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Mapping the Elemental Composition of Ceres and Vesta: Dawn's Gamma Ray and Neutron Detector

机译:绘制谷神星和维斯塔元素的成分图:黎明的伽马射线和中子探测器

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Dawn is a NASA discovery mission that will explore the main belt asteroids (1) Ceres and (4) Vesta. Ceres and Vesta are among the oldest bodies in the solar system and represent very different evolutionary paths. By studying these ancient, complementary asteroids, we will answer fundamental questions about the early solar system and planetary formation processes. The Dawn payload consists of a Framing Camera (FC), a visual and infrared mapping spectrometer (VIR), and a Gamma Ray and Neutron Detector (GRaND). The instruments provide data needed to investigate the structure, geology, mineralogy, and geochemistry of the asteroids. GRaND provides the data for the geochemistry investigation, including maps of most major elements and selected radioactive and trace elements. An updated description of the GRaND instrument is given along with the expected performance of GRaND at Vesta and Ceres. Approaches to combine data from FC, VIR and GRaND are discussed.
机译:黎明(Dawn)是NASA的一项发现任务,它将探索主要的小行星带(1)谷神星和(4)Vesta。谷神星和维斯塔星是太阳系中最古老的天体,它们代表了截然不同的进化路径。通过研究这些古老的互补小行星,我们将回答有关早期太阳系和行星形成过程的基本问题。黎明的有效载荷包括一个帧照相机(FC),一个视觉和红外映射光谱仪(VIR)以及一个伽玛射线和中子探测器(GRaND)。这些仪器提供了调查小行星的结构,地质,矿物学和地球化学所需的数据。 GRaND为地球化学调查提供数据,包括大多数主要元素的图谱以及选定的放射性和痕量元素。给出了GRaND仪器的最新描述以及GRaND在Vesta和Ceres的预期性能。讨论了组合来自FC,VIR和GRaND的数据的方法。

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