Small Solar System Bodies as granular media

Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetary systems) can be better understood by analysing the constitution and physical properties of small bodies in...

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Published inThe Astronomy and astrophysics review Vol. 27; no. 1; pp. 1 - 64
Main Authors Hestroffer, D., Sánchez, P., Staron, L., Bagatin, A. Campo, Eggl, S., Losert, W., Murdoch, N., Opsomer, E., Radjai, F., Richardson, D. C., Salazar, M., Scheeres, D. J., Schwartz, S., Taberlet, N., Yano, H.
Format Journal Article Web Resource
LanguageEnglish
Published Berlin/Heidelberg Springer Berlin Heidelberg 01.12.2019
Springer Nature B.V
Springer Verlag
Springer
Subjects
Asteroid missions
Asteroids
Astronomy
Astrophysics
Astrophysics and Astroparticles
Astrophysics and Cosmology
Aérospatiale, astronomie & astrophysique
Celestial mechanics
Condensed matter physics
Constitution
Dwarf planets
Earth
Earth and Planetary Astrophysics
Elastic deformation
Evolution
Geologic depressions
Granular materials
granular matter
Life on Earth
Mechanical properties
Mechanics
Near-Earth Objects
Observations and Techniques
Organic chemistry
Physical properties
Physical, chemical, mathematical & earth Sciences
Physics
Physics and Astronomy
Physique, chimie, mathématiques & sciences de la terre
Planetary evolution
Planetary systems
Planetology
Planets
Plastic deformation
Porosity
Regolith
Review Article
Sciences of the Universe
self-gravitating bodies
Soil mechanics
Solar system
Space Exploration and Astronautics
Space missions
Space science, astronomy & astrophysics
Space Sciences (including Extraterrestrial Physics
Surface properties
Terrestrial planets
Gravitational aggregates
Granular media
Methods: numerical, laboratory, observational
Small bodies of the Solar System SSSB, minor planets, asteroids: general
Planetary formation
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Abstract Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetary systems) can be better understood by analysing the constitution and physical properties of small bodies in the Solar System. Currently, two space missions (Hayabusa2, OSIRIS-REx) have recently arrived at their respective targets and will bring a sample of the asteroids back to Earth. Other small body missions have also been selected by, or proposed to, space agencies. The threat posed to our planet by near-Earth objects (NEOs) is also considered at the international level, and this has prompted dedicated research on possible mitigation techniques. The DART mission, for example, will test the kinetic impact technique. Even ideas for industrial exploitation have risen during the last years. Lastly, the origin of water and life on Earth appears to be connected to asteroids. Hence, future space mission projects will undoubtedly target some asteroids or other SSSBs. In all these cases and research topics, specific knowledge of the structure and mechanical behaviour of the surface as well as the bulk of those celestial bodies is crucial. In contrast to large telluric planets and dwarf planets, a large proportion of such small bodies is believed to consist of gravitational aggregates (‘rubble piles’) with no—or low—internal cohesion, with varying macro-porosity and surface properties (from smooth regolith covered terrain, to very rough collection of boulders), and varying topography (craters, depressions, ridges). Bodies with such structure can sustain some plastic deformation without being disrupted in contrast to the classical visco-elastic models that are generally valid for planets, dwarf planets, and large satellites. These SSSBs are hence better described through granular mechanics theories, which have been a subject of intense theoretical, experimental, and numerical research over the last four decades. This being the case, it has been necessary to use the theoretical, numerical and experimental tools developed within soil mechanics, granular dynamics, celestial mechanics, chemistry, condensed matter physics, planetary and computer sciences, to name the main ones, in order to understand the data collected and analysed by observational astronomy (visible, thermal, and radio), and different space missions. In this paper, we present a review of the multi-disciplinary research carried out by these different scientific communities in an effort to study SSSBs.
