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Ocean of Storms

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Ocean of Storms
NameOcean of Storms
CaptionMosaic of the Ocean of Storms from the Lunar Reconnaissance Orbiter.
Coordinates18.4, N, 57.4, W...
Diameter2,592 km
EponymLatin for "Ocean of Storms"

Ocean of Storms. It is a vast lunar mare on the western edge of the Moon's near side, the largest of the lunar maria. Unlike a true ocean, it is an immense plain of solidified basalt formed by ancient volcanic eruptions. Its formation and geological history are central to understanding the Moon's thermal evolution and have been a prime target for numerous exploration missions, including the landmark Apollo 12 landing.

Overview

The Ocean of Storms is the most extensive of the lunar maria, stretching over 2,500 kilometers across. It is bordered by several other notable features, including the Mare Imbrium to the north, the Mare Humorum to the south, and the Mare Nubium to the southeast. Unlike circular maria contained within impact basins, its irregular shape suggests a different, more complex formation mechanism linked to the Moon's internal processes. Its relatively low albedo makes it a prominent dark feature visible from Earth, and it has been observed since the earliest telescopic studies by astronomers like Galileo Galilei.

Geological characteristics

The geology is dominated by flood basalts similar to terrestrial features like the Columbia River Basalt Group. These basaltic lavas are generally younger than the surrounding highlands, with ages estimated between 1 to 3 billion years. The region exhibits a variety of geological structures, including wrinkle ridges, such as the prominent Dorsa Barlow, and numerous volcanic domes. A key feature is the Procellarum KREEP Terrane, an area geochemically enriched in potassium, rare-earth elements, and phosphorus, which is believed to be linked to a giant impact event or prolonged volcanic activity. The Gargantuan Basin, a hypothesized ancient impact structure, may underlie much of the area.

Exploration and missions

It has been a primary target for lunar exploration. The first soft landing on the Moon was achieved here by the Soviet Luna 9 probe. NASA's Surveyor 1 and Surveyor 3 also landed within its bounds. The most famous mission was Apollo 12, which landed near the Surveyor 3 site, enabling the return of parts of that spacecraft for analysis. More recently, the Chinese Lunar Exploration Program successfully deployed the Chang'e 5 spacecraft, which collected and returned the youngest lunar samples to date from a region near Mons Rümker. Orbital missions like Clementine, Lunar Prospector, and the Lunar Reconnaissance Orbiter have extensively mapped its composition and topography.

Scientific significance

Samples returned by Apollo 12 and Chang'e 5 have been invaluable, providing precise ages for its volcanic units and insights into the Moon's late-stage magmatic activity. The presence of the Procellarum KREEP Terrane suggests a unique geochemical history involving the lunar mantle. Studies of its basalts help constrain models of the Moon's thermal history and the timing of volcanic cessation. Its structure is also critical to the study of planetary geology, offering comparisons to volcanic provinces on Mars, such as the Tharsis region, and informing theories about the formation of large igneous provinces on Earth.

The vast, dark plain has served as a evocative setting in science fiction. It features prominently in Arthur C. Clarke's novel A Fall of Moondust and is referenced in episodes of the television series Space: 1999. The Apollo 12 landing site is often highlighted in documentaries such as those produced for the BBC and National Geographic. It also appears in various video games, including the strategy game Delta-V: Rings of Saturn and simulations within the Kerbal Space Program community.

Category:Lunar maria Category:Regions on the Moon