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A brief visit from a red and extremely elongated interstellar asteroid

机译:红色和极长的星际小行星短暂访问

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None of the approximately 750,000 known asteroids and comets in the Solar System is thought to have originated outside it, despite models of the formation of planetary systems suggesting that orbital migration of giant planets ejects a large fraction of the original planetesimals into interstellar space(1). The high predicted number density(2) of icy interstellar objects (2.4 x 10(-4) per cubic astronomical unit) suggests that some should have been detected, yet hitherto none has been seen. Many decades of asteroid and comet characterization have yielded formation models that explain the mass distribution, chemical abundances and planetary configuration of the Solar System today, but there has been no way of telling whether the Solar System is typical of planetary systems. Here we report observations and analysis of the object 1I/2017 U1 ('Oumuamua) that demonstrate its extrasolar trajectory, and that thus enable comparisons to be made between material from another planetary system and from our own. Our observations during the brief visit by the object to the inner Solar System reveal it to be asteroidal, with no hint of cometary activity despite an approach within 0.25 astronomical units of the Sun. Spectroscopic measurements show that the surface of the object is spectrally red, consistent with comets or organic-rich asteroids that reside within the Solar System. Light-curve observations indicate that the object has an extremely oblong shape, with a length about ten times its width, and a mean radius of about 102 metres assuming an albedo of 0.04. No known objects in the Solar System have such extreme dimensions. The presence of 'Oumuamua in the Solar System suggests that previous estimates of the number density of interstellar objects, based on the assumption that all such objects were cometary, were pessimistically low. Planned upgrades to contemporary asteroid survey instruments and improved data processing techniques are likely to result in the detection of more interstellar objects in the coming years.
机译:尽管有行星系统的形成模型表明巨行星的轨道迁移将大部分原始小行星射入星际空间,但太阳系中大约750,000个已知的小行星和彗星都没有一个起源于它之外。 。冰星际物体的高预测数密度(2)(每立方天文单位2.4 x 10(-4))表明应该已经发现了一些,但迄今为止还没有发现。几十年来,对小行星和彗星的描述已经产生了形成模型,这些模型可以解释当今太阳系的质量分布,化学丰度和行星结构,但是尚无法确定太阳系是否是行星系统的典型代表。在这里,我们报告对1I / 2017 U1('Oumuamua)物体的观测和分析,这些观测和分析证明了其太阳系轨迹,因此可以对来自另一个行星系统的材料与我们自己的材料进行比较。在物体短暂访问内部太阳系的过程中,我们的观察表明它是小行星,尽管接近太阳的0.25天文单位内没有彗星活动的迹象。光谱测量表明,该物体的表面是光谱红色的,与太阳系中的彗星或富含有机物的小行星一致。光曲线观察表明,该物体具有极长的椭圆形形状,其长度约为其宽度的十倍,假定反照率为0.04,则其平均半径约为102米。太阳系中没有已知的物体具有这样的极端尺寸。太阳系中“ Oumuamua”的存在表明,基于所有这些天体都是彗星的假设,以前对星际天体数量密度的估计是悲观的。对现代小行星测量仪器的计划升级和改进的数据处理技术可能会在未来几年中导致更多星际天体的探测。

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  • 来源
    《Nature》 |2017年第7685期|378-381|共4页
  • 作者单位

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    ESA SSA NEO Coordinat Ctr, Largo Galileo Galilei 1, I-00044 Frascati, Italy|Osserv Astron Roma, Via Frascati 33, I-00040 Monte Porzio Catone, Italy;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    European Southern Observ, Karl Schwarzschild Str 2, D-85748 Garching, Germany;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

    Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA;

  • 收录信息 美国《科学引文索引》(SCI);美国《工程索引》(EI);美国《生物学医学文摘》(MEDLINE);美国《化学文摘》(CA);
  • 原文格式 PDF
  • 正文语种 eng
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  • 入库时间 2022-08-18 02:51:58

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