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The Birth Environment of the Solar System
Open accessAbstract
This review examines our current understanding of the possible birth environments of our Solar System. Because most stars form within groups and clusters, the question becomes one of determining the nature of the birth aggregate of the Sun. This discussion starts by reviewing Solar System properties that provide constraints on our environmental history. We then outline the range of star-forming environments that are available in the Galaxy and discuss how they affect star and planet formation. The nature of the solar birth cluster is constrained by many physical considerations, including radiation fields provided by the background environment, dynamical scattering interactions, and by the necessity of producing the short-lived radioactive nuclear species inferred from meteoritic measurements. Working scenarios for the solar birth aggregate can be constructed, as discussed herein, although significant uncertainties remain.
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“Importantly, this broadening is expected, given that the solar system almost certainly originated within a star cluster (see Adams 2010; Arakawa & Kokubo 2023), and the orbital distribution of TNOs would have been affected by cluster dynamics within the first ∼100 Myr of the solar system's evolution.”
From Generation of Low-inclination, Neptune-crossing Trans-Neptunian Objects by Planet Nine (2024) · cites this paper as Adams 2010
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“Various lines of evidence indicate the solar system did not originate in isolation, and instead formed within a cluster of 10 3 10 4 stars (Adams and Laughlin 2001; Portegies Zwart 2009; Adams 2010; Pfalzner et al. 2015).”
From The planet nine hypothesis (2019) · cites this paper as Adams 2010
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Wijnen, T. P. G., Pols, O. R., Pelupessy, F. I., & Zwart, S. P. (2017) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201731072 · Cited by 15
Creating retrogradely orbiting planets by prograde stellar fly-bys
Breslau, A., & Pfalzner, S. (2018) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201833729 · Cited by 15
Planets in open clusters detectable byKepler
Chatterjee, S., Ford, E. B., Geller, A. M., & Rasio, F. A. (2012) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2012.22057.x · Cited by 15
Forming different planetary systems
Zhou, J., Xie, J., Liu, H.-G., Zhang, H., & Sun, Y. (2012) · Research in Astronomy and Astrophysics · doi:10.1088/1674-4527/12/8/010 · Cited by 15
Inclination Excitation of Solar System Debris Disk Due to Stellar Flybys
Moore, N. W. H., Li, G., & Adams, F. C. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/abb08f · Cited by 16
Self-citationThe AMBRE project: searching for the closest solar siblings
de Laverny, P., Recio-Blanco, A., Sousa, S. G., Mena, E. D., Kordopatis, G., Ferreira, A. C. S., Santos, N. C., Hakobyan, A. A., & Tsantaki, M. (2018) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201834285/pdf · Cited by 14
Oberg, N., Kamp, I., Cazaux, S. M., Woitke, P., & Thi, W. ‐. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202244092 · Cited by 14
The evolution of circumstellar discs in the galactic centre: an application to the G-clouds
Owen, J. E., & Lin, D. N. C. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3506 · Cited by 16
Reiter, M., McLeod, A. F., Klaassen, P., Guzmán, A. E., Dale, J. E., Mottram, J. C., & Garay, G. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2752 · Cited by 14
Disc truncation in embedded star clusters: Dynamical encounters versus face-on accretion
Wijnen, T. P. G., Pols, O. R., Pelupessy, I., & Zwart, S. P. (2017) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201731072/pdf · Cited by 14
HDO Ice Detected toward an Isolated Low-mass Protostar with JWST
