The orbit of comet Tsuchinshan 1977q

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Abstract

Comet Tsuchinshan (1977q) was discovered at Purple Mountain Observatory on Nov. 3, 1977. The osculating orbital elements (referred to the barycenter of the sun and Mercury) given in table 1 are derived from 42 observations Nov. 3, 1977 to Jan. 10, 1978 at our observatory and abroad, taking into account the perturbations of all major planets. In all the observations the rms residual is 1.″78. Our observations are also published in table 2. With the elements thus obtained, the appropriate ephemerides in recent years have been calculated and listed in table 4. And then, in consideration of accurate perturbations, we compute the original and future orbits (referred to the center of mass of solar system) while the comet is about 60 A. U. from the sun. The results that both the original and future orbits are hyperbolicaare given in table 5 and may be compared with the osculating elements. Nevertheless, the two months observed interval for determining orbit is short. In order to obtain the more reliable conclusion, it is necessary to make some efforts for increasing the observed arc.

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冢山彗星1977q的轨道
1977年11月3日,紫金山天文台发现了冢山彗星(1977q)。表1中给出的密切轨道元素(指太阳和水星的质心)是根据1977年11月3日至1978年1月10日在我们天文台和国外进行的42次观测得出的,其中考虑了所有主要行星的扰动。在所有观测值中,残差均方根为1.″78。我们的观察结果也发表在表2中。根据所获得的元素,我们计算了近年来的星历表,并将其列在表4中。然后,考虑到精确的扰动,我们计算了彗星在大约60a时的原始和未来轨道(参照太阳系的质心)。美国远离太阳。表5给出了原轨道和未来轨道都是双曲线的结果,可以与密切元进行比较。然而,观测到的两个月确定轨道的间隔很短。为了得到更可靠的结论,有必要在增大观测弧度方面做一些努力。
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