Abstract
Unraveling the timing and duration of mare volcanism on the Moon is essential for understanding its thermal evolution. The end of mare volcanism is poorly constrained, because mare basalts are incompletely sampled. In this study, employing SELENE (Kaguya) high-resolution images, we performed new crater size-frequency measurements for 49 young mare units (
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Morota, T., Haruyama, J., Ohtake, M., Matsunaga, T., Honda, C., Yokota, Y., … Hiesinger, H. (2011). Timing and characteristics of the latest mare eruption on the Moon. Earth and Planetary Science Letters, 302(3–4), 255–266. https://doi.org/10.1016/j.epsl.2010.12.028
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