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Oceanus Procellarum

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a billion years younger than any other previously returned lunar sample. Late lunar volcanic activity was considered surprising as the Moon is much smaller than Earth; interior heat necessary for volcanism should have been lost three billion years ago, so volcanic rocks as late as those found in Oceanus Procellarum must require additional heat sources.
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During the Apollo program, flight operations planners were concerned about having the optimum lighting conditions at the landing site, hence the alternative target sites moved progressively westward, following the terminator. A delay of two days for weather or equipment reasons would have sent Apollo
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Relatively recent (less than 2 bya) volcanic activity had been suspected in the Oceanus Procellarum due to the presence of relatively uneroded features. The 2020 Chang'e-5 sample return mission provided constraints on the age of Oceanus Procellarum, finding it to be 1963 ± 57 million years old – over
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There are several hypotheses about the origin of Oceanus Procellarum and a related asymmetry between the near and far sides of the Moon. One of the most likely is that Procellarum was a result of an ancient giant impact on the near side of the Moon. The size of the impact basin has been estimated to
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Previous studies suggested that Oceanus Procellarum should have high concentrations of the heat-producing elements such as potassium, thorium, and uranium, but samples returned showed that the concentration of suspected radioactive elements is much lower than necessary to provide prolonged heating.
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Procellarum may have also been formed by spatially inhomogeneous heating during the Moon's formation. The GRAIL mission, which mapped the gravity gradients of the Moon, found square formations resembling rift valleys surrounding the region beneath the lava plains, suggesting the basin was formed by
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Nakamura, R.; Yamamoto, S.; Matsunaga, T.; Ishihara, Y.; Morota, T.; Hiroi, T.; Takeda, H.; Ogawa, Y.; Yokota, Y.; Hirata, N.; Ohtake, M.; Saiki, K. (2012). "Compositional evidence for an impact origin of the Moon's Procellarum basin".
376:. Basalts in Oceanus Procellarum have been estimated to be as young as one billion years old. Unlike the other lunar maria, however, Oceanus Procellarum may or may not be contained within a single, well-defined impact basin. 532:
Other hypotheses include a late accretion of a companion Moon on the far side. The latter postulates that in addition to the present Moon, another smaller (about 1,200 km in diameter) moon was formed from debris of the
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still existed or just ceased to exist. It deposited 5–30 km of crustal material on the far side forming highlands. If this is the case, all impact related structures such as crater
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nearly 165 meters from Surveyor 3 in Oceanus Procellarum. Their landing site has become known as Statio Cognitum (Latin, "to be known from experience").
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heating and cooling of the lunar surface by internal processes rather than by an impact, which would have left a round crater.
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lies within the eastern edge of the mare, distinct with its bright ray materials sprawling over the darker material.
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Jutzi, M.; Asphaug, E. (2011). "Forming the lunar farside highlands by accretion of a companion moon".
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in Oceanus Procellarum in December 2020 and collected 1.73 kg (3.8 lb) of lunar rock samples.
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Gravity anomalies (red) bordering the Procellarum region overlaid on a global elevation map
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Che, Xiaochao; Nemchin, Alexander; Liu, Dunyi; Long, Tao; Wang, Chen; Norman, Marc D.;
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The 'oceanus' area in a Selenochromatic Image (Si); targeted some chromatic landmarks
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crater (within the larger Flamsteed P) in 1966, and Surveyor 3 landed in 1967. The