AbstractList Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetary systems) can be better understood by analysing the constitution and physical properties of small bodies in the Solar System. Currently, two space missions (Hayabusa 2, OSIRIS-REx) are on their way to their respective targets and perform samples return; other missions have been selected or proposed to space agencies. The threat posed to our planet by Near- Earth Objects (NEOs) is also considered at the international level, and this has prompted dedicated research on possible mitigation techniques. Thus, the DART space mission will test the kinetic impact technique. Even ideas for industrial exploitation have risen during the last years, as future space mission projects will undoubtedly target some asteroids or other SSSBs. Lastly, the origin of water and life on Earth appears to be connected to asteroids.In all these cases and research topics, specific knowledge of the structure and mechanical behaviour of the surface as well as the bulk of those celestial bodies is crucial. In contrast to large telluric planets and dwarf planets, a large proportion of such small bodies is believed to consist of gravitational aggregates (‘rubble piles’) with no—or low—internal cohesion, with varying macro-porosity and surface properties (from smooth regolith covered terrain, to very rough collection of boulders), and varying topography (cratering, depressions, ridges). Bodies with such structure can sustain some plastic deformation without being disrupted in contrast to the classical visco-elastic models that are generally valid for planets, dwarf planets, and large satellites. These SSSBs are hence better approached through granular mechanics theories, which have been a subject of intense theoretical, experimental, and numerical research over the last four decades.This being the case, it has been necessary to use the theoretical, numerical and experimental tools developed within Soil Mechanics, Granular Dynamics, Celestial Mechanics, Chemistry, Condensed Matter Physics, Planetary and Computer Sciences, to name the main ones, in order to understand the data collected and analysed by observational astronomy (visible, thermal, and radio), and different space missions.In this paper, we present a review of the multi-disciplinary research carried out by these different scientific communities in an effort to study SSSBs.
Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetary systems) can be better understood by analysing the constitution and physical properties of small bodies in the Solar System. Currently, two space missions (Hayabusa2, OSIRIS-REx) have recently arrived at their respective targets and will bring a sample of the asteroids back to Earth. Other small body missions have also been selected by, or proposed to, space agencies. The threat posed to our planet by near-Earth objects (NEOs) is also considered at the international level, and this has prompted dedicated research on possible mitigation techniques. The DART mission, for example, will test the kinetic impact technique. Even ideas for industrial exploitation have risen during the last years. Lastly, the origin of water and life on Earth appears to be connected to asteroids. Hence, future space mission projects will undoubtedly target some asteroids or other SSSBs. In all these cases and research topics, specific knowledge of the structure and mechanical behaviour of the surface as well as the bulk of those celestial bodies is crucial. In contrast to large telluric planets and dwarf planets, a large proportion of such small bodies is believed to consist of gravitational aggregates (‘rubble piles’) with no—or low—internal cohesion, with varying macro-porosity and surface properties (from smooth regolith covered terrain, to very rough collection of boulders), and varying topography (craters, depressions, ridges). Bodies with such structure can sustain some plastic deformation without being disrupted in contrast to the classical visco-elastic models that are generally valid for planets, dwarf planets, and large satellites. These SSSBs are hence better described through granular mechanics theories, which have been a subject of intense theoretical, experimental, and numerical research over the last four decades. This being the case, it has been necessary to use the theoretical, numerical and experimental tools developed within soil mechanics, granular dynamics, celestial mechanics, chemistry, condensed matter physics, planetary and computer sciences, to name the main ones, in order to understand the data collected and analysed by observational astronomy (visible, thermal, and radio), and different space missions. In this paper, we present a review of the multi-disciplinary research carried out by these different scientific communities in an effort to study SSSBs.
Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scien- tific interest in many aspects. The origin, formation, and evolution of our Solar System (and other planetary systems) can be better understood by analysing the constitution and physical properties of small bodies in the Solar System. Currently, two space missions (Hayabusa2, OSIRIS-REx) have recently arrived at their respective targets and will bring a sample of the asteroids back to Earth. Other small body missions have also been selected by, or proposed to, space agencies. The threat posed to our planet by near-Earth objects (NEOs) is also considered at the international level, and this has prompted dedicated research on possible mitigation techniques. The DART mission, for example, will test the kinetic impact technique. Even ideas for industrial exploitation have risen during the last years. Lastly, the origin of water and life on Earth appears to be connected to asteroids. Hence, future space mission projects will undoubtedly target some asteroids or other SSSBs. In all these cases and research topics, specific knowledge of the structure and mechanical behaviour of the surface as well as the bulk of those celestial bodies is crucial. In contrast to large telluric plan- ets and dwarf planets, a large proportion of such small bodies is believed to consist of gravitational aggregates (‘rubble piles’) with no—or low—internal cohesion, with varying macro-porosity and surface properties (from smooth regolith covered terrain, to very rough collection of boulders), and varying topography (craters, depressions, ridges). Bodies with such structure can sustain some plastic deformation without being disrupted in contrast to the classical visco-elastic models that are generally valid for planets, dwarf planets, and large satellites. These SSSBs are hence better described through granular mechanics theories, which have been a subject of intense theoretical, experimental, and numerical research over the last four decades. This being the case, it has been necessary to use the theoretical, numerical and experimental tools developed within soil mechanics, granular dynamics, celestial mechanics, chemistry, condensed matter physics, planetary and computer sciences, to name the main ones, in order to understand the data collected and analysed by observational astronomy (visible, ther- mal, and radio), and different space missions. In this paper, we present a review of the multi-disciplinary research carried out by these different scientific communities in an effort to study SSSBs.
