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    Please use this identifier to cite or link to this item: https://ir.lib.ncu.edu.tw/handle/987654321/102003


    Title: DISCOVERY of A NEW RETROGRADE TRANS-NEPTUNIAN OBJECT: HINT of A COMMON ORBITAL PLANE for LOW SEMIMAJOR AXIS, HIGH-INCLINATION TNOs and CENTAURS
    Authors: 陳文屏;Chen (陳英同), Ying-Tung;Lin (林省文), Hsing Wen;Holman, Matthew J.;Payne, Matthew J.;Fraser, Wesley C.;Lacerda, Pedro;Ip (葉永烜), Wing-Huen;Chen (陳文屏), Wen-Ping;Kudritzki, Rolf-Peter;Jedicke, Robert;Wainscoat, Richard J.;Tonry, John L.;Magnier, Eugene A.;Waters, Christopher;Kaiser, Nick;Wang, Shiang-Yu;Lehner, Matthew
    Contributors: 理學院天文研究所
    Keywords: Aircraft detection;Clustering;Disks;Dwarf planets;Kuiper belt: general;Oort Cloud;Origins;Planes;surveys;Trans-Neptunian objects
    Date: 2016-08-20
    Issue Date: 2026-04-21 14:55:37 (UTC+8)
    Publisher: IOP Publishing Ltd.;The American Astronomical Society
    Abstract: 摘要: ABSTRACT Although the majority of Centaurs are thought to have originated in the scattered disk, with the high-inclination members coming from the Oort cloud, the origin of the high-inclination component of trans-Neptunian objects (TNOs) remains uncertain. We report the discovery of a retrograde TNO, which we nickname &quot;Niku,&quot; detected by the Pan-STARRS 1 Outer Solar System Survey. Our numerical integrations show that the orbital dynamics of Niku are very similar to that of 2008 KV42 (Drac), with a half-life of ∼500 Myr. Comparing similar high-inclination TNOs and Centaurs (q > 10 au, a < 100 au, and i > 60°), we find that these objects exhibit a surprising clustering of ascending node, and occupy a common orbital plane. This orbital configuration has high statistical significance: 3.8- . An unknown mechanism is required to explain the observed clustering. This discovery may provide a pathway to investigating a possible reservoir of high-inclination objects.
    其他題名: APJL
    其他題名: Astrophys. J. Lett
    出版者: The American Astronomical Society
    出版日期: 2016-08-20
    出處: Astrophysical journal. Letters, 2016-08, Vol.827 (2), p.L24--L24
    資源來源: Institute of Physics Journals
    版權: 2016. The American Astronomical Society. All rights reserved.
    識別號: ISSN: 2041-8205
    識別號: ISSN: 2041-8213
    識別號: EISSN: 2041-8213
    識別號: DOI: 10.3847/2041-8205/827/2/L24
    Appears in Collections:[Graduate Institute of Astronomy] journal & Dissertation

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