Lindbergh (crater)
Encyclopedia
Lindbergh is a small lunar
Moon
The Moon is Earth's only known natural satellite,There are a number of near-Earth asteroids including 3753 Cruithne that are co-orbital with Earth: their orbits bring them close to Earth for periods of time but then alter in the long term . These are quasi-satellites and not true moons. For more...

 crater
Impact crater
In the broadest sense, the term impact crater can be applied to any depression, natural or manmade, resulting from the high velocity impact of a projectile with a larger body...

 that is located in the western part of the Mare Fecunditatis
Mare Fecunditatis
Mare Fecunditatis is a lunar mare which is 840 km in diameter. The Fecuditatis basin formed in the Pre-Nectarian epoch, while the basin material surrounding the mare is of the...

. It lies to the west of the flooded crater Bilharz
Bilharz (crater)
Bilharz is a lunar impact crater that lies in the eastern part of the Mare Fecunditatis. It is the largest member of a close triple-crater formation with Atwood to the east and Naonobu to the northeast. To the southeast is the prominent crater Langrenus....

, and northeast of Ibn Battuta
Ibn Battuta (crater)
Ibn Battuta is a small lunar crater on the Mare Fecunditatis, a lunar mare in the eastern part of the Moon's near side. It lies to the southwest of the crater Lindbergh, and northeast of the prominent Goclenius....

. Lindbergh was previously designated Messier G before being given its name by the IAU
International Astronomical Union
The International Astronomical Union IAU is a collection of professional astronomers, at the Ph.D. level and beyond, active in professional research and education in astronomy...

. The unusual elongated crater Messier
Messier (crater)
Messier is a relatively young lunar impact crater located on the Mare Fecunditatis. The crater has a discernible oblong shape that is not caused by foreshortening. The longer dimension is oriented in an east–west direction....

 lies about 150 km to the northwest.

This is an isolated crater that is entirely surrounded by lunar mare
Lunar mare
The lunar maria are large, dark, basaltic plains on Earth's Moon, formed by ancient volcanic eruptions. They were dubbed maria, Latin for "seas", by early astronomers who mistook them for actual seas. They are less reflective than the "highlands" as a result of their iron-rich compositions, and...

. It is circular and bowl-shaped, with an interior floor that is about half the diameter of the crater. The inner walls slope gently down to the floor, and lacks notable features or impacts.
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