Influence of Topography on the Site Selection of a Moon-Based Earth Observation Station

The Moon provides a long-term, stable, and unique location for Earth observation. Several space agencies, such as NASA, ESA, and CNSA, have conducted lunar explorations. To build a Moon-based observation station, site selection is the first step. The time coverage of Earth observation, e.g., the who...

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Autores principales: Guoqiang Chen, Huadong Guo, Yixing Ding, Haolu Shang, Mingyang Lv, Ke Zhang
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Lenguaje:EN
Publicado: MDPI AG 2021
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Acceso en línea:https://doaj.org/article/550a739b32a2411daf6f810976762a27
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spelling oai:doaj.org-article:550a739b32a2411daf6f810976762a272021-11-11T19:11:01ZInfluence of Topography on the Site Selection of a Moon-Based Earth Observation Station10.3390/s212171981424-8220https://doaj.org/article/550a739b32a2411daf6f810976762a272021-10-01T00:00:00Zhttps://www.mdpi.com/1424-8220/21/21/7198https://doaj.org/toc/1424-8220The Moon provides a long-term, stable, and unique location for Earth observation. Several space agencies, such as NASA, ESA, and CNSA, have conducted lunar explorations. To build a Moon-based observation station, site selection is the first step. The time coverage of Earth observation, e.g., the whole Earth disc observation or Earth-related plasmasphere and magnetosphere, the duration of sunlight coverage, and topography (i.e., slope) are the three major factors influencing site selection, especially in the Moon’s south pole region. In this study, we used the Chang’E digital elevation model (DEM) together with Earth, Moon, and Sun positions deduced from JPL ephemeris for site selection. Two craters, Faustini and Shoemaker, were chosen for the fuzzy evaluation of these three factors based on a multiple-input single-output (MISO) model during a 19-year period. The results show that the edge regions of craters and small hills, potholes, or uplifts inside craters are unsuitable for a Moon-based observation station. The south pole area, including these two craters, has relatively low time coverage of sunlight and some unevenly distributed, permanent shadow areas. This indicates a low thermal environment for radiation protection, whereas the relatively flat topography and the ability to cover a field of view several times the Earth’s radius enable observations of the plasmasphere and magnetosphere.Guoqiang ChenHuadong GuoYixing DingHaolu ShangMingyang LvKe ZhangMDPI AGarticleMoon-based observation stationEarth observationsun lightfuzzy evaluationChemical technologyTP1-1185ENSensors, Vol 21, Iss 7198, p 7198 (2021)
institution DOAJ
collection DOAJ
language EN
topic Moon-based observation station
Earth observation
sun light
fuzzy evaluation
Chemical technology
TP1-1185
spellingShingle Moon-based observation station
Earth observation
sun light
fuzzy evaluation
Chemical technology
TP1-1185
Guoqiang Chen
Huadong Guo
Yixing Ding
Haolu Shang
Mingyang Lv
Ke Zhang
Influence of Topography on the Site Selection of a Moon-Based Earth Observation Station
description The Moon provides a long-term, stable, and unique location for Earth observation. Several space agencies, such as NASA, ESA, and CNSA, have conducted lunar explorations. To build a Moon-based observation station, site selection is the first step. The time coverage of Earth observation, e.g., the whole Earth disc observation or Earth-related plasmasphere and magnetosphere, the duration of sunlight coverage, and topography (i.e., slope) are the three major factors influencing site selection, especially in the Moon’s south pole region. In this study, we used the Chang’E digital elevation model (DEM) together with Earth, Moon, and Sun positions deduced from JPL ephemeris for site selection. Two craters, Faustini and Shoemaker, were chosen for the fuzzy evaluation of these three factors based on a multiple-input single-output (MISO) model during a 19-year period. The results show that the edge regions of craters and small hills, potholes, or uplifts inside craters are unsuitable for a Moon-based observation station. The south pole area, including these two craters, has relatively low time coverage of sunlight and some unevenly distributed, permanent shadow areas. This indicates a low thermal environment for radiation protection, whereas the relatively flat topography and the ability to cover a field of view several times the Earth’s radius enable observations of the plasmasphere and magnetosphere.
format article
author Guoqiang Chen
Huadong Guo
Yixing Ding
Haolu Shang
Mingyang Lv
Ke Zhang
author_facet Guoqiang Chen
Huadong Guo
Yixing Ding
Haolu Shang
Mingyang Lv
Ke Zhang
author_sort Guoqiang Chen
title Influence of Topography on the Site Selection of a Moon-Based Earth Observation Station
title_short Influence of Topography on the Site Selection of a Moon-Based Earth Observation Station
title_full Influence of Topography on the Site Selection of a Moon-Based Earth Observation Station
title_fullStr Influence of Topography on the Site Selection of a Moon-Based Earth Observation Station
title_full_unstemmed Influence of Topography on the Site Selection of a Moon-Based Earth Observation Station
title_sort influence of topography on the site selection of a moon-based earth observation station
publisher MDPI AG
publishDate 2021
url https://doaj.org/article/550a739b32a2411daf6f810976762a27
work_keys_str_mv AT guoqiangchen influenceoftopographyonthesiteselectionofamoonbasedearthobservationstation
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AT haolushang influenceoftopographyonthesiteselectionofamoonbasedearthobservationstation
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