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https://ir.lib.ncu.edu.tw/handle/987654321/102018
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| 題名: | THE OUTER SOLAR SYSTEM ORIGINS SURVEY. I. DESIGN and FIRST-QUARTER DISCOVERIES |
| 作者: | 葉永烜;Bannister, Michele T.;Kavelaars, J. J.;Petit, Jean-Marc;Gladman, Brett J.;Gwyn, Stephen D. J.;Chen, Ying-Tung;Volk, Kathryn;Alexandersen, Mike;Benecchi, Susan D.;Delsanti, Audrey;Fraser, Wesley C.;Granvik, Mikael;Grundy, Will M.;Guilbert-Lepoutre, Aurélie;Hestroffer, Daniel;Ip, Wing-Huen;Jakubik, Marian;Lynne Jones, R.;Kaib, Nathan;Kavelaars, Catherine F.;Lacerda, Pedro;Lawler, Samantha;Lehner, Matthew J.;Lin, Hsing Wen;Lister, Tim;Lykawka, Patryk Sofia;Monty, Stephanie;Marsset, Michael;Murray-Clay, Ruth;Noll, Keith S.;Parker, Alex;Pike, Rosemary E.;Rousselot, Philippe;Rusk, David;Schwamb, Megan E.;Shankman, Cory;Sicardy, Bruno;Vernazza, Pierre;Wang, Shiang-Yu |
| 貢獻者: | 理學院天文研究所 |
| 關鍵詞: | Astrophysics;Earth and Planetary Astrophysics;Kuiper Belt: general;Physics;surveys |
| 日期: | 2016-09-01 |
| 上傳時間: | 2026-04-21 14:56:59 (UTC+8) |
| 出版者: | IOP Publishing Ltd.;The American Astronomical Society |
| 摘要: | 摘要： ABSTRACT We report the discovery, tracking, and detection circumstances for 85 trans-Neptunian objects (TNOs) from the first 42 deg2 of the Outer Solar System Origins Survey. This ongoing r-band solar system survey uses the 0.9 deg2 field of view MegaPrime camera on the 3.6 m Canada-France-Hawaii Telescope. Our orbital elements for these TNOs are precise to a fractional semimajor axis uncertainty <0.1%. We achieve this precision in just two oppositions, as compared to the normal three to five oppositions, via a dense observing cadence and innovative astrometric technique. These discoveries are free of ephemeris bias, a first for large trans-Neptunian surveys. We also provide the necessary information to enable models of TNO orbital distributions to be tested against our TNO sample. We confirm the existence of a cold "kernel" of objects within the main cold classical Kuiper Belt and infer the existence of an extension of the "stirred" cold classical Kuiper Belt to at least several au beyond the 2:1 mean motion resonance with Neptune. We find that the population model of Petit et al. remains a plausible representation of the Kuiper Belt. The full survey, to be completed in 2017, will provide an exquisitely characterized sample of important resonant TNO populations, ideal for testing models of giant planet migration during the early history of the solar system.
其他題名： AJ
其他題名： Astron. J
出版者： The American Astronomical Society
出版日期： 2016-09-01
出處： The Astronomical journal, 2016-09, Vol.152 (3), p.70
資源來源： Institute of Physics Journals
版權： 2016. The American Astronomical Society. All rights reserved.
版權： licence_http://creativecommons.org/publicdomain/zero
識別號： ISSN: 0004-6256
識別號： ISSN: 1538-3881
識別號： EISSN: 1538-3881
識別號： DOI: 10.3847/0004-6256/152/3/70 |
| 顯示於類別: | [天文研究所] 期刊論文
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