A Tendency Toward Alignment in Single-star Warm-Jupiter Systems
文献类型:期刊论文
作者 | Rice, Malena1,3,4; Wang, Songhu2; Wang, Xian-Yu5,6; Stefansson, Gudmundur7; Isaacson, Howard8,9; Howard, Andrew W.10; Logsdon, Sarah E.11; Schweiker, Heidi11; Dai, Fei12; Brinkman, Casey13 |
刊名 | ASTRONOMICAL JOURNAL |
出版日期 | 2022-09-01 |
卷号 | 164期号:3页码:15 |
ISSN号 | 0004-6256 |
DOI | 10.3847/1538-3881/ac8153 |
英文摘要 | The distribution of spin-orbit angles for systems with wide-separation, tidally detached exoplanets offers a unique constraint on the prevalence of dynamically violent planetary evolution histories. Tidally detached planets provide a relatively unbiased view of the primordial stellar obliquity distribution, since they cannot tidally realign within the system lifetime. We present the third result from our Stellar Obliquities in Long-period Exoplanet Systems (SOLES) survey: a measurement of the Rossiter-McLaughlin effect across two transits of the tidally detached warm Jupiter TOI-1478 b with the WIYN/NEID and Keck/HIRES spectrographs, revealing a sky-projected spin-orbit angle lambda = 6.2(-5.5)(+5.9 degrees). degrees. Combining this new measurement with the full set of archival obliquity measurements, including two previous constraints from the SOLES survey, we demonstrate that, in single-star systems, tidally detached warm Jupiters are preferentially more aligned than closer-orbiting hot Jupiters. This finding has two key implications: (1) planets in single-star systems tend to form within aligned protoplanetary disks, and (2) warm Jupiters form more quiescently than hot Jupiters, which, in single-star systems, are likely perturbed into a misaligned state through planet-planet interactions in the post-disk-dispersal phase. We also find that lower-mass Saturns span a wide range of spin-orbit angles, suggesting a prevalence of planet-planet scattering and/or secular mechanisms in these systems. |
WOS关键词 | ALIGNED ORBIT ; HOT-JUPITER ; PLANET ; SPECTROMETER ; EXOPLANETS ; ROTATION ; DWARF ; NEID ; KELT ; KECK |
资助项目 | Heising-Simons Foundation 51 Pegasi b Fellowship ; National Science Foundation Graduate Research Fellowship Program[DGE-1752134] ; W. M. Keck Foundation ; Astronomical Big Data Joint Research Center ; National Aeronautics and Space Administration ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership |
WOS研究方向 | Astronomy & Astrophysics |
语种 | 英语 |
出版者 | IOP Publishing Ltd |
WOS记录号 | WOS:000842245500001 |
资助机构 | Heising-Simons Foundation 51 Pegasi b Fellowship ; Heising-Simons Foundation 51 Pegasi b Fellowship ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; W. M. Keck Foundation ; W. M. Keck Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership ; Heising-Simons Foundation 51 Pegasi b Fellowship ; Heising-Simons Foundation 51 Pegasi b Fellowship ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; W. M. Keck Foundation ; W. M. Keck Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership ; Heising-Simons Foundation 51 Pegasi b Fellowship ; Heising-Simons Foundation 51 Pegasi b Fellowship ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; W. M. Keck Foundation ; W. M. Keck Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership ; Heising-Simons Foundation 51 Pegasi b Fellowship ; Heising-Simons Foundation 51 Pegasi b Fellowship ; National Science Foundation Graduate Research Fellowship Program ; National Science Foundation Graduate Research Fellowship Program ; W. M. Keck Foundation ; W. M. Keck Foundation ; Astronomical Big Data Joint Research Center ; Astronomical Big Data Joint Research Center ; National Aeronautics and Space Administration ; National Aeronautics and Space Administration ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership ; NASA-NSF Exoplanet Observational Research (NN-EXPLORE) partnership |
源URL | [http://ir.bao.ac.cn/handle/114a11/87699] |
专题 | 中国科学院国家天文台 |
通讯作者 | Rice, Malena |
作者单位 | 1.Yale Univ, Dept Astron, New Haven, CT 06511 USA 2.Indiana Univ, Dept Astron, Bloomington, IN 47405 USA 3.MIT, Dept Phys, Cambridge, MA 02139 USA 4.MIT, Kavli Inst Astrophys & Space Res, 77 Massachusetts Ave, Cambridge, MA 02139 USA 5.Chinese Acad Sci, Natl Astron Observ, Beijing 10010, Peoples R China 6.Univ Chinese Acad Sci, Beijing 100049, Peoples R China 7.Princeton Univ, Dept Astrophys Sci, 4 Ivy Lane, Princeton, NJ 08540 USA 8.Univ Calif Berkeley, Dept Astron, Berkeley, CA 94720 USA 9.Univ Southern Queensland, Ctr Astrophys, Toowoomba, Qld, Australia 10.CALTECH, Dept Astron, Pasadena, CA 91125 USA |
推荐引用方式 GB/T 7714 | Rice, Malena,Wang, Songhu,Wang, Xian-Yu,et al. A Tendency Toward Alignment in Single-star Warm-Jupiter Systems[J]. ASTRONOMICAL JOURNAL,2022,164(3):15. |
APA | Rice, Malena.,Wang, Songhu.,Wang, Xian-Yu.,Stefansson, Gudmundur.,Isaacson, Howard.,...&Holcomb, Rae.(2022).A Tendency Toward Alignment in Single-star Warm-Jupiter Systems.ASTRONOMICAL JOURNAL,164(3),15. |
MLA | Rice, Malena,et al."A Tendency Toward Alignment in Single-star Warm-Jupiter Systems".ASTRONOMICAL JOURNAL 164.3(2022):15. |
入库方式: OAI收割
来源:国家天文台
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