Lunar Day Three

  • Tammy Plotner
Part of the Astronomer’s Pocket Field Guide book series (ASTROPOC)


Tonight we will return again to the northeast quadrant of the Moon for a closer look at Mare Crisium region (Fig. 4.1). The “Sea of Crises” is not only unique for its lack of connection with any other maria, but it is home to a gravitational anomaly called a mascon. This “mass concentration” might possibly consist of fragments of the asteroid or comet whose impact with the lunar surface created the basin buried beneath the lava flow. The mascon creates an area of high gravity and causes changes in the orbits of lunar probes. This excess gravity has even been known to cause low orbiting lunar satellites to either crash land or be flung out into space! Take a look at Mare Crisium in your telescope and trace the long frozen wave of lava along its west bank known as Dorsum Oppel. Did you catch the two small punctuations of crater Swift to the north and crater Pierce to its south? When you reach the central point of the western shoreline, look for Promontoriums Olivium and Lavinium. It is easy to catch the sharp, small crater Picard to the east, but did you spot the ruins of crater Yerkes between them? Or, even tinier Curtis east of Picard?


Lava Flow Lunar Surface Lunar Orbit Gravitational Anomaly Small Crater 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

Copyright information

© Springer Science+Business Media, LLC 2010

Authors and Affiliations

  1. 1.CaledoniaUSA

Personalised recommendations