Slavicinska, K., Tychoniec, Ł., Navarro, M. G., van Dishoeck, E. F., Tobin, J. J., van Gelder, M. L., Chen, Y., Boogert, A. C. A., Drechsler, W. B., Beuther, H., et al. (2025) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/addb45 · Cited by 13
Searching for solar siblings in APOGEE and Gaia DR2 with N-body simulations
Webb, J. J., Price-Jones, N., Bovy, J., Zwart, S. P., Hunt, J. D., Mackereth, J. T., & Leung, H. W. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa788 · Cited by 13
Creating retrogradely orbiting planets by prograde stellar fly-bys
Breslau, A., & Pfalzner, S. (2019) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201833729/pdf · Cited by 13
On the Fate of Interstellar Objects Captured by Our Solar System
Napier, K. J., Adams, F. C., & Batygin, K. (2021) · The Planetary Science Journal · doi:10.3847/psj/ac29bb · Cited by 13
Self-citationChemistry in Externally FUV-irradiated Disks in the Outskirts of the Orion Nebula Cluster
Díaz-Berríos, J. K., Guzmán, V. V., Walsh, C. M., Öberg, K. I., Cleeves, L. I., de la Villarmois, E. A., & Carpenter, J. M. (2024) · The Astrophysical Journal · doi:10.3847/1538-4357/ad4603 · Cited by 12
Solar System Migration Points to a Renewed Concept: Galactic Habitable Orbits
Baba, J., Tsujimoto, T., & Saitoh, T. R. (2024) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ad9260 · Cited by 15
A solar C/O ratio in planet-forming gas at 1 au in a highly irradiated disk
Schroetter, I., Berné, O., Bron, É., Alarcón, F., Amiot, P., Bergin, E. A., Boersma, C., Cami, J., Coleman, G. A. L., Dartois, E., et al. (2025) · Nature Astronomy · doi:10.1038/s41550-025-02596-6 · Cited by 12
Stellar escapers from M67 can reach solar-like Galactic orbits
Jørgensen, T. G., & Church, R. P. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa185 · Cited by 12
On the mass segregation of cores and stars
Alcock, H. L., & Parker, R. J. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2646 · Cited by 12
Oxygen isotopes in HED meteorites and their constraints on parent asteroids
Zhang, C., Miao, B., & He, H. (2019) · Planetary and Space Science · doi:10.1016/j.pss.2019.02.007 · Cited by 12
Did a stellar fly-by shape the planetary system around Pr 0211 in the cluster M44?
Pfalzner, S., Bhandare, A., & Vincke, K. (2018) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201731375/pdf · Cited by 12
Changes in orientation and shape of protoplanetary discs moving through an ambient medium
Wijnen, T. P. G., Pelupessy, I., Pols, O. R., & Zwart, S. P. (2017) · Springer Link (Chiba Institute of Technology) · doi:10.1051/0004-6361/201730793/pdf · Cited by 12
Generation of Low-inclination, Neptune-crossing Trans-Neptunian Objects by Planet Nine
Batygin, K., Morbidelli, A., Brown, M. E., & Nesvorný, D. (2024) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ad3cd2 · Cited by 11
“Importantly, this broadening is expected, given that the solar system almost certainly originated within a star cluster (see Adams 2010; Arakawa & Kokubo 2023), and the orbital distribution of TNOs would have been affected by cluster dynamics within the first ∼ 100 Myr of the solar system’s…”
Background
Metadata
- Authors
- Adams, F. C.
- Affiliations
- University of Michigan (US)
- Corresponding author
- Adams, Fred C.
- Venue
- Annual Review of Astronomy and Astrophysics
- Publisher
- Annual Reviews
- Published
- 2010-08-01
- Volume
- 48
- Issue
- 1
- Pages
- 47-85
- ISSN
- 0066-4146 (ISSN-L)
- 1545-4282
- OpenAlex
- W2159354014
- Cited by
- 464
- References
- 136
- Citations by year
- 2026: 14 · 2025: 34 · 2024: 33 · 2023: 26 · 2022: 37 · 2021: 48 · 2020: 40 · 2019: 31 · 2018: 38 · 2017: 22 · 2016: 24 · 2015: 27 · 2014: 22 · 2013: 26 · 2012: 23
- FWCI
- 1.93
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Locations
- Annual Review of Astronomy and Astrophysics (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Astrophysics and Star Formation Studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Keywords
- star formation, planet formation, radiation field, dynamical scattering, short-lived radionuclides, meteorites, solar system formation
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