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Discovery of a comet by its Lyman-α emission

机译:通过莱曼-α发射发现彗星

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Several searches for near-Earth objects have recently been initiated, as a result of increased awareness of the hazard of impacts on the Earth. These programs mainly search for asteroids, so amateur astronomers can still contribute to the discovery of comets, especially out of the orbital plane of the Solar System. An ideal way to search for comets would be to use a spaceborne instrument capable of imaging the whole sky on a daily basis in a systematic and repeatable way. Such an instrument already exists on the solar observatory SOHO; it operates at the Lyman-α wavelength of neutral hydrogen, which is the main component of the emission cloud of a comet. Here we report the discovery, using archival data from this satellite, of a hitherto unnoticed comet which reached a perihelion of 1.546 a.u. on 26 June 1997. We derive the water production rate of the comet as a function of time and find that it increases after perihelion, like that of comet Halley.
机译:由于人们越来越认识到撞击地球的危险,最近已开始对近地物体进行几次搜索。这些程序主要搜索小行星,因此业余天文学家仍然可以为发现彗星做出贡献,尤其是在太阳系轨道平面之外。搜寻彗星的理想方法是使用能够每天以系统且可重复的方式对整个天空进行成像的星载仪器。这样的仪器已经存在于太阳观测台SOHO中;它在中性氢的Lyman-α波长下工作,中性氢是彗星发射云的主要成分。在这里,我们报告使用该卫星的档案数据发现的一颗迄今未被注意到的彗星,它的近日点为1.546a.u。我们在1997年6月26日得出了彗星的产水率随时间的变化,发现它在近日点之后增加了,就像哈雷彗星一样。

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