imbrium basin were thought to have been formed by the Imbrium impact; the event literally shattered the Moon's entire lithosphere. At the region of the Moon's surface exactly opposite Imbrium Basin, there is a region of chaotic terrain (the crater Van de Graaff) which is thought to have been formed when the seismic waves of the impact were focused there after travelling through the Moon's interior. Mare Imbrium is about 750 miles (1,210 km) wide.

A mass concentration (mascon), or gravitational high, was identified in the center of Mare Imbrium from Doppler tracking of the five Lunar Orbiter spacecraft in 1968.[7] The Imbrium mascon is the largest on the Moon. It was confirmed and mapped at higher resolution with later orbiters such as Lunar Prospector and GRAIL.

  • Shaded Relief map

  • Gravity map based on GRAIL

Names

Like most of the other maria on the Moon, Mare Imbrium was named by Giovanni Riccioli, whose 1651 nomenclature system has become standardized.[8]

The earliest known name for the mare may be "The Shrine of Hecate"; Plutarch records that the Ancient Greeks gave this name to the largest of the "hollows and deeps" on the Moon, believing it to be the place where the souls of the deceased were tormented. Ewen A. Whitaker argues that this likely refers to Mare Imbrium, "the largest regular-shaped dark area unbroken by bright patches" that can be seen with the naked eye.[9]

Around 1600, William Gilbert made a map of the Moon that names Mare Imbrium "Regio Magna Orientalis" (the Large Eastern Region). Michael van Langren's 1645 map named it "Mare Austriacum" (the Austrian Sea).[10]

Observation and exploration

Mare Imbrium is visible to the naked eye from Earth. In the traditional 'Man in the Moon' image seen on the Moon in Western folklore, Mare Imbrium forms the man's right eye.[11]

Luna 17

On 17 November 1970 at 03:47 Universal Time, the Soviet spacecraft Luna 17 made a soft landing in the mare, at latitude 38.28 N, and longitude 35.00 W. Luna 17 carried Lunokhod 1, the first robotic rover to be deployed on the Moon or any extraterrestrial body. Lunokhod 1, a remote-controlled rover, was successfully deployed and undertook a mission lasting several months.

Apollo 15

In 1971, the crewed Apollo 15 mission landed in the southeastern region of Mare Imbrium, between Hadley Rille and the Apennine Mountains. Commander David Scott and Lunar Module Pilot James Irwin spent three days on the surface of the Moon, including 18½ hours outside the spacecraft on lunar extra-vehicular activity. Command Module Pilot Alfred Worden remained in orbit and acquired hundreds of high-resolution photographs of Mare Imbrium (and other regions of the Moon) as well as other types of scientific data. The crew on the surface explored the area using the first lunar rover and returned to Earth with 77 kilograms (170 lb) of lunar surface material. Samples were collected from Mons Hadley Delta, believed to be a fault block of pre-Imbrian (Nectarian or Pre-Nectarian) lunar crust, including the "Genesis Rock." This was also the only Apollo mission to visit a lunar rille, and to observe outcrops of lunar bedrock visible in the rille wall.[12]

2013 Impact

On 17 March 2013, an object hit the lunar surface in Mare Imbrium and exploded in a flash of apparent magnitude 4.[13] The resulting crater was 18 meters wide.[14] This was the brightest impact recorded since NASA's lunar impact team began monitoring in 2005.

Chinese landing

Main pages: Astronomy:Chang'e 3 and Engineering:Yutu (rover)
The planned landing site for Chang'e 3 was Sinus Iridum. The actual landing took place on Mare Imbrium

Chang'e 3 landed on 14 December 2013 on Mare Imbrium, about 40 km south of the 6 km diameter Laplace F crater,[15][16] at 44.1260°N 19.5014°W.[16][17][18] The lander deployed the Yutu rover 7 hours and 24 minutes later.[19] Chang'e 3 mission attempted to perform the first direct measurement of the structure and depth of the lunar soil down to a depth of 30 m (98 ft), and investigate the lunar crust structure down to several hundred meters deep.[20] The rover's ground penetrating radar found evidence of at least nine distinct rock layers, indicating that the area had surprisingly complex geological processes and is compositionally distinct from the Apollo and Luna landing sites.[21][22]