ArticleNumber 6
Author Schwartz, S.
Richardson, D. C.
Yano, H.
Eggl, S.
Opsomer, E.
Taberlet, N.
Hestroffer, D.
Scheeres, D. J.
Staron, L.
Murdoch, N.
Sánchez, P.
Losert, W.
Radjai, F.
Bagatin, A. Campo
Salazar, M.
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  fullname: Hestroffer, D.
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  organization: IMCCE, Paris Observatory, Université PSL, CNRS, Sorbonne Université, Univ. Lille
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  surname: Sánchez
  fullname: Sánchez, P.
  organization: CCAR, University of Colorado Boulder
– sequence: 3
  givenname: L.
  surname: Staron
  fullname: Staron, L.
  organization: Inst. Jean Le Rond d’Alembert, Sorbonne Université, CNRS
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  givenname: A. Campo
  surname: Bagatin
  fullname: Bagatin, A. Campo
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  givenname: S.
  surname: Eggl
  fullname: Eggl, S.
  organization: IMCCE, Paris Observatory, Université PSL, CNRS, Sorbonne Université, Univ. Lille, LSST/DiRAC Institute, Department of Astronomy, University of Washington
– sequence: 6
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  surname: Losert
  fullname: Losert, W.
  organization: Department of Physics, Institute for Physical Science and Technology, University of Maryland
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  surname: Murdoch
  fullname: Murdoch, N.
  organization: DEOS/SSPA, Institut Supérieur de l’Aéronautique et de l’Espace (ISAE-SUPAERO), Université de Toulouse
– sequence: 8
  givenname: E.
  surname: Opsomer
  fullname: Opsomer, E.
  organization: GRASP, Research Unit CESAM, University of Liège
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  organization: Labratoire Lagrange, Univ. Nice, CNRS, Observatoire de la Côte d’Azur, Lunar and Planetary Laboratory, University of Arizona
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Issue 1
Keywords Gravitational aggregates
Granular media
Methods: numerical, laboratory, observational
Small bodies of the Solar System SSSB, minor planets, asteroids: general
Planetary formation
Language English
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Asteroids and Self-Gravitating Bodies as Granular Systems
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Snippet Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scientific interest in many aspects. The origin, formation, and evolution of our...
Asteroids and other Small Solar System Bodies (SSSBs) are of high general and scien- tific interest in many aspects. The origin, formation, and evolution of...
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SubjectTerms Asteroid missions
Asteroids
Astronomy
Astrophysics
Astrophysics and Astroparticles
Astrophysics and Cosmology
Aérospatiale, astronomie & astrophysique
Celestial mechanics
Condensed matter physics
Constitution
Dwarf planets
Earth
Earth and Planetary Astrophysics
Elastic deformation
Evolution
Geologic depressions
Granular materials
granular matter
Life on Earth
Mechanical properties
Mechanics
Near-Earth Objects
Observations and Techniques
Organic chemistry
Physical properties
Physical, chemical, mathematical & earth Sciences
Physics
Physics and Astronomy
Physique, chimie, mathématiques & sciences de la terre
Planetary evolution
Planetary systems
Planetology
Planets
Plastic deformation
Porosity
Regolith
Review Article
Sciences of the Universe
self-gravitating bodies
Soil mechanics
Solar system
Space Exploration and Astronautics
Space missions
Space science, astronomy & astrophysics
Space Sciences (including Extraterrestrial Physics
Surface properties
Terrestrial planets
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Title Small Solar System Bodies as granular media
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