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DOI | 10.1038/s41550-019-0974-x |
A compact multi-planet system around a bright nearby star from the Dispersed Matter Planet Project | |
Staab, D.1,2; Haswell, C. A.1; Barnes, J. R.1; Anglada-Escude, G.3; Fossati, L.4; Doherty, J. P. J.1; Cooper, J.1; Jenkins, J. S.5; Diaz, M. R.5; Soto, M. G.3,5 | |
通讯作者 | Haswell, C. A. |
来源期刊 | NATURE ASTRONOMY
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ISSN | 2397-3366 |
出版年 | 2020 |
卷号 | 4期号:4页码:399-407 |
英文摘要 | Star DMPP-1 hosts a compact, four-planet system comprising three irradiated super-Earth-mass planets and one Neptune-mass planet, discovered through radial velocity measurements and the star's anomalously low chromospheric emission. To put the Solar System's terrestrial planets in context, the detection and characterization of low-mass exoplanets is important but challenging. The Dispersed Matter Planet Project targets stars with anomalously low Ca ii H and K chromospheric emission, indicative of circumstellar absorbing gas. Here we report high-precision, high-cadence radial-velocity measurements of the F8V star DMPP-1 (HD 38677). These were motivated by depressed Ca ii H and K line cores indicative of short-period, ablating planets producing circumstellar gas. We find a compact planetary system with orbital periods of about 2.9-19 days, comprising three super-Earth-mass planets (about 3-10 M-circle plus) and one Neptune-mass planet (about 24 M-circle plus). The irradiated super-Earths may be remnant cores of giant planets after mass loss while crossing the Neptune desert. A priori inferences about the presence of short-period planets enabled the efficient discovery of the DMPP-1 planets. We anticipate informative follow-up characterization studies. |
类型 | Article |
语种 | 英语 |
国家 | England ; Austria ; Chile |
开放获取类型 | Green Submitted |
收录类别 | SCI-E |
WOS记录号 | WOS:000508042900002 |
WOS关键词 | EXTRASOLAR PLANET ; SEARCH |
WOS类目 | Astronomy & Astrophysics |
WOS研究方向 | Astronomy & Astrophysics |
EI主题词 | 2019-12-23 |
来源机构 | University of London |
资源类型 | 期刊论文 |
条目标识符 | http://119.78.100.177/qdio/handle/2XILL650/311914 |
作者单位 | 1.Open Univ, Sch Phys Sci, Walton Hall, Milton Keynes, Bucks, England; 2.Rutherford Appleton Lab, AVS, Oxford, England; 3.Queen Mary Univ London, Sch Phys & Astron, London, England; 4.Austrian Acad Sci, Space Res Inst, Graz, Austria; 5.Univ Chile, Dept Astron, Camino Observatorio, Santiago, Chile |
推荐引用方式 GB/T 7714 | Staab, D.,Haswell, C. A.,Barnes, J. R.,et al. A compact multi-planet system around a bright nearby star from the Dispersed Matter Planet Project[J]. University of London,2020,4(4):399-407. |
APA | Staab, D..,Haswell, C. A..,Barnes, J. R..,Anglada-Escude, G..,Fossati, L..,...&Soto, M. G..(2020).A compact multi-planet system around a bright nearby star from the Dispersed Matter Planet Project.NATURE ASTRONOMY,4(4),399-407. |
MLA | Staab, D.,et al."A compact multi-planet system around a bright nearby star from the Dispersed Matter Planet Project".NATURE ASTRONOMY 4.4(2020):399-407. |
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