See also

References

  1. ↑ "Mare Imbrium". Gazetteer of Planetary Nomenclature. USGS Astrogeology Research Program.
  2. ↑ P. H. Schultz & D.A. Crawford, Origin and implications of non-radial Imbrium Sculpture on the Moon, Nature 535, 391–394 (2016)
  3. ↑ Merle, R. E.; Nemchin, A. A.; Grange, M. L.; Whitehouse, M. J.; Pidgeon, R. T. (2014). "High resolution U-Pb ages of Ca-phosphates in Apollo 14 breccias: Implications for the age of the Imbrium impact". Meteoritics & Planetary Science 49 (12): 2241–2251. doi:10.1111/maps.12395. Bibcode: 2014M&PS...49.2241M. 
  4. ↑ Nemchin, Alexander A.; Long, Tao; Jolliff, Bradley L.; Wan, Yusheng; Snape, Joshua F.; Zeigler, Ryan; Grange, Marion L.; Liu, Dunyi et al. (2021-04-01). "Ages of lunar impact breccias: Limits for timing of the Imbrium impact" (in en). Geochemistry 81 (1): 125683. doi:10.1016/j.chemer.2020.125683. ISSN 0009-2819. Bibcode: 2021ChEG...81l5683N. 
  5. ↑ Zhang, Bidong; Lin, Yangting; Moser, Desmond E.; Hao, Jialong; Shieh, Sean R.; Bouvier, Audrey (December 2019). "Imbrium Age for Zircons in Apollo 17 South Massif Impact Melt Breccia 73155" (in en). Journal of Geophysical Research: Planets 124 (12): 3205–3218. doi:10.1029/2019JE005992. ISSN 2169-9097. Bibcode: 2019JGRE..124.3205Z. https://onlinelibrary.wiley.com/doi/abs/10.1029/2019JE005992. 
  6. ↑ Gilbert, Grove Karl. The Moon's face, a study of the origin of its features. Washington, Philosophical Society of Washington, 1893.
  7. ↑ P. M. Muller, W. L. Sjogren (1968). "Mascons: Lunar Mass Concentrations". Science 161 (3842): 680–684. doi:10.1126/science.161.3842.680. PMID 17801458. Bibcode: 1968Sci...161..680M. 
  8. ↑ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 61.
  9. ↑ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 7
  10. ↑ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), pp. 15, 41.
  11. ↑ Ewen A. Whitaker, Mapping and Naming the Moon (Cambridge University Press, 1999), p. 3. [ISBN missing]
  12. ↑ Apollo 15 Preliminary Science Report (NASA SP-289), Scientific and Technical Information Office, National Aeronautics and Space Administration, Washington, D.C., 1972.
  13. ↑ Dr. Tony Phillips (17 May 2013). "Bright Explosion on the Moon". Science@NASA. https://science.nasa.gov/science-news/science-at-nasa/2013/16may_lunarimpact/. 
  14. ↑ NASA's Goddard Space Flight Center (17 March 2015). "New Craters on the Moon". Goddard Media Studios. https://svs.gsfc.nasa.gov/11806. 
  15. ↑ "Chang'e 3 landing coordinates". China News (CN). 14 December 2013. http://planetary.s3.amazonaws.com/assets/images/3-moon/20131214_change_landing_location.jpg. 
  16. ↑ 16.0 16.1 Emily Lakdawalla; Phil Stooke (December 2013). "Chang'e 3 has successfully landed on the Moon!". The Planetary Society. http://www.planetary.org/blogs/emily-lakdawalla/2013/12140619-change-3-has-successfully-landed.html. 
  17. ↑ "China successfully lands robotic rover on the moon>". http://www.spaceflightnow.com/china/change3/131214landing/#.Uqzk7EAwCZA. 
  18. ↑ "Landing map of Chang'e 3". http://ww2.sinaimg.cn/mw1024/5f50f3afgw1ebjm28fzibj20v31rjgvr.jpg. 
  19. ↑ O'Neil, Ian (14 December 2013). "China's Rover Rolls! Yutu Begins Moon Mission". Discovery News (CCTV). http://news.discovery.com/space/chinas-rover-rolls-yutu-begins-moon-mission-131214.htm. 
  20. ↑ "欧阳自远：嫦娥三号明年发射将实现着陆器与月球车联合探测". Xinhua. 14 June 2012. http://news.xinhuanet.com/politics/2012-06/14/c_112217044.htm. 
  21. ↑ Wall, Mike (12 March 2015). "The Moon's History Is Surprisingly Complex, Chinese Rover Finds". Space.com. http://www.space.com/28810-moon-history-chinese-lunar-rover.html?adbid=10152690360766466&adbpl=fb&adbpr=17610706465. 
  22. ↑ Xiao, Long (13 March 2015). "A young multilayered terrane of the northern Mare Imbrium revealed by Chang'E-3 mission". Science 347 (6227): 1226–1229. doi:10.1126/science.1259866. PMID 25766228. Bibcode: 2015Sci...347.1226X. 

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