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Eclipses and Occultations of Galilean Satellites Observed at Yunnan Observatory in 2003 被引量:2
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作者 Qing-Yu Peng Benoit Noyelles 《Chinese Journal of Astronomy and Astrophysics》 SCIE CAS CSCD 2007年第2期317-324,共8页
We describe and analyze observations of mutual events of Galilean satellites made at the Yunnan Observatory in February 2003 from CCD imaging for the first time in China. Astrometric positions were deduced from these ... We describe and analyze observations of mutual events of Galilean satellites made at the Yunnan Observatory in February 2003 from CCD imaging for the first time in China. Astrometric positions were deduced from these photometric observations by modelling the relative motion and the photometry of the involved satellites during each event. 展开更多
关键词 planets and satellites individual Jupiter- astrometry - eclipse - occultation
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Mutual eclipses of J2 Europa by J1 Io observed at Yunnan Observatory in 2009 被引量:1
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作者 Xi-Liang Zhang Zhong Liu 《Research in Astronomy and Astrophysics》 SCIE CAS CSCD 2011年第10期1243-1248,共6页
Mutual events between natural satellites include mutual occultation and mutual eclipse. Mutual eclipse is another kind of mutual occultation as viewed from the center of the Sun instead of the Earth. Two mutual eclips... Mutual events between natural satellites include mutual occultation and mutual eclipse. Mutual eclipse is another kind of mutual occultation as viewed from the center of the Sun instead of the Earth. Two mutual eclipses of J2 Europa by J1 Io (2009 Aug. 28 and Sept. 12) were observed at Yunnan Observatory during the PHEMU09 international campaign. We will calculate the astrometric data of these Galilean satellites by analyzing and fitting the light curves we obtained. The limb-darkening was considered during modeling the light intensity of eclipsed satellites in the penumbra zone, by taking the Lommel-Seeliger scattering law into account. Several dynamical quantifies, such as the relative coordinates of the eclipsing satellite from the eclipsed one △α cos δ and △δ, impact parameter and mid-time corresponding to the impact parameter and the deviations O - C of observed △α cos d and △δ relative to ephemerides, were obtained for each event respectively. 展开更多
关键词 eclipses -- kinematics and dynamics-methods -- planets and satellites individual: Galilean satellites
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