Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system

The scale of the solar system is slowly changing, likely increasing as a result of solar mass loss, with additional change possible if there is a secular variation of the gravitational constant, G. The measurement of the change of scale could provide insight into the past and the future of the solar...

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Main Authors: Mazarico, Erwan, Neumann, Gregory A., Sun, Xiaoli, Torrence, Mark H., Mao, Dan-dan, Zuber, Maria, Genova, Antonio, Smith, David Edmund
Other Authors: Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Format: Article
Published: Elsevier BV 2018
Online Access:http://hdl.handle.net/1721.1/118808
https://orcid.org/0000-0003-2652-8017
https://orcid.org/0000-0001-5584-492X
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author Mazarico, Erwan
Neumann, Gregory A.
Sun, Xiaoli
Torrence, Mark H.
Mao, Dan-dan
Zuber, Maria
Genova, Antonio
Smith, David Edmund
author2 Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
author_facet Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences
Mazarico, Erwan
Neumann, Gregory A.
Sun, Xiaoli
Torrence, Mark H.
Mao, Dan-dan
Zuber, Maria
Genova, Antonio
Smith, David Edmund
author_sort Mazarico, Erwan
collection MIT
description The scale of the solar system is slowly changing, likely increasing as a result of solar mass loss, with additional change possible if there is a secular variation of the gravitational constant, G. The measurement of the change of scale could provide insight into the past and the future of the solar system, and in addition a better understanding of planetary motion and fundamental physics. Estimates for the expansion of the scale of the solar system are of order 1.5 cm year[superscript −1]AU[superscript −1], which over several years is an observable quantity with present-day laser ranging systems. This estimate suggests that laser measurements between planets could provide an accurate estimate of the solar system expansion rate. We examine distance measurements between three bodies in the inner solar system – Earth's Moon, Mars and Venus – and outline a mission concept for making the measurements. The concept involves placing spacecraft that carry laser ranging transponders in orbit around each body and measuring the distances between the three spacecraft over a period of several years. The analysis of these range measurements would allow the co-estimation of the spacecraft orbit, planetary ephemerides, other geophysical parameters related to the constitution and dynamics of the central bodies, and key geodetic parameters related to the solar system expansion, the Sun, and theoretical physics.
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spelling mit-1721.1/1188082024-05-15T02:22:28Z Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system Mazarico, Erwan Neumann, Gregory A. Sun, Xiaoli Torrence, Mark H. Mao, Dan-dan Zuber, Maria Genova, Antonio Smith, David Edmund Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences Smith, David E. Zuber, Maria Genova, Antonio The scale of the solar system is slowly changing, likely increasing as a result of solar mass loss, with additional change possible if there is a secular variation of the gravitational constant, G. The measurement of the change of scale could provide insight into the past and the future of the solar system, and in addition a better understanding of planetary motion and fundamental physics. Estimates for the expansion of the scale of the solar system are of order 1.5 cm year[superscript −1]AU[superscript −1], which over several years is an observable quantity with present-day laser ranging systems. This estimate suggests that laser measurements between planets could provide an accurate estimate of the solar system expansion rate. We examine distance measurements between three bodies in the inner solar system – Earth's Moon, Mars and Venus – and outline a mission concept for making the measurements. The concept involves placing spacecraft that carry laser ranging transponders in orbit around each body and measuring the distances between the three spacecraft over a period of several years. The analysis of these range measurements would allow the co-estimation of the spacecraft orbit, planetary ephemerides, other geophysical parameters related to the constitution and dynamics of the central bodies, and key geodetic parameters related to the solar system expansion, the Sun, and theoretical physics. 2018-10-30T18:21:10Z 2018-10-30T18:21:10Z 2018-02 2017-12 2018-10-05T12:58:00Z Article http://purl.org/eprint/type/JournalArticle 0032-0633 http://hdl.handle.net/1721.1/118808 Smith, David E., et al. “Trilogy, a Planetary Geodesy Mission Concept for Measuring the Expansion of the Solar System.” Planetary and Space Science, vol. 153, Apr. 2018, pp. 127–33. © 2018 The Authors https://orcid.org/0000-0003-2652-8017 https://orcid.org/0000-0001-5584-492X http://dx.doi.org/10.1016/J.PSS.2018.02.003 Planetary and Space Science Creative Commons Attribution-NonCommercial-NoDerivs License http://creativecommons.org/licenses/by-nc-nd/4.0/ application/pdf Elsevier BV Elsevier
spellingShingle Mazarico, Erwan
Neumann, Gregory A.
Sun, Xiaoli
Torrence, Mark H.
Mao, Dan-dan
Zuber, Maria
Genova, Antonio
Smith, David Edmund
Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system
title Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system
title_full Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system
title_fullStr Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system
title_full_unstemmed Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system
title_short Trilogy, a planetary geodesy mission concept for measuring the expansion of the solar system
title_sort trilogy a planetary geodesy mission concept for measuring the expansion of the solar system
url http://hdl.handle.net/1721.1/118808
https://orcid.org/0000-0003-2652-8017
https://orcid.org/0000-0001-5584-492X
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