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  2. Fra Mauro formation - Wikipedia

    en.wikipedia.org/wiki/Fra_Mauro_formation

    Photograph taken on Apollo 14 showing a cluster of boulders near the rim of Cone crater. Note the layering on some of the larger boulders. Analysis of Apollo 14 samples suggests that there are five major geologic constituents present in the immediate landing area: regolith breccias, fragmental breccias, igneous lithologies, granulitic lithologies, and impact-melt lithologies.

  3. Apollo 14 - Wikipedia

    en.wikipedia.org/wiki/Apollo_14

    In Apollo 14's most famous event, Shepard hit two golf balls he had brought with him with a makeshift club. While Shepard and Mitchell were on the surface, Roosa remained in lunar orbit aboard the Command and Service Module, performing scientific experiments and photographing the Moon, including the landing site of the future Apollo 16 mission

  4. Cone (crater) - Wikipedia

    en.wikipedia.org/wiki/Cone_(crater)

    Cone crater is a small crater in the Fra Mauro highlands, north of Fra Mauro crater, on the Moon.The name of the crater was formally adopted by the IAU in 1973. [1]The Apollo 14 astronauts Alan Shepard and Edgar Mitchell landed the Lunar Module (LM) Antares southwest of Cone crater on February 5, 1971.

  5. Relive the dramatic Apollo 14 launch and moon landing, 50 ...

    www.aol.com/relive-dramatic-apollo-14-launch...

    On Jan. 31, 1971, NASA sent the Apollo 14 mission skyward. The eighth crewed mission in the Apollo program (and third one to reach the surface of the Moon) lifted off on a Sunday afternoon with ...

  6. Fillet (geology) - Wikipedia

    en.wikipedia.org/wiki/Fillet_(geology)

    Image taken by astronaut Al Shepard of the boulder named 'Filleted Rock' displaying a fine-grained deposit at its base, i.e., fillet. Image taken at Station C2 of the Apollo 14 landing site. Rock width is about 1.5 m. The fillet is characterized by an onlap contact with the adjacent rock and by a shallow or concave profile. Associated ...

  7. Geology of the Moon - Wikipedia

    en.wikipedia.org/wiki/Geology_of_the_Moon

    It is estimated that the far-side crust is on average thicker than the near side by about 15 km. [35] Seismology has constrained the thickness of the crust only near the Apollo 12 and Apollo 14 landing sites. Although the initial Apollo-era analyses suggested a crustal thickness of about 60 km at this site, recent reanalyses of this data ...

  8. Mare Imbrium - Wikipedia

    en.wikipedia.org/wiki/Mare_Imbrium

    The planned landing site for Chang'e 3 was Sinus Iridum. The actual landing took place on Mare Imbrium. Chang'e 3 landed on 14 December 2013 on Mare Imbrium, about 40 km south of the 6 km diameter Laplace F crater, [18] [19] at 44.1260°N 19.5014°W. [19] [20] [21] The lander deployed the Yutu rover 7 hours and 24 minutes later. [22]

  9. Apollo Lunar Surface Experiments Package - Wikipedia

    en.wikipedia.org/wiki/Apollo_Lunar_Surface...

    The Apollo Lunar Surface Experiments Package (ALSEP) comprised a set of scientific instruments placed by the astronauts at the landing site of each of the five Apollo missions to land on the Moon following Apollo 11 (Apollos 12, 14, 15, 16, and 17). Apollo 11 left a smaller package called the Early Apollo Scientific Experiments Package, or EASEP.