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The impact likely happened very early in the Moon's history: at the time when
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due to the abundance of their radioactive isotopes providing heat from decay
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floods that covered the region in a thick, nearly flat layer of solidified
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Most of the dark region is Oceanus Procellarum and smaller maria, such as
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to the south. To the northeast, Oceanus Procellarum is separated from
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Vast lunar mare on the western edge of the near side of Earth's Moon
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Byrne, C. J. (2008). "A Large Basin on the Near Side of the Moon".
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Like all lunar maria, Oceanus Procellarum was formed by ancient
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landing site (center) used in mission planning (1.75 x 1.75 km)
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Around its edges lie many minor bays and seas, including
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Jennifer Hauser and Zamira Rahim (16 December 2020).
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Andrea Thompson 06 November 2008 (6 November 2008).
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October 2012, Charles Q. Choi 29 (29 October 2012).
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one of the three largest craters in the Solar System
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Luna 13 landed southeast of 8: 150: 817:: CS1 maint: numeric names: authors list ( 778:: CS1 maint: numeric names: authors list ( 1260: 1246: 1238: 127:Learn how and when to remove this message 614: 1637: 1208: 718: 810: 795:"Signs of Late Volcanism Seen on Moon" 771: 149: 341:'Ocean of Storms') is a vast 7: 749: 747: 65:adding citations to reliable sources 731:Gazetteer of Planetary Nomenclature 632:(designated ALS3) instead of ALS2— 25: 979:(Press release). NASA. 2014-10-01 1688: 1676: 1664: 1652: 1640: 471: 455: 435: 241: 156: 41: 52:needs additional citations for 608:landed at Statio Tianchuan on 1: 1115:Jones, Andrew (8 July 2021). 655:landed the Lunar Module (LM) 482:– closeup (artist's concept). 220:2,592 km (1,611 mi) 1163:"Apollo 12 Mission Overview" 525:around Oceanus Procellarum. 345:on the western edge of the 1737: 29: 1620:List of maria on the Moon 1615: 955:10.1007/s11038-007-9225-8 639:During the November 1969 155: 935:Earth, Moon, and Planets 697:Human Lunar Return study 1078:10.1126/science.abl7957 947:2007EM&P..101..153B 448:GRAIL gravity gradients 368:eruptions resulting in 624: 494: 412:Aristarchus ray crater 331: 144: 727:"Oceanus Procellarum" 707:Volcanism on the Moon 618: 492: 142: 76:"Oceanus Procellarum" 841:US Geological Survey 833:"Sinus Viscositatis" 692:Aristarchus (crater) 672:by greek metal band 634:Mare Tranquillitatis 545:Late lunar volcanism 450:) (October 1, 2014). 408:Carpathian Mountains 61:improve this article 1070:2021Sci...374..887C 1019:10.1038/nature10289 1011:2011Natur.476...69J 912:2012NatGe...5..775N 871:"NASA – Copernicus" 733:. USGS Astrogeology 332:Ōceanus procellārum 237:Oceanus Procellarum 195: /  152: 151:Oceanus Procellarum 147:Feature on the moon 1231:"Selenochromatica" 668:In the 2004 album 663:In popular culture 625: 521:) and low calcium 495: 393:Sinus Viscositatis 383:to the north, and 145: 1716:Maria on the Moon 1628: 1627: 1229:Ferruggia, Aldo. 1191:lroc.sese.asu.edu 1064:(6569): 887–890. 1050:Joy, Katherine H. 900:Nature Geoscience 340: 234: 233: 137: 136: 129: 111: 16:(Redirected from 1728: 1693: 1692: 1691: 1681: 1680: 1679: 1669: 1668: 1667: 1657: 1656: 1645: 1644: 1643: 1636: 1262: 1255: 1248: 1239: 1234: 1216: 1213: 1201: 1200: 1198: 1197: 1183: 1177: 1176: 1174: 1173: 1167:www.lpi.usra.edu 1159: 1153: 1152: 1140: 1134: 1133: 1131: 1129: 1112: 1106: 1105: 1045: 1039: 1038: 994: 988: 987: 985: 984: 973: 967: 966: 941:(3–4): 153–188. 930: 924: 923: 920:10.1038/NGEO1614 894: 885: 884: 882: 881: 867: 861: 858: 852: 851: 849: 847: 829: 823: 822: 816: 808: 806: 805: 790: 784: 783: 777: 769: 767: 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Index

Ocean of Storms
Sea of Storms

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Imbrium
Serenitatis
Coordinates
18°24′N 57°24′W / 18.4°N 57.4°W / 18.4; -57.4
Diameter
Eponym
/ˈsənəsˌprɒsɛˈlɛərəm/
oh-SEE-ə-nəs PROSS-el-AIR-əm
Latin
lit.
lunar mare
near side of the
Moon
Oceanus
volcanic

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