监测预警

基于月基望远镜的近地小行星观测

  • 祝寒友 ,
  • 胡震宇 ,
  • 申智春
展开
  • 上海宇航系统工程研究所,上海 201109
祝寒友(1996—),工程师,主要研究方向为小行星监测预警、在轨处置与资源利用。通信地址:上海市元江路3888号(201109) 电子邮箱:zhuhanyou0122@163.com

网络出版日期: 2023-12-11

Near-Earth Asteroid Observations Based on Lunar Telescopes

  • ZHU Han-you ,
  • HU Zhen-yu ,
  • SHEN Zhi-chun
Expand
  • Aerospace System Engineering Shanghai,Shanghai 201109,China

Online published: 2023-12-11

摘要

近地小行星监测预警是行星防御的重要一环,但是现有的近地小行星观测能力无法实现对大部分百米量级近地小行星的观测,距离行星防御对监测预警的需求仍有较大缺口。针对近地小行星监测预警体系不完善的问题,本文通过分析月基望远镜的选址和口径需求,阐明月基望远镜观测近地小行星的可能性,提出利用月基望远镜进行近地小行星观测的方法能对现有的地基和天基近地小行星监测预警体系进行补充,对近地小行星的定轨能力有较大提升,具有重要意义。

本文引用格式

祝寒友 , 胡震宇 , 申智春 . 基于月基望远镜的近地小行星观测[J]. 空间科学与试验学报, 2021 , 21(4) : 22 -29 . DOI: 10.19963/j.cnki.2096-4099.2021.04.003

Abstract

The monitoring and warning of NEAs is an important part of planetary defense,but the existing NEA observation capabilities cannot observe most NEAs with a diameter less than100m.There is still a large gap between the observation capabilities and the demand for monitoring and warning from planetary defense.In view of the imperfect monitoring and warning system for NEAs,this paper analyzes the location and aperture requirements of lunar-based telescopes to clarify the possibility of observing NEAs by lunar-based telescopes,and proposes the use of lunar-based telescopes for NEA observations.This method can supplement the existing ground-based and space-based NEA monitoring and warning systems,and greatly improve the ability to determine the initial orbit of newly discovered asteroids,which is of great significance.

参考文献

[1] 张飞.小行星防御中的撞击研究[D].南京:南京大学,2019.
[2] 龚自正,李明,陈川,等.小行星监测预警、安全防御和资源利用的前沿科学问题及关键技术[J].科学通报,2020,65:346-372.
[3] 常锐.小行星的巡天观测[J].国际太空,2017,07:34-37.
[4] Larson S,Brownlee J,Hergenrother C,et al.The Catalina sky survey for NEOs[J].Bull Am