PREDICTED PERFORMANCE OF AN X-RAY NAVIGATION SYSTEM FOR FUTURE DEEP SPACE AND LUNAR MISSIONS

被引:0
|
作者
Getchius, Joel [1 ]
Long, Anne [2 ]
Farahmand, Mitra [2 ]
Winternitz, Luke [3 ]
Hassouneh, Munther A. [3 ]
Mitchell, Jason W. [3 ]
机构
[1] Omitron Inc, Beltsville, MD 20771 USA
[2] Ai Solut Inc, Lanham, MD 20706 USA
[3] NASA, Goddard Space Flight Ctr, Greenbelt, MD 20771 USA
来源
关键词
D O I
暂无
中图分类号
TP [自动化技术、计算机技术];
学科分类号
0812 ;
摘要
In November 2017, the NASA Goddard Space Flight Center Station Explorer for X-ray Timing and Navigation Technology experiment successfully demonstrated the feasibility of X-ray Pulsar Navigation (XNAV) as part of the Neutron Star Interior Composition Explorer mission, which is an X-ray Astrophysics Mission of Opportunity currently operating onboard the International Space Station. XNAV provides a GPS-like, absolute autonomous navigation and timing capability available anywhere in the Solar System and beyond. While the most significant benefits of XNAV are expected to come in support of very deep-space missions, the absolute autonomous navigation and timing capability also has utility for inner Solar System missions where increased autonomy or backup navigation and timing services are required, e.g., address loss of communication scenarios. The NASA commitment to develop a Gateway to support exploration of the Moon and eventually Mars, as well as current and future robotic missions such as James Webb Space Telescope and New Horizons, certainly will tax the existing ground based infrastructure in terms of availability. Therefore, an extended look at the feasibility and potential performance of XNAV for comparable missions is warranted. In this paper, we briefly review the XNAV concept and present case studies of its utility and performance for a Gateway orbit, Sun-Earth libration orbit, and a deep space transit trajectory.
引用
收藏
页码:601 / 619
页数:19
相关论文
共 50 条
  • [31] The role of the background in past and future X-ray missions
    Silvano Molendi
    [J]. Experimental Astronomy, 2017, 44 : 263 - 271
  • [32] Future X-ray Missions for High Resolution Spectroscopy
    Takaya Ohashi
    [J]. Space Science Reviews, 2010, 157 : 25 - 36
  • [33] X-ray Pulsar based Autonomous Navigation for Lunar Rovers
    Li, Jingjing
    Zhang, Yutu
    Shao, Sipei
    Hu, Huijun
    Ding, Zhengtao
    [J]. PROCEEDINGS OF 2017 IEEE INTERNATIONAL CONFERENCE ON UNMANNED SYSTEMS (ICUS), 2017, : 156 - 162
  • [34] Performance of high frame-rate X-ray CCDs for future strategic missions
    Bautz, M.
    Foster, R.
    Grant, C. E.
    LaMarr, B.
    Malonis, A.
    Miller, E.
    Prigozhin, G.
    Burke, B.
    Cooper, M.
    Donlon, K.
    Lambert, R.
    Warner, K.
    Young, D.
    Chattopadhyay, T.
    Herrmann, S.
    Morris, R. G.
    Leitz, C.
    Allen, S.
    [J]. SPACE TELESCOPES AND INSTRUMENTATION 2022: ULTRAVIOLET TO GAMMA RAY, 2022, 12181
  • [35] Predicted performance of the LCLS x-ray diagnostics
    Gluskin, E
    Ilinski, P
    Vinokurov, N
    [J]. PHYSICS OF, AND SCIENCE WITH, THE X-RAY FREE-ELECTRON LASER, 2001, 581 : 131 - 140
  • [36] X-RAY MAP OF DEEP SPACE
    POUNDS, K
    [J]. NEW SCIENTIST, 1978, 78 (1101) : 286 - 287
  • [37] A Facility for Soft Proton Irradiation of X-Ray Detectors and Instrument Testing for Future Space Missions
    Diebold, Sebastian
    Jochum, Josef
    Kendziorra, Eckhard
    Perinati, Emanuele
    Santangelo, Andrea
    Tenzer, Chris
    [J]. 2013 14TH EUROPEAN CONFERENCE ON RADIATION AND ITS EFFECTS ON COMPONENTS AND SYSTEMS (RADECS), 2013,
  • [38] Self-contained autonomous navigation system for deep space missions
    Guo, YP
    [J]. SPACEFLIGHT MECHANICS 1999, VOL 102, PTS I AND II, 1999, 102 : 1099 - 1113
  • [39] Observing the effects of strong gravity with future X-ray missions
    Reynolds, CS
    [J]. X-RAY ASTRONOMY: STELLAR ENDPOINTS, AGN, AND THE DIFFUSE X-RAY BACKGROUND, 2001, 599 : 346 - 354
  • [40] Instrumentation and Future Missions in the Upcoming Era of X-ray Polarimetry
    Fabiani, Sergio
    [J]. GALAXIES, 2018, 6 (02)