首页> 外文期刊>Revista Mexicana de Astronomia y Astrofisica >New orbits for comets C/1960 M1 (Humason), C/1980 E1 (Bowell), and musings on extrasolar comets
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New orbits for comets C/1960 M1 (Humason), C/1980 E1 (Bowell), and musings on extrasolar comets

机译:C / 1960 M1(Humason),C / 1980 E1(Bowell)和太阳系彗星的冥想的新轨道

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摘要

New orbits are calculated for Comets Humason (C/1960 M1) and Bowell (C/1980 E1). Humason's orbit is based on 34 observation made over 348 days and Bowell's on 203 observations made over nearly eight years. Both comets have hyperbolic orbits. Backwards integrations indicate that both comets had originally highly elliptical orbits which changed to hyperbolas by the injection of energy from the Solar System. Given that both of their perihelions are more than 3 AU from the Sun, the possibility of nongravitational forces is remote. For Comet Secchi (C/1853 E1), however, the orbit is hyperbolic at more than 100000 AU from the Sun and with no indication of nongravitational forces. If the orbit is a hyperbola at that distance, could the comet's origin not be from beyond the Oort cloud?.
机译:计算彗星Humason(C / 1960 M1)和Bowell(C / 1980 E1)的新轨道。 Humason的轨道基于在348天的时间内进行的34次观测,而Bowell的轨道基于将近8年的观测在203次观测。两种彗星都有双曲线轨道。向后积分表明,这两个彗星最初都具有高度椭圆形的轨道,这些轨道通过从太阳系注入能量而变为双曲线。鉴于它们的近日点都距离太阳3 AU以上,因此非引力的可能性很小。但是,对于塞基彗星(C / 1853 E1),该轨道是双曲的,离太阳超过100000 AU,并且没有非引力的迹象。如果轨道在该距离处是双曲线,那么彗星的起源难道不是来自奥尔特云之外吗?

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