Brownlee Donald E, Horz Friedrich, Newburn Ray L, Zolensky Michael, Duxbury Thomas C, Sandford Scott, Sekanina Zdenek, Tsou Peter, Hanner Martha S, Clark Benton C, Green Simon F, Kissel Jochen
Department of Astronomy, University of Washington, Seattle, WA 98195, USA.
Science. 2004 Jun 18;304(5678):1764-9. doi: 10.1126/science.1097899.
Images taken by the Stardust mission during its flyby of 81P/Wild 2 show the comet to be a 5-kilometer oblate body covered with remarkable topographic features, including unusual circular features that appear to be impact craters. The presence of high-angle slopes shows that the surface is cohesive and self-supporting. The comet does not appear to be a rubble pile, and its rounded shape is not directly consistent with the comet being a fragment of a larger body. The surface is active and yet it retains ancient terrain. Wild 2 appears to be in the early stages of its degradation phase as a small volatile-rich body in the inner solar system.
“星尘”号探测器在飞越81P/怀尔德2号彗星时拍摄的图像显示,这颗彗星是一个直径5公里的扁球体,表面布满了显著的地形特征,包括看似撞击坑的异常圆形特征。高角度斜坡的存在表明其表面具有粘性且能自我支撑。这颗彗星似乎不是一堆碎石,其圆形形状与它是一个更大天体的碎片这一情况并不直接相符。其表面活跃,但仍保留着古老的地形。怀尔德2号似乎正处于其作为内太阳系中一个富含挥发物的小天体的退化阶段的早期。