Complete Lunar Exploration Coverage Analysis

sponsorship acknowledged. NASA’s Vision for Space Exploration is to establish a permanent human presence on the Moon beginning no later than 2020. It is essential to provide an architecture that is ex-pandable and evolvable to meet the current and future communication requirements for Constellation’...

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Main Authors: Charles H. Lee, Kar-ming Cheung
Other Authors: The Pennsylvania State University CiteSeerX Archives
Format: Text
Language:English
Published: 2008
Subjects:
Online Access:http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.5524
http://tmo.jpl.nasa.gov/progress_report/42-175/175F.pdf
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spelling ftciteseerx:oai:CiteSeerX.psu:10.1.1.541.5524 2023-05-15T18:22:03+02:00 Complete Lunar Exploration Coverage Analysis Charles H. Lee Kar-ming Cheung The Pennsylvania State University CiteSeerX Archives 2008 application/pdf http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.5524 http://tmo.jpl.nasa.gov/progress_report/42-175/175F.pdf en eng http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.5524 http://tmo.jpl.nasa.gov/progress_report/42-175/175F.pdf Metadata may be used without restrictions as long as the oai identifier remains attached to it. http://tmo.jpl.nasa.gov/progress_report/42-175/175F.pdf text 2008 ftciteseerx 2016-01-08T11:05:27Z sponsorship acknowledged. NASA’s Vision for Space Exploration is to establish a permanent human presence on the Moon beginning no later than 2020. It is essential to provide an architecture that is ex-pandable and evolvable to meet the current and future communication requirements for Constellation’s International Space Station missions and lunar missions. This architecture includes the existing NASA ground-based and Earth-orbiting networks, as well as a possible network of lunar relay satellites. A key metric for decisions in selecting or expanding the communication infrastructure is its coverage capability. This article provides detailed cover-age analysis for various phases of a lunar exploration mission, including the launches of the Crew Exploration Vehicle (CEV) and the Lunar Surface Access Module/Earth Departure Stage (LSAM/EDS), their low-Earth-orbiting operations and docking; the trans-lunar inser-tion of the CEV/LSAM stack, its lunar orbiting insertion and low-lunar-orbiting operations; and the LSAM descent/ascent operations, as well as the Earth return phase. The human outpost of lunar exploration is assumed to be at the lunar south pole; the top 10 landing sites suggested by NASA’s Exploration Systems Architecture Study for lunar sortie missions are also considered. Surface-to-surface, Earth, and solar coverage at the lunar south pole using Goldstone Solar System Radar terrain data are also analyzed and discussed. I. Text South pole Unknown South Pole
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description sponsorship acknowledged. NASA’s Vision for Space Exploration is to establish a permanent human presence on the Moon beginning no later than 2020. It is essential to provide an architecture that is ex-pandable and evolvable to meet the current and future communication requirements for Constellation’s International Space Station missions and lunar missions. This architecture includes the existing NASA ground-based and Earth-orbiting networks, as well as a possible network of lunar relay satellites. A key metric for decisions in selecting or expanding the communication infrastructure is its coverage capability. This article provides detailed cover-age analysis for various phases of a lunar exploration mission, including the launches of the Crew Exploration Vehicle (CEV) and the Lunar Surface Access Module/Earth Departure Stage (LSAM/EDS), their low-Earth-orbiting operations and docking; the trans-lunar inser-tion of the CEV/LSAM stack, its lunar orbiting insertion and low-lunar-orbiting operations; and the LSAM descent/ascent operations, as well as the Earth return phase. The human outpost of lunar exploration is assumed to be at the lunar south pole; the top 10 landing sites suggested by NASA’s Exploration Systems Architecture Study for lunar sortie missions are also considered. Surface-to-surface, Earth, and solar coverage at the lunar south pole using Goldstone Solar System Radar terrain data are also analyzed and discussed. I.
author2 The Pennsylvania State University CiteSeerX Archives
format Text
author Charles H. Lee
Kar-ming Cheung
spellingShingle Charles H. Lee
Kar-ming Cheung
Complete Lunar Exploration Coverage Analysis
author_facet Charles H. Lee
Kar-ming Cheung
author_sort Charles H. Lee
title Complete Lunar Exploration Coverage Analysis
title_short Complete Lunar Exploration Coverage Analysis
title_full Complete Lunar Exploration Coverage Analysis
title_fullStr Complete Lunar Exploration Coverage Analysis
title_full_unstemmed Complete Lunar Exploration Coverage Analysis
title_sort complete lunar exploration coverage analysis
publishDate 2008
url http://citeseerx.ist.psu.edu/viewdoc/summary?doi=10.1.1.541.5524
http://tmo.jpl.nasa.gov/progress_report/42-175/175F.pdf
geographic South Pole
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http://tmo.jpl.nasa.gov/progress_report/42-175/175F.pdf
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