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    Carrel is a small lunar crater on the Mare Tranquillitatis. It has a somewhat distorted appearance, having a slight protruding bulge in the northwest rim. The interior is somewhat irregular, with ridges and some slumped material. This crater lies across a ridge in the surface of the mare. It was named after the … See more

    • Oblique view of Carrel from Apollo 15 panoramic camera. This shows numerous bright avalanche deposits, and that the floor is a jumble of slump blocks.
    • Another view of the interior from Apollo 15 See more

     
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    What crater is Carrel on the Mare Tranquillitatis?Carrel is a small lunar crater on the Mare Tranquillitatis. It has a somewhat distorted appearance, having a slight protruding bulge in the northwest rim. The interior is somewhat irregular, with ridges and some slumped material. This crater lies across a ridge in the surface of the mare .
    Which craters have a small central rise and localized slumped material?We found two complex craters (Hargitai & Öhman, 2014; Melosh, 1989a; Melosh & Ivanov, 1999) in our survey that contain a small central rise (and hence are complex craters) and localized slumped material. Their geographic locations are labeled in Figure 8. The central uplifts are also visible in their topographic profiles.
    Which craters are labelled in Mare Tranquillitatis?Major craters and Apollo 11 landing site in Mare Tranquillitatis are labelled. Blue circles marks two basin model as per De Hon ( 2017 ). The area shows various structural and morphological features such as the presence of long rille, wrinkle ridges, domes, collapsed pit and faults (figure 9 ).
    Why is impact cratering important?Understanding impact cratering mechanics is critical for using craters to study the history of a planetary body. The Moon was the first well-imaged planetary body to possess an abundance of impact craters, and a variety of new high-resolution satellite data are reinvigorating lunar crater studies.
  6. WebCarrel crater (15.6 km in diameter) is located near the center of Mare Tranquillitatis. On the north wall of this crater, you can find several eye-catching flow features, starting from near the top of the wall, merged …

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  11. Journal of Geophysical Research: Planets - Wiley …

    WebMar 7, 2019 · The 15–20 km diameter range comprises simple craters (bowl-shaped depressions), transitional craters (craters in which material slumped down the wall and accumulated locally), and complex craters (in addition …

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