May 23, 2022
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MARE NECTARIS /Â MASCON
Mare Nectaris es un mar situado en la cara visible de nuestro satélite al sur de Mare Tranquilitatis. Es totalmente circular, con un diámetro de 350 km. El trÃo de cráteres son Teophylus, Cyrillus y Catherina.
En diversos lugares de la Luna, especialmente en la cara visible, podemos encontrar un Mascon (mass concentration), una anomalÃa gravitacional que consiste en una zona de alta densidad situada bajo la superficie, la mayorÃa producidas por impactos meteorÃticos. En la imagen en falso color se puede apreciar la anomalÃa, gracias a la sonda GRAIL.Â
Maksutov Cassegrain 127. Cámara QHY 5II M.
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