Renoir is a crater on the planet Mercury. Its name, after the French painter Pierre-Auguste Renoir (1841–1919), was adopted by the International Astronomical Union in 1976. Renoir is a peak ring basin, one of 110 on Mercury, including Raditladi and Rachmaninoff. Though these basins are relatively young geologic features, Renoir is one of the oldest of its type. Because of its greater age, Renoir displays more of the effects of tectonics and later impact events than the other peak ring impact basins. It is thought to have formed at the end of the period with the highest meteor impact rates in Mercury's history. It is located in the Kuiper quadrangle. Renoir also has an area of high reflectance, classified as a plain, resulting from previous volcanic activity on the planet. Like Rachmaninoff
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| - Renoir (cràter) (ca)
- Cratere Renoir (it)
- Renoir (crater) (en)
- 雷諾瓦撞擊坑 (zh)
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| - Renoir è un cratere sulla superficie di Mercurio. (it)
- 雷諾瓦撞擊坑（英語：Renoir）是一個位於水星的撞擊坑，直徑219.88公里，座標橫跨15.71-20.87°S, 49.18-54.61°W。1976年國際天文學聯合會以法國畫家皮耶-奧古斯特·雷諾瓦命名該撞擊坑。 (zh)
- Renoir és un cràter d'impacte en el planeta Mercuri de 220 km de diàmetre. Porta el nom del pintor francès Pierre-Auguste Renoir (1841-1919), i el seu nom va ser aprovat per la Unió Astronòmica Internacional el 1976. (ca)
- Renoir is a crater on the planet Mercury. Its name, after the French painter Pierre-Auguste Renoir (1841–1919), was adopted by the International Astronomical Union in 1976. Renoir is a peak ring basin, one of 110 on Mercury, including Raditladi and Rachmaninoff. Though these basins are relatively young geologic features, Renoir is one of the oldest of its type. Because of its greater age, Renoir displays more of the effects of tectonics and later impact events than the other peak ring impact basins. It is thought to have formed at the end of the period with the highest meteor impact rates in Mercury's history. It is located in the Kuiper quadrangle. Renoir also has an area of high reflectance, classified as a plain, resulting from previous volcanic activity on the planet. Like Rachmaninoff (en)
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| - Renoir crater as seen by the MESSENGER spacecraft (en)
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| - Renoir és un cràter d'impacte en el planeta Mercuri de 220 km de diàmetre. Porta el nom del pintor francès Pierre-Auguste Renoir (1841-1919), i el seu nom va ser aprovat per la Unió Astronòmica Internacional el 1976. Renoir és una conca amb un anell de pics de Mercuri, una de diverses, que inclouen les conques de Raditladi i Rachmaninoff. Encara que aquestes conques són característiques geològiques relativament joves, Renoir és una de les més antigues del seu tipus. A causa de la seva antiguitat, Renoir mostra més efectes de tectònica i esdeveniments d'impacte posteriors que les altres conques d'impacte amb anell de pics. Es creu que es va formar al final del període amb les majors taxes d'impacte en la història de Mercuri. Situat al (H-6), es classifica com una «conca amb molts anells». Renoir també té una àrea d'alta , classificada com a plana, resultant de l'activitat volcànica anterior del planeta. Juntament amb Rachmaninoff, es tracta d'una de les dues conques de Mercuri amb una plana d'alta reflectància situada completament dins del cim central. Renoir té una estructura d'anells concèntrics, el que significa que també s'anomena «conca concèntrica». La seva vora interior és diferent, però, les conques similars solen tenir una vora externa més diferent que la vora interior. Les conques com Renoir són conegudes per tenir valls profundes al voltant d'elles. El radi i la massa inferiors de Mercuri en comparació amb altres cossos com Mart significa que les seves conques, incloent Renoir i Rodin, tenen un major diàmetre; En conseqüència, les conques de múltiples anells en cossos com la Lluna, incloses les conques com Hertzsprung i Mare Orientale, són encara més grans que les de Mercuri. (ca)
- Renoir is a crater on the planet Mercury. Its name, after the French painter Pierre-Auguste Renoir (1841–1919), was adopted by the International Astronomical Union in 1976. Renoir is a peak ring basin, one of 110 on Mercury, including Raditladi and Rachmaninoff. Though these basins are relatively young geologic features, Renoir is one of the oldest of its type. Because of its greater age, Renoir displays more of the effects of tectonics and later impact events than the other peak ring impact basins. It is thought to have formed at the end of the period with the highest meteor impact rates in Mercury's history. It is located in the Kuiper quadrangle. Renoir also has an area of high reflectance, classified as a plain, resulting from previous volcanic activity on the planet. Like Rachmaninoff, it is a basin with a high-reflectance plain located entirely within the central peak ring. Renoir has a concentric ring structure, meaning that it is also called a "concentric ring basin". Its interior rim is distinct, however, similar basins usually have a more distinct outer rim than inner rim. Basins like Renoir are known for having deep valleys in and around them. Mercury's lower radius and mass compared to other bodies like Mars mean that its basins - including Renoir and Rodin - have a greater diameter; consequently, the multi-ring basins on bodies like the Moon, including basins like Hertzsprung and Mare Orientale, are even larger than those on Mercury. (en)
- Renoir è un cratere sulla superficie di Mercurio. (it)
- 雷諾瓦撞擊坑（英語：Renoir）是一個位於水星的撞擊坑，直徑219.88公里，座標橫跨15.71-20.87°S, 49.18-54.61°W。1976年國際天文學聯合會以法國畫家皮耶-奧古斯特·雷諾瓦命名該撞擊坑。 (zh)
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