Mare basalts embayed ejecta structures formed by the massive Imbrium impact in this sub-scene of LROC Narrow Angle Camera (NAC) observation M131501983RE (2.2 km higher above, 902 meters in the LROC Featured Image field of view [full image HERE], immediately above). Arrows denote the contact between younger mare basalts and older Imbrium ejecta, image [NASA/GSFC/Arizona State University].
Lillian Ostrach
LROC News System
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Preliminary Lunar Reconnaissance Orbiter (LRO) laser altimetry (LOLA) data showing Imbrium as seen from Earth, the most predominant, clearly identifiable feature on the near side seen with the naked eye from Earth. Imbrium is central to most of the Moon's mare phenomena and it's highest diversity of compounds. [NASA/GSFC].
Since the mare basalts are embaying this feature, the basalts postdate the formation of the Imbrium basin. Using remotely-sensed data to establish this kind of geologic relationship on the lunar surface helps to clarify the geologic history of the Moon, an important consideration for planning future lunar exploration.
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