Observational Study of the Rotation Rates of Very Small Near-Earth Asteroids

该奖项是根据2009年美国复苏和再投资法案（公法111-5）资助的。这个项目的动机是我们对目前发现的最小的近地小行星（NEAs）的物理特性缺乏了解。对于自转周期来说尤其如此，它可以提供有关小行星内部成分、断裂程度和碰撞历史的信息。目前的数据表明，直径小于200米的NEAs旋转速度超过2.2小时，这是理论上推导出的无力椭球体的临界旋转极限，而较大的天体旋转速度较慢。这表明，这些快速旋转的小天体是固体的，因此很可能是曾经组成碎石堆母体的单个碎片，这些碎片被灾难性的撞击破坏了。然而，已知自转周期的小型小行星的样本量很小，需要更可靠的统计样本。马格达莱纳岭天文台最先进的2.4米望远镜将用于确定每年15-20个小型近地天体的自转周期（通过光曲线）和物质分类（通过分光光度法）。到三年项目结束时，有特点的小型国家环境评估的数量预计将增加一倍以上。如果正如pi的初步观测所表明的那样，存在很大比例的缓慢旋转的小天体，那么在低质量的一端，“碎石堆”（相对于整体或一致的天体）很可能是常见的。这样的结果对于评估和规划这些物体构成的威胁非常重要。该项目将在一所少数族裔服务机构开展，并为这些学生提供研究和培训经验（尽管这里不包括直接支持）。研究人员将把近地小行星观测和这项研究中涉及的概念作为K-12教育工作者的科学硕士教学计划的一部分，他们定期就这些主题进行公开演讲。

AST-0908868Eileen RyanThis award is funded under the American Recovery and Reinvestment Act of 2009 (Public Law 111-5).This project is motivated by our lack of knowledge of the physical properties of the very smallest Near-Earth Asteroids (NEAs) now being discovered. This is particularly true for rotation periods, which can provide information about an asteroid's internal composition, degree of fracture, and collisional history. Current data suggest that NEAs smaller than 200 meters in diameter rotate faster than 2.2 hours, which is the theoretically derived critical rotation limit for strengthless ellipsoids, while larger bodies rotate more slowly. This suggests that the small fast rotating objects are solid and so are likely to be individual fragments that once made up a rubble pile parent body that was disrupted by a catastrophic impact. However, the sample size of small asteroids with known rotation periods is small and a more robust statistical sample is needed. The state-of-the-art 2.4-meter telescope at the Magdalena Ridge Observatory will be used to determine rotation periods (through light curves) and material classifications (through spectrophotometry) for 15-20 small NEAs per year. By the end of the three year project, the number of characterized small NEAs is expected to have more than doubled.If, as suggested by preliminary observations by the PIs, a large percentage of slowly rotating small bodies exists, it may well be the case that "rubble piles" (versus monolithic or coherent bodies) are common at the low-mass end. Such a result is important in assessing and planning for the threat posed by these objects. The project will be carried out at a minority serving institution and provide research and training experiences for these students (though no direct support is included here). The researchers will include Near-Earth Asteroid observations and the concepts involved in this research as part of a Masters of Science Teaching program for K-12 educators, and they routinely give public talks on these topics.