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King (crater)

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Article Genealogy
Parent: Wiener (crater) Hop 4
Expansion Funnel Raw 26 → Dedup 0 → NER 0 → Enqueued 0
1. Extracted26
2. After dedup0 (None)
3. After NER0 ()
4. Enqueued0 ()
King (crater)
CaptionOblique view from Apollo 17
Coordinates5.0, N, 120.5, E...
Diameter76 km
Depth3.6 km
Colong240
EponymArthur Scott King, Edward Skinner King

King (crater) is a prominent impact feature located on the far side of the Moon. It is a large, relatively young crater situated within the rugged southern highlands, lying to the north of the enormous South Pole–Aitken basin. The crater is notable for its complex, terraced walls, extensive ejecta blanket, and a distinctive system of bright rays, indicating its geological youth compared to the heavily cratered terrain that surrounds it.

Description

King is classified as a complex crater, exhibiting a well-defined, terraced inner wall and a relatively flat floor that lacks a central peak, a common feature in larger lunar impacts. The crater's rim is sharp and circular, rising significantly above the surrounding terrain, which is part of the densely cratered Lunar highlands. Its continuous ejecta blanket forms a bright, extensive ray system that overlies older features, including the neighboring crater Ibn Firnas. The interior floor appears smoother than the external landscape, likely due to impact melt pooling, and is marked by several smaller craterlets. The crater's morphology has been studied in detail through orbital imagery from missions like Lunar Orbiter and the Lunar Reconnaissance Orbiter.

Formation and age

Based on its crisp morphology and prominent ray system, King is interpreted as a Copernican-aged crater, meaning it formed less than about 1.1 billion years ago, during a period of relatively recent lunar geologic activity. The impact that created King excavated material from deep within the lunar crust, possibly from the upper mantle, as it is situated on the northern rim of the ancient South Pole–Aitken basin, the Moon's largest known impact structure. The event generated significant volumes of impact melt, which coated the floor and contributed to the smooth appearance. Its age makes it a key stratigraphic marker for dating other surface features in this region of the lunar far side.

Satellite craters

By convention, smaller craters associated with King are identified on lunar maps by a letter appended to its name. Significant satellites include **King A**, a sizable crater attached to the northeastern rim, and **King Y**, which lies to the southwest. These secondary craters, often formed by material ejected during the primary King impact, exhibit their own sharp features but are generally more degraded than the main crater. The distribution of these satellites helps map the ejecta field and understand the dynamics of the original impact event. Their study contributes to the broader geologic mapping of the area conducted by the United States Geological Survey (USGS) Astrogeology Science Center.

Exploration and observations

As it is on the far side, King has never been observed directly from Earth. Its detailed study began with photographs from the Soviet Luna 3 probe and was greatly advanced by the NASA Lunar Orbiter program in the 1960s. High-resolution images and topographic data have since been provided by more recent missions, including Clementine, Kaguya (SELENE), and the Lunar Reconnaissance Orbiter (LRO). These datasets have allowed for precise altimetry measurements, mineralogical mapping, and detailed analysis of its impact melt deposits. The crater was also imaged by the crew of Apollo 17 during their transit to the Moon.

Significance and research

King is a scientifically significant site for understanding young impact processes and the composition of the lunar crust and upper mantle. Its location on the rim of the South Pole–Aitken basin makes it a potential window into the deep lunar subsurface, with ejected material possibly containing samples of the Moon's lower crust or mantle. Scientists from institutions like the Planetary Science Institute and Brown University have analyzed its spectral properties, suggesting the presence of distinct mineralogies like olivine and pyroxene. Research on King contributes to broader questions in planetary science regarding impact chronology, melt sheet formation, and the geologic history of the lunar far side, with implications for future resource exploration and potential crewed missions to the region. Category:Impact craters on the Moon Category:Far side of the Moon