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Stellar Occultations by TNOs: the January 08, 2011 by (208996) 2003 AZ84 and the May 04, 2011 by (50000) Quaoar

机译:TNO的恒星掩星:(208996)2003 AZ84于2011年1月8日,(50000)Quaoar于2011年5月4日

摘要

Between February 2010 and May 2011, our group has observed five stellar occultations by Trans-Neptunian Objects (TNOs), giving the size and shape for some of the biggest TNO's: Varuna, Eris, 2003 AZ84, Makemake and Quaoar. Here we present two of them: the January 08 stellar occultation by 2003 AZ84, and the May 04 by Quaoar. For the event of 2003 AZ84 we obtained one positive and another negative occultation chords in Chile. We give a lower limit to the diameter of the TNO. The event of Quaoar was observed from 16 sites distributed in Uruguay, Argentina, Chile and Brazil. Five of them yielded positive detection of the occultation. A preliminary analysis shows that the body is probably elongated and significantly bigger than the size determined by Fraser & Brown 2010, with a diameter of 890km. Using the size determined by the occultation, we will discuss the implications for the body density and albedo determination. The upper limit of the atmosphere is also studied.
机译:在2010年2月至2011年5月之间,我们的小组观测到了5个由海王星天体(TNO)造成的恒星掩星,给出了一些最大的TNO的大小和形状:Varuna,Eris,2003 AZ84,Makemake和Quaoar。在这里,我们介绍其中的两个:2003年AZ84于1月8日进行的恒星掩星,以及Quaoar于5月4日进行的星际掩星。对于2003年的AZ84事件,我们在智利获得了一个正掩星和另一个负掩星。我们给TNO的直径下限。在分布于乌拉圭,阿根廷,智利和巴西的16个地点观测到Quaoar事件。其中五个产生了对掩星的阳性检测。初步分析显示,该车体可能细长,并且比弗雷泽与布朗(Fraser&Brown 2010)确定的直径(890公里)大得多。使用掩星确定的大小,我们将讨论对身体密度和反照率确定的影响。还研究了大气的上限。

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