Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations

The internal heat flow related to the Moon’s composition, interior structure, and evolution history is not well-constrained and understood on a global scale. Up to now, only two in situ heat flow experiments, Apollo 15 and 17 were deployed nearly 50 years ago. The measured high values of heat flow m...

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Published in:Frontiers in Astronomy and Space Sciences
Main Authors: Guangfei Wei, Xiongyao Li, Hong Gan, Yaolin Shi
Format: Article in Journal/Newspaper
Language:English
Published: Frontiers Media S.A. 2023
Subjects:
Online Access:https://doi.org/10.3389/fspas.2023.1179558
https://doaj.org/article/c4220e504568478aad19c57a72b2d29c
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spelling ftdoajarticles:oai:doaj.org/article:c4220e504568478aad19c57a72b2d29c 2023-06-11T04:16:47+02:00 Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations Guangfei Wei Xiongyao Li Hong Gan Yaolin Shi 2023-05-01T00:00:00Z https://doi.org/10.3389/fspas.2023.1179558 https://doaj.org/article/c4220e504568478aad19c57a72b2d29c EN eng Frontiers Media S.A. https://www.frontiersin.org/articles/10.3389/fspas.2023.1179558/full https://doaj.org/toc/2296-987X 2296-987X doi:10.3389/fspas.2023.1179558 https://doaj.org/article/c4220e504568478aad19c57a72b2d29c Frontiers in Astronomy and Space Sciences, Vol 10 (2023) Chang’E-2 microwave radiometer Diviner Moon pole heat flow Astronomy QB1-991 Geophysics. Cosmic physics QC801-809 article 2023 ftdoajarticles https://doi.org/10.3389/fspas.2023.1179558 2023-05-28T00:35:47Z The internal heat flow related to the Moon’s composition, interior structure, and evolution history is not well-constrained and understood on a global scale. Up to now, only two in situ heat flow experiments, Apollo 15 and 17 were deployed nearly 50 years ago. The measured high values of heat flow might be influenced by lateral heat at highland/mare boundaries and enhanced by heat production from radioactive elements enriched unit, and may also be disturbed by astronauts’ activities. In this study, we proposed a new method to retrieve heat flows at two permanently shadowed craters, Haworth and Shoemaker of the Moon’s south pole, from Chang’E-2 microwave radiometer data and Diviner observations. Our results show that the average heat flow is 4.9 ± 0.2 mW/m2. This provides a constraint for the bulk concentration of Thorium within the lunar south polar crust 656 ± 54 ppb, which helps us understand the Moon’s thermal evolution and differentiation. Article in Journal/Newspaper South pole Directory of Open Access Journals: DOAJ Articles South Pole Frontiers in Astronomy and Space Sciences 10
institution Open Polar
collection Directory of Open Access Journals: DOAJ Articles
op_collection_id ftdoajarticles
language English
topic Chang’E-2
microwave radiometer
Diviner
Moon
pole
heat flow
Astronomy
QB1-991
Geophysics. Cosmic physics
QC801-809
spellingShingle Chang’E-2
microwave radiometer
Diviner
Moon
pole
heat flow
Astronomy
QB1-991
Geophysics. Cosmic physics
QC801-809
Guangfei Wei
Xiongyao Li
Hong Gan
Yaolin Shi
Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations
topic_facet Chang’E-2
microwave radiometer
Diviner
Moon
pole
heat flow
Astronomy
QB1-991
Geophysics. Cosmic physics
QC801-809
description The internal heat flow related to the Moon’s composition, interior structure, and evolution history is not well-constrained and understood on a global scale. Up to now, only two in situ heat flow experiments, Apollo 15 and 17 were deployed nearly 50 years ago. The measured high values of heat flow might be influenced by lateral heat at highland/mare boundaries and enhanced by heat production from radioactive elements enriched unit, and may also be disturbed by astronauts’ activities. In this study, we proposed a new method to retrieve heat flows at two permanently shadowed craters, Haworth and Shoemaker of the Moon’s south pole, from Chang’E-2 microwave radiometer data and Diviner observations. Our results show that the average heat flow is 4.9 ± 0.2 mW/m2. This provides a constraint for the bulk concentration of Thorium within the lunar south polar crust 656 ± 54 ppb, which helps us understand the Moon’s thermal evolution and differentiation.
format Article in Journal/Newspaper
author Guangfei Wei
Xiongyao Li
Hong Gan
Yaolin Shi
author_facet Guangfei Wei
Xiongyao Li
Hong Gan
Yaolin Shi
author_sort Guangfei Wei
title Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations
title_short Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations
title_full Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations
title_fullStr Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations
title_full_unstemmed Retrieval of lunar polar heat flow from Chang’E-2 microwave radiometer and Diviner observations
title_sort retrieval of lunar polar heat flow from chang’e-2 microwave radiometer and diviner observations
publisher Frontiers Media S.A.
publishDate 2023
url https://doi.org/10.3389/fspas.2023.1179558
https://doaj.org/article/c4220e504568478aad19c57a72b2d29c
geographic South Pole
geographic_facet South Pole
genre South pole
genre_facet South pole
op_source Frontiers in Astronomy and Space Sciences, Vol 10 (2023)
op_relation https://www.frontiersin.org/articles/10.3389/fspas.2023.1179558/full
https://doaj.org/toc/2296-987X
2296-987X
doi:10.3389/fspas.2023.1179558
https://doaj.org/article/c4220e504568478aad19c57a72b2d29c
op_doi https://doi.org/10.3389/fspas.2023.1179558
container_title Frontiers in Astronomy and Space Sciences
container_volume 10
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