Self-Secondaries Formed by Cold Spot Craters on the Moon
Self-secondaries are a population of background secondaries, and they have been observed on top of impact melt and ballistically emplaced ejecta deposits on various planetary bodies. Self-secondaries are formed by impacts of sub-vertically launched ejecta, but the launch mechanism is not confirmed....
Main Authors: | Yiren Chang, Zhiyong Xiao, Yang Liu, Jun Cui |
---|---|
Format: | Article |
Language: | English |
Published: |
MDPI AG
2021-03-01
|
Series: | Remote Sensing |
Subjects: | |
Online Access: | https://www.mdpi.com/2072-4292/13/6/1087 |
Similar Items
-
Depth-to-diameter Ratios of Fresh Craters on the Moon and Implications for Surface Age Estimates
by: Rachael H. Hoover, et al.
Published: (2024-01-01) -
Volcanoes and impact craters on the moon and mars/
by: 371072 Leonardi, Piero
Published: (1976) -
Moon morphology interpretations : based on lunar orbiter photography/
by: 219882 Schultz, Peter H.
Published: (1976) -
Surface Roughness at the Moon’s South Pole: The Influence of Condensed Volatiles on Surface Roughness at the Moon’s South Pole
by: Lizeth O. Magaña, et al.
Published: (2024-01-01) -
On the importance of self-secondaries
by: Zhiyong Xiao
Published: (2018-07-01)