Evolutionary History of the Large-Scale Scarp in Jules Verne Crater, Moon.

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Title: Evolutionary History of the Large-Scale Scarp in Jules Verne Crater, Moon.
Authors: Wu, Congzhe1,2 (AUTHOR), Liu, Jianzhong2,3 (AUTHOR) liujianzhong@mail.gyig.ac.cn, Michael, Gregory2,3 (AUTHOR), Hiesinger, Harald4 (AUTHOR), van der Bogert, Carolyn H.1,4 (AUTHOR), Iqbal, Wajiha2,4 (AUTHOR), Zhu, Kai2,3 (AUTHOR), Liu, Jingwen2,4 (AUTHOR)
Source: Remote Sensing. May2025, Vol. 17 Issue 9, p1582. 26p.
Subjects: Lunar craters, Age
Abstract: We conducted a detailed study using multi-source data to date the mare activity and lobate scarp formation within the Jules Verne crater on the Moon. In previous studies, the Jules Verne crater has been classified as a pre-Nectarian impact crater. Our analysis indicates that it has an absolute model age (AMA) of 4.21 − 0.034 + 0.032 Ga. After its formation, a magmatic intrusion event created floor fractures, followed by two basaltic eruption events—one at 3.4 Ga and another at 2.6 Ga. Subsequently, around 1.4 billion years ago, lunar seismic activity likely took place in this region, resetting the surface ages of the crater floor fractures and surrounding areas, as evidenced by the scarp. [ABSTRACT FROM AUTHOR]
Copyright of Remote Sensing is the property of MDPI and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract. (Copyright applies to all Abstracts.)
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  Data: Evolutionary History of the Large-Scale Scarp in Jules Verne Crater, Moon.
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  Data: <searchLink fieldCode="AR" term="%22Wu%2C+Congzhe%22">Wu, Congzhe</searchLink><relatesTo>1,2</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Liu%2C+Jianzhong%22">Liu, Jianzhong</searchLink><relatesTo>2,3</relatesTo> (AUTHOR)<i> liujianzhong@mail.gyig.ac.cn</i><br /><searchLink fieldCode="AR" term="%22Michael%2C+Gregory%22">Michael, Gregory</searchLink><relatesTo>2,3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Hiesinger%2C+Harald%22">Hiesinger, Harald</searchLink><relatesTo>4</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22van+der+Bogert%2C+Carolyn+H%2E%22">van der Bogert, Carolyn H.</searchLink><relatesTo>1,4</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Iqbal%2C+Wajiha%22">Iqbal, Wajiha</searchLink><relatesTo>2,4</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Zhu%2C+Kai%22">Zhu, Kai</searchLink><relatesTo>2,3</relatesTo> (AUTHOR)<br /><searchLink fieldCode="AR" term="%22Liu%2C+Jingwen%22">Liu, Jingwen</searchLink><relatesTo>2,4</relatesTo> (AUTHOR)
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  Data: <searchLink fieldCode="JN" term="%22Remote+Sensing%22">Remote Sensing</searchLink>. May2025, Vol. 17 Issue 9, p1582. 26p.
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  Data: <searchLink fieldCode="DE" term="%22Lunar+craters%22">Lunar craters</searchLink><br /><searchLink fieldCode="DE" term="%22Age%22">Age</searchLink>
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  Label: Abstract
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  Data: We conducted a detailed study using multi-source data to date the mare activity and lobate scarp formation within the Jules Verne crater on the Moon. In previous studies, the Jules Verne crater has been classified as a pre-Nectarian impact crater. Our analysis indicates that it has an absolute model age (AMA) of 4.21 − 0.034 + 0.032 Ga. After its formation, a magmatic intrusion event created floor fractures, followed by two basaltic eruption events—one at 3.4 Ga and another at 2.6 Ga. Subsequently, around 1.4 billion years ago, lunar seismic activity likely took place in this region, resetting the surface ages of the crater floor fractures and surrounding areas, as evidenced by the scarp. [ABSTRACT FROM AUTHOR]
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  Data: <i>Copyright of Remote Sensing is the property of MDPI and its content may not be copied or emailed to multiple sites without the copyright holder's express written permission. Additionally, content may not be used with any artificial intelligence tools or machine learning technologies. However, users may print, download, or email articles for individual use. This abstract may be abridged. No warranty is given about the accuracy of the copy. Users should refer to the original published version of the material for the full abstract.</i> (Copyright applies to all Abstracts.)
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        Value: 10.3390/rs17091582
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        Text: English
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              Text: May2025
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