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Lichtenberg is an isolated lunar impact crater located in the western part of the Oceanus Procellarum. The nearest crater of note is Briggs to the south. Lichtenberg has a small system of rays, a characteristic of Copernican age craters. The rays extend to the north and west of the crater but not elsewhere. The remaining flanks of the surface about the crater exhibit the low albedo of the lunar mare, and the mare deposits have overlaid the existing rays on the east and south sides of the crater. These are thus among the youngest deposits of basaltic lava on the Moon, and are believed to be less than 1 billion years in age. However, the most recent lunar geologic map (2020) does not show the mare next to Lichtenberg as being Copernican in age - it is mapped as Upper .

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  • Lichtenberg (Mondkrater) (de)
  • Lichtenberg (cráter) (es)
  • Cratere Lichtenberg (it)
  • Lichtenberg (crater) (en)
  • Lichtenberg (inslagkrater) (nl)
  • Lichtenberg (cratera) (pt)
  • Лихтенберг (лунный кратер) (ru)
  • 利希滕贝格陨石坑 (zh)
rdfs:comment
  • Lichtenberg ist ein Einschlagkrater auf der nordwestlichen Mondvorderseite.Er liegt nördlich des Kraters Briggs in der Ebene des Oceanus Procellarum. Er zeigt ein kleines, in nördlicher und westlicher Richtung verlaufendes Strahlensystem auf. Der Kraterrand ist kaum erodiert mit konzentrischen Rutschungen im Inneren. Der Krater wurde 1935 von der IAU nach dem deutschen Physiker und Schriftsteller Georg Christoph Lichtenberg offiziell benannt. (de)
  • Lichtenberg is een inslagkrater in het noordwestelijk gedeelte van het gebied dat bekend is als Oceanus Procellarum op de naar de Aarde toegekeerde kant van de Maan. (nl)
  • Lichtenberg è un cratere lunare di 19,53 km situato nella parte nord-occidentale della faccia visibile della Luna. Il cratere è dedicato al fisico tedesco Georg Christoph Lichtenberg. (it)
  • Кратер Лихтенберг (лат. Lichtenberg) — небольшой молодой ударный кратер в западной части Океана Бурь на видимой стороне Луны. Название присвоено в честь выдающегося немецкого учёного и публициста Георга Кристофа Лихтенберга (1742—1799) и утверждено Международным астрономическим союзом в 1935 г. Образование кратера относится к коперниковскому периоду. (ru)
  • 利希滕贝格陨石坑(Lichtenberg)是月球正面位于风暴洋西部一座年轻的小撞击坑,形成于哥白尼纪,以德国著名学者和作家格奥尔格·克里斯托夫·利希滕贝格(Georg Christoph Lichtenberg,1742年-1799年)之名命名,1935年被国际天文联合会批准接受。 (zh)
  • Lichtenberg es un cráter de impacto lunar relativamente aislado, localizado en la parte occidental del Oceanus Procellarum. El cráter más cercano con nombre propio es Briggs, situado al sur. Este cráter presenta un pequeño sistema de marcas radiales, una característica propia de los impactos del Período Copernicano. Los rayos se extienden solamente hacia el norte y el oeste del cráter, y los flancos restantes de la superficie alrededor del cráter, recubiertos por la lava, exhiben el bajo albedo propio del mar lunar. En consecuencia, se encuentran entre los depósitos más recientes de lava basáltica de la Luna, y se piensa que cuentan con menos de mil millones de años de edad.​ (es)
  • Lichtenberg is an isolated lunar impact crater located in the western part of the Oceanus Procellarum. The nearest crater of note is Briggs to the south. Lichtenberg has a small system of rays, a characteristic of Copernican age craters. The rays extend to the north and west of the crater but not elsewhere. The remaining flanks of the surface about the crater exhibit the low albedo of the lunar mare, and the mare deposits have overlaid the existing rays on the east and south sides of the crater. These are thus among the youngest deposits of basaltic lava on the Moon, and are believed to be less than 1 billion years in age. However, the most recent lunar geologic map (2020) does not show the mare next to Lichtenberg as being Copernican in age - it is mapped as Upper . (en)
  • Lichtenberg é uma cratera de impacto lunar isolada localizada na parte ocidental do Oceanus Procellarum . A cratera mais próxima da nota é Briggs ao sul. Lichtenberg tem um pequeno sistema de raios , uma característica das crateras da era copernicana . Os raios se estendem para o norte e oeste da cratera, mas não para outros lugares. Os flancos remanescentes da superfície em torno da cratera exibem o baixo albedo da égua lunar , e os depósitos da égua têm coberto os raios existentes nos lados leste e sul da cratera. Eles estão, portanto, entre os depósitos mais jovens de lava basáltica na Lua, e acredita-se que tenham menos de 1 bilhão de anos de idade. O cientista lunar Paul Spudis defende uma missão de retorno de amostra não tripulada à jovem égua para obter uma data radiométrica absolut (pt)
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  • http://commons.wikimedia.org/wiki/Special:FilePath/Lichtenberg_crater_4170_h1.jpg
  • http://commons.wikimedia.org/wiki/Special:FilePath/Lichtenberg_crater_Fig13.7c.jpg
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