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首页> 外文期刊>The Astrophysical Journal. Letters >Discovery and Physical Characterization of a Large Scattered Disk Object at 92 au
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Discovery and Physical Characterization of a Large Scattered Disk Object at 92 au

机译:92 AU的大散射磁盘对象的发现和物理表征

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摘要

We report the observation and physical characterization of the possible dwarf planet 2014. UZ224 ("DeeDee"), a dynamically detached trans-Neptunian object discovered at 92 au. This object is currently the second-most distant known trans-Neptunian object with reported orbital elements, surpassed in distance only by the dwarf planet Eris. The object was discovered with an r-band magnitude of 23.0 in data collected by the Dark Energy Survey between 2014 and 2016. Its 1140 year orbit has (a, e, i)=(109 au, 0.65, 26 degrees.8). It will reach its perihelion distance of 38 au in the year 2142. Integrations of its orbit show it to be dynamically stable on Gyr timescales, with only weak interactions with Neptune. We have performed follow-up observations with ALMA, using 3 hr of on-source integration time to measure the object's thermal emission in the Rayleigh-Jeans tail. The signal is detected at 7 sigma significance, from which we determine a V-band albedo of 13.1(-2.4)(+3.3)(stat)sys percent and a diameter of 635(-61)(+57)(stat)(-39)(+32)(sys) km assuming a spherical body with uniform surface properties.
机译:我们报告了2014年可能矮星的观察和物理特征。UZ224(“DeeDee”),在92 AU发现的动态分离的跨境对象。该对象目前是具有报告的轨道元素的第二个最遥远的跨境对象,仅限距离矮小的行星eris的距离。在2014年至2016年间的黑暗能量调查收集的数据中发现了该目的的R带幅度为23.0。其1140年轨道(A,E,I)=(109 AU,0.65,26度.8)。它将在2142年度达到38澳元的近距离距离。其轨道的整合表明它在Gyr Timescalles上动态稳定,只有与海王星的弱互动。我们使用3小时的源集成时间进行了与ALMA进行后续观察,以测量瑞利牛仔裤尾部的物体的热排放。该信号以7 sigma的意义检测,从中测定13.1(-2.4)(+ 3.3)(统计)SYS百分比和635(-61)(+ 57)(统计)(统计)(统计)的V波段-39)(+ 32)(Sys)km假设具有均匀表面性质的球体。

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  • 作者单位

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Penn Dept Phys &

    Astron Philadelphia PA 19104 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Michigan Dept Astron Ann Arbor MI 48109 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Michigan Dept Astron Ann Arbor MI 48109 USA;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Univ Penn Dept Phys &

    Astron Philadelphia PA 19104 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Univ Michigan Dept Astron Ann Arbor MI 48109 USA;

    Natl Optic Astron Observ Cerro Tololo Interamer Observ La Serena Chile;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Natl Optic Astron Observ Cerro Tololo Interamer Observ La Serena Chile;

    UCL Dept Phys &

    Astron London WC1E 6BT England;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    LSST Tucson AZ 85721 USA;

    UCL Dept Phys &

    Astron London WC1E 6BT England;

    Inst Astrophys CNRS UMR 7095 F-75014 Paris France;

    UCL Dept Phys &

    Astron London WC1E 6BT England;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol Stanford CA 94305 USA;

    Lab Interinstituc e Astronomia LIneA BR-20921400 Rio De Janeiro RJ Brazil;

    Univ Illinois Dept Astron Urbana IL 61801 USA;

    Barcelona Inst Sci &

    Technol IFAE E-08193 Bellaterra Barcelona Spain;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol Stanford CA 94305 USA;

    Lab Interinstituc e Astronomia LIneA BR-20921400 Rio De Janeiro RJ Brazil;

    IIT Hyderabad Dept Phys Kandi 502285 Telangana India;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    CALTECH Jet Prop Lab Pasadena CA 91109 USA;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Univ Autonoma Madrid Inst Fis Teor UAM CSIC E-28049 Madrid Spain;

    IEEC CSIC Inst Ciencies Espai E-08193 Barcelona Spain;

    Univ Calif Berkeley Dept Astron Berkeley CA 94720 USA;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol Stanford CA 94305 USA;

    Lab Interinstituc e Astronomia LIneA BR-20921400 Rio De Janeiro RJ Brazil;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Ohio State Univ Ctr Cosmol &

    Astroparticle Phys Columbus OH 43210 USA;

    Natl Optic Astron Observ Cerro Tololo Interamer Observ La Serena Chile;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol Stanford CA 94305 USA;

    Australian Astron Observ N Ryde NSW 2113 Australia;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    UCL Dept Phys &

    Astron London WC1E 6BT England;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Lab Interinstituc e Astronomia LIneA BR-20921400 Rio De Janeiro RJ Brazil;

    Univ Penn Dept Phys &

    Astron Philadelphia PA 19104 USA;

    Texas A&

    M Univ George P &

    Cynthia Woods Mitchell Inst Fundamenta College Stn TX 77843 USA;

    Ohio State Univ Ctr Cosmol &

    Astroparticle Phys Columbus OH 43210 USA;

    Univ Illinois Dept Astron Urbana IL 61801 USA;

    Barcelona Inst Sci &

    Technol IFAE E-08193 Bellaterra Barcelona Spain;

    Univ Portsmouth Inst Cosmol &

    Gravitat Portsmouth PO1 3FX Hants England;

    CALTECH Jet Prop Lab Pasadena CA 91109 USA;

    Univ Sussex Dept Phys &

    Astron Brighton BN1 9QH E Sussex England;

    Stanford Univ Kavli Inst Particle Astrophys &

    Cosmol Stanford CA 94305 USA;

    CIEMAT Madrid Spain;

    CIEMAT Madrid Spain;

    Univ Southampton Sch Phys &

    Astron Southampton SO17 1BJ Hants England;

    Natl Optic Astron Observ Cerro Tololo Interamer Observ La Serena Chile;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Lab Interinstituc e Astronomia LIneA BR-20921400 Rio De Janeiro RJ Brazil;

    Oak Ridge Natl Lab Comp Sci &

    Math Div Oak Ridge TN 37831 USA;

    Natl Ctr Supercomp Applicat Urbana IL 61801 USA;

    Univ Michigan Dept Phys Ann Arbor MI 48109 USA;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

    Fermilab Natl Accelerator Lab Batavia IL 60510 USA;

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  • 原文格式 PDF
  • 正文语种 eng
  • 中图分类 天体力学(理论天文学);
  • 关键词

    infrared: planetary systems; Kuiper belt: general; methods: observational; techniques: photometric;

    机译:红外线:行星系统;Kuiper皮带:一般;方法:观察;技术:光度法;

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