Lunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction Pattern

The Lunar Laser Ranging (LLR) retroreflector arrays have been on the Moon for half a century. During that time, the laser range uncertainty has improved by a factor of 100. Consequently, the science results have also improved by orders of magnitude. New retroreflectors are scheduled to go to the Moo...

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Main Authors: James G. Williams, Luca Porcelli, Simone Dell’Agnello, Lorenza Mauro, Marco Muccino, Douglas G. Currie, Dennis Wellnitz, Chensheng Wu, Dale H. Boggs, Nathan H. Johnson
Format: Article
Language:English
Published: IOP Publishing 2023-01-01
Series:The Planetary Science Journal
Subjects:
Online Access:https://doi.org/10.3847/PSJ/acbeab
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author James G. Williams
Luca Porcelli
Simone Dell’Agnello
Lorenza Mauro
Marco Muccino
Douglas G. Currie
Dennis Wellnitz
Chensheng Wu
Dale H. Boggs
Nathan H. Johnson
author_facet James G. Williams
Luca Porcelli
Simone Dell’Agnello
Lorenza Mauro
Marco Muccino
Douglas G. Currie
Dennis Wellnitz
Chensheng Wu
Dale H. Boggs
Nathan H. Johnson
author_sort James G. Williams
collection DOAJ
description The Lunar Laser Ranging (LLR) retroreflector arrays have been on the Moon for half a century. During that time, the laser range uncertainty has improved by a factor of 100. Consequently, the science results have also improved by orders of magnitude. New retroreflectors are scheduled to go to the Moon on Commercial Lander Payload Services missions and the Lunar Geophysical Network mission. The new retroreflectors are single 10 cm corner cube retroreflectors that will not spread the laser pulse during reflection like the existing arrays do. Due to the orbital and Earth rotational speeds, there is a velocity aberration of 0.″8–1.″5 for existing stations. Larger corner cubes require attention to ensure that the spread of possible velocity aberration displacements is optimally contained within the diffraction pattern. The diffraction pattern can be changed by making one or more of the rear dihedral angles slightly different from 90°. Improvements in the equipment at the LLR stations and improvements in the data analysis software are also desirable. Future possibilities are described.
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spelling doaj.art-cd050a609b1b4b108fcb3e72372523be2024-02-03T04:13:52ZengIOP PublishingThe Planetary Science Journal2632-33382023-01-01458910.3847/PSJ/acbeabLunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction PatternJames G. Williams0https://orcid.org/0000-0002-8441-5937Luca Porcelli1https://orcid.org/0000-0002-2153-4242Simone Dell’Agnello2https://orcid.org/0000-0002-0691-8213Lorenza Mauro3Marco Muccino4https://orcid.org/0000-0002-2234-9225Douglas G. Currie5https://orcid.org/0000-0002-6177-9826Dennis Wellnitz6https://orcid.org/0000-0002-6607-8949Chensheng Wu7https://orcid.org/0000-0002-8414-4487Dale H. Boggs8https://orcid.org/0000-0002-1568-3428Nathan H. Johnson9Jet Propulsion Laboratory, California Institute of Technology , Pasadena, CA 91109-8099, USA ; James.G.Williams@jpl.nasa.govNational Institute for Nuclear Physics—Frascati National Labs (INFN—LNF) , Frascati (Rome), ItalyNational Institute for Nuclear Physics—Frascati National Labs (INFN—LNF) , Frascati (Rome), ItalyNational Institute for Nuclear Physics—Frascati National Labs (INFN—LNF) , Frascati (Rome), ItalyNational Institute for Nuclear Physics—Frascati National Labs (INFN—LNF) , Frascati (Rome), Italy; aeroTecno s.r.l. , Rome, ItalyUniversity of Maryland , College Park, MD 20742, USAUniversity of Maryland , College Park, MD 20742, USAUniversity of Maryland , College Park, MD 20742, USA; KBR, Inc. , Greenbelt, MD 20770, USAJet Propulsion Laboratory, California Institute of Technology , Pasadena, CA 91109-8099, USA ; James.G.Williams@jpl.nasa.govNational Institute for Nuclear Physics—Frascati National Labs (INFN—LNF) , Frascati (Rome), ItalyThe Lunar Laser Ranging (LLR) retroreflector arrays have been on the Moon for half a century. During that time, the laser range uncertainty has improved by a factor of 100. Consequently, the science results have also improved by orders of magnitude. New retroreflectors are scheduled to go to the Moon on Commercial Lander Payload Services missions and the Lunar Geophysical Network mission. The new retroreflectors are single 10 cm corner cube retroreflectors that will not spread the laser pulse during reflection like the existing arrays do. Due to the orbital and Earth rotational speeds, there is a velocity aberration of 0.″8–1.″5 for existing stations. Larger corner cubes require attention to ensure that the spread of possible velocity aberration displacements is optimally contained within the diffraction pattern. The diffraction pattern can be changed by making one or more of the rear dihedral angles slightly different from 90°. Improvements in the equipment at the LLR stations and improvements in the data analysis software are also desirable. Future possibilities are described.https://doi.org/10.3847/PSJ/acbeabSpace vehicle instrumentsThe MoonEarth-moon system
spellingShingle James G. Williams
Luca Porcelli
Simone Dell’Agnello
Lorenza Mauro
Marco Muccino
Douglas G. Currie
Dennis Wellnitz
Chensheng Wu
Dale H. Boggs
Nathan H. Johnson
Lunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction Pattern
The Planetary Science Journal
Space vehicle instruments
The Moon
Earth-moon system
title Lunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction Pattern
title_full Lunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction Pattern
title_fullStr Lunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction Pattern
title_full_unstemmed Lunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction Pattern
title_short Lunar Laser Ranging Retroreflectors: Velocity Aberration and Diffraction Pattern
title_sort lunar laser ranging retroreflectors velocity aberration and diffraction pattern
topic Space vehicle instruments
The Moon
Earth-moon system
url https://doi.org/10.3847/PSJ/acbeab
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