论文标题

2021年8月22日,欧罗巴和甘卫姆德之间的准间隔日食的光度观察

The photometric observation of the quasi-simultaneous mutual eclipse and occultation between Europa and Ganymede on 22 August 2021

论文作者

So, Chu Wing, Luk, Godfrey Ho Ching, Chung, Giann On Ching, Leung, Po Kin, Hui, Kenneith Ho Keung, Cheung, Jack Lap Chung, Chan, Ka Wo, Yuen, Edwin Lok Hei, Lee, Lawrence Wai Kwan, Lau, Patrick Kai Ip, Cheung, Gloria Wing Shan, Chan, Prince Chun Lam, Pun, Jason Chun Shing

论文摘要

共同事件(MES)是行星天然卫星之间的日食和掩体。在大多数情况下,日食和​​掩体会单独发生。但是,同一卫星对将在特定的轨道构型下表现出Eclipse和仿真的准中。这种罕见的事件被称为准同时相互事件(QSME)。在2021年的Jovian卫星共同事件活动中,我们观察到Europa和Ganymede之间的QSME。本研究旨在详细描述和研究该事件。我们在香港太空博物馆Sai Kung Iobservatory的300毫米望远镜上观察了QSME。我们从光圈光度法中获得了欧罗巴和ganymede的合并通量。开发了一个几何模型来解释观察到的光曲线。我们的结果与理论预测(O-C)进行了比较。我们发现,我们简单的几何模型可以相当准确地解释QSME,而QSME光曲线是日食和掩星的光曲线的叠加。值得注意的是,观察到的通量滴在理论预测的2.6%之内。事件的大小中央时间O -CS的范围为-14.4至43.2 s。磁通量下降和计时的O-C都与采用更复杂模型的其他研究相媲美。鉴于事件稀有性,模型的简单性和准确性,我们鼓励对QSME的更多观察和分析,以改善太阳系胚层。

Mutual events (MEs) are eclipses and occultations among planetary natural satellites. Most of the time, eclipses and occultations occur separately. However, the same satellite pair will exhibit an eclipse and an occultation quasi-simultaneously under particular orbital configurations. This kind of rare event is termed as a quasi-simultaneous mutual event (QSME). During the 2021 campaign of mutual events of jovian satellites, we observed a QSME between Europa and Ganymede. The present study aims to describe and study the event in detail. We observed the QSME with a CCD camera attached to a 300-mm telescope at the Hong Kong Space Museum Sai Kung iObservatory. We obtained the combined flux of Europa and Ganymede from aperture photometry. A geometric model was developed to explain the light curve observed. Our results are compared with theoretical predictions (O-C). We found that our simple geometric model can explain the QSME fairly accurately, and the QSME light curve is a superposition of the light curves of an eclipse and an occultation. Notably, the observed flux drops are within 2.6% of the theoretical predictions. The size of the event central time O-Cs ranges from -14.4 to 43.2 s. Both O-Cs of flux drop and timing are comparable to other studies adopting more complicated models. Given the event rarity, model simplicity and accuracy, we encourage more observations and analysis on QSMEs to improve Solar System ephemerides.

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