首页> 外文期刊>Icarus: International Journal of Solar System Studies >New astrometric positions of the Jovian irregular satellites Elara and Pasiphae in 2016-2018
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New astrometric positions of the Jovian irregular satellites Elara and Pasiphae in 2016-2018

机译:2016-2018在Jovian不规则卫星elara和pasiphae的新的星形姿势

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A total of 372 astrometric positions of Jovian irregular satellites Elara and Pasiphae were obtained during three successive oppositions in 2016, 2017, and 2018, by 1 m telescope at Yunnan Observatory. Based on Gaia DR2 catalogue, 196 new positions of Elara and 176 new positions of Pasiphae were collected. We compared our observations to the theoretical positions retrieved from IMCCE ephemeris online service with satellite ephemeris of Emelyanov model and planetary ephemeris DE431. For Elara, in each direction, the mean (O-C) is better than -0.004 arcsec and the dispersion is no more than 0.063 arcsec. For Pasiphae, in each direction, the mean (O-C) is better than -0.045 arcsec and the dispersion is no more than 0.082 arcsec. Our new observations have a smaller dispersion than previous observations. Moreover, we also compared two recent orbit models of each satellite as well as three different planetary ephemerides of Jupiter. These comparisons show that the differences among all the three planetary ephemerides are small.
机译:在2016年,2016年,2016年和2018年,在云南天文台1米望远镜,在三次连续的反对期间,在三次连续的反对期间获得了jovian不规则卫星elara和pasiphae的372个星系。基于Gaia Dr2目录,收集了196年的Elara和176个新立场的新职位。我们将观察结果与从Imiceanov Model和行星Ephemeris de431的卫星星历和行星Eplemeris de431的卫星星历中检索到的理论位置。对于Elara,在每个方向上,平均值(O-C)优于-0.004弧度,分散不超过0.063 arcsec。对于Pasiphae,在每个方向上,平均值(O-C)优于-0.045弧度,并且分散体不超过0.082 arcsec。我们的新观察比以前的观察结果较小。此外,我们还将每个卫星的最近轨道模型进行了比较了两个轨道模型以及三种不同行星的木星星际杂志。这些比较表明,所有三个行星间隙中的差异都很小。

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