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首页> 外文期刊>Astronomy and astrophysics >Surface composition and dynamical evolution of two retrograde objects in the outer solar system: 2008 YB3 and 2005 VD
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Surface composition and dynamical evolution of two retrograde objects in the outer solar system: 2008 YB3 and 2005 VD

机译:外太阳系中两个逆行物体的表面组成和动力学演化:2008 YB3和2005 VD

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摘要

Most of the objects in the trans-Neptunian belt (TNb) and related populations move in prograde orbits with low eccentricity and inclination. However, the list of icy minor bodies moving in orbits with an inclination above 40° has increased in recent years. The origin of these bodies, and in particular of those objects in retrograde orbits, is not well determined, and different scenarios are considered, depending on their inclination and perihelion. In this paper, we present new observational and dynamical data of two objects in retrograde orbits, 2008 YB3 and 2005 VD. We find that the surface of these extreme objects is depleted of ices and does not contain the “ultra-red” matter typical of some Centaurs. Despite small differences, these objects share common colors and spectral characteristics with the Trojans, comet nuclei, and the group of grey Centaurs. All of these populations are supposed to be covered by a mantle of dust responsible for their reddish-to-neutral color. To investigate if the surface properties and dynamical evolution of these bodies are related, we integrate their orbits for 108 years to the past. We find a remarkable difference in their dynamical evolutions: 2005 VD’s evolution is dominated by a Kozai resonance with planet Jupiter while that of 2008 YB3 is dominated by close encounters with planets Jupiter and Saturn. Our models suggest that the immediate site of provenance of 2005 VD is the in the Oort Cloud, whereas for 2008 YB3 it is in the trans-Neptunian region. Additionally, the study of their residence time shows that 2005 VD has spent a larger lapse of time moving in orbits in the region of the giant planets than 2008 YB3. Together with the small differences in color between these two objects, with 2005 VD being more neutral than 2008 YB3, this fact suggests that the surface of 2005 VD has suffered a higher degree of processing, which is probably related to cometary activity episodes.
机译:跨海王星带(TNb)和相关种群中的大多数物体都在低偏心率和倾斜度的前进轨道上运动。但是,近年来,在倾斜度超过40°的轨道上移动的冰冷小物体的清单有所增加。这些物体的起源,特别是逆行轨道上的那些物体的起源还不确定,并且根据它们的倾斜度和近日点,考虑了不同的情况。在本文中,我们介绍了逆行轨道上两个物体2008 YB3和2005 VD的新观测和动力学数据。我们发现这些极端物体的表面上已经结冰,并且不包含某些半人马座的“超红色”物质。尽管差异很小,但这些对象与特洛伊木马,彗核和灰色半人马族群具有相同的颜色和光谱特征。所有这些种群都应该被一层粉尘覆盖,这些粉尘导致它们的颜色从红到中性。为了研究这些物体的表面性质和动力学演化是否相关,我们将它们的轨道整合了108年。我们发现它们的动力演化存在显着差异:2005年VD的演化以与木星行星的Kozai共振为主,而2008年YB3的演化以与木星和土星的紧密接触为主导。我们的模型表明,2005 VD起源的直接站点是奥尔特云,而2008 YB3的起源站点是跨海王星地区。此外,对它们的停留时间的研究表明,与2008 YB3相比,2005 VD在巨型行星区域内的轨道移动所花费的时间更长。再加上这两个对象之间的颜色差异很小,2005 VD比2008 YB3更中性,这一事实表明2005 VD的表面受到了更高程度的加工,这很可能与彗星活动有关。

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