傑克·希爾斯
關於澳大利亞山脈，請見「傑克山崗」。傑克·希爾斯（Jack G. Hills）是一名美國天文學家。他曾提出內奧爾特雲的概念，該區域因此也冠上他的姓，稱為「希爾斯雲」[1][2]。他大部分職業生涯都是在美國洛斯阿拉莫斯國家實驗室渡過的。從1998年開始，他成為該實驗室的研究員[3]。
| 傑克·希爾斯 | |
|---|---|
 傑克·希爾斯 |
參考資料
- ^ Stellar Dynamics: Jack Hills. Department of Physics and Astronomy. （原始內容存檔於15 December 2014）.
- ^ Michael Moltenbrey. Dawn of Small Worlds: Dwarf Planets, Asteroids, Comets. Springer. 24 October 2015: 97 [2019-01-13]. ISBN 978-3-319-23003-0. （原始內容存檔於2019-05-13）.
- ^ Laboratory Fellows from 1981 to the present （頁面存檔備份，存於網際網路檔案館） Los Alamos National Security J. G. Hills has made large contributions to Laboratory and international programs in astrophysics, interplanet science, and asteroid interdiction. He also is recognized worldwide as one of the major authorities in the field of stellar dynamics and has made seminal contributions to the quantitative understanding of interactions between binary and single stars in clusters.
拓展閱讀
- Jack G. Hills. Comet showers and the steady-state infall of comets from the Oort Cloud. Astronomical Journal. 1981, 86: 1730–1740. Bibcode:1981AJ.....86.1730H. doi:10.1086/113058.
- J. G. Hills. Dynamical constraints on the mass and perihelion distance of Nemesis and the stability of its orbit. Nature. 1984, 311 (5987): 636–638. Bibcode:1984Natur.311..636H. doi:10.1038/311636a0.
 | 這是一篇關於美國天文學家的小作品。您可以透過編輯或修訂擴充其內容。 |