论文标题

X射线观测的虚拟望远镜

Virtual Telescope for X-Ray Observations

论文作者

Rankin, Kyle, Krizmanic, John, Shah, Neerav, Stochaj, Steven, Naseri, Asal

论文摘要

由NASA选择的X射线观测望远镜(VTXO)是由NASA进行的,是由NASAS Goddard太空飞行中心(GSFC)和新墨西哥州立大学(NMSU)开发的小型卫星任务。 VTXO将执行X射线观测值,其角度分辨率约为50 milliarcseconds,这比当前最先进的X射线望远镜所能达到的数量级要好。 VTXOS细角分辨率使测量紧凑型X射线源的环境更靠近中心发动机。该分辨率将通过使用分阶段的菲涅耳透镜(PFL)光学元件来实现,该光学元件可提供X射线带中接近衍射限制成像的光学元件。但是,PFL需要较长的焦距才能实现其成像性能,因为VTXO决定了望远镜光学器件和相机的分离为1 km。由于在空间中构建一个如此大的结构是不现实的,因此适用于VTXO的解决方案是将相机放置在两个单独的航天器上,并将其与必要的间距形成。这需要厘米水平的控制,以及两个航天器相对横向位置的亚毫米水平知识。本文将介绍VTXOS电流基线,并特别强调了飞行动态设计。

Selected by NASA for an Astrophysics Science SmallSat study, The Virtual Telescope for X-Ray Observations (VTXO) is a small satellite mission being developed by NASAs Goddard Space Flight Center (GSFC) and New Mexico State University (NMSU). VTXO will perform X-ray observations with an angular resolution around 50 milliarcseconds, an order of magnitude better than is achievable by current state of the art X-ray telescopes. VTXOs fine angular resolution enables measuring the environments closer to the central engines in compact X-ray sources. This resolution will be achieved by the use of Phased Fresnel Lenses (PFLs) optics which provide near diffraction-limited imaging in the X-ray band. However, PFLs require long focal lengths in order to realize their imaging performance, for VTXO this dictates that the telescopes optics and the camera will have a separation of 1 km. As it is not realistic to build a structure this large in space, the solution being adapted for VTXO is to place the camera, and the optics on two separate spacecraft and fly them in formation with the necessary spacing. This requires centimeter level control, and sub-millimeter level knowledge of the two spacecrafts relative transverse position. This paper will present VTXOs current baseline, with particular emphasis on the missions flight dynamics design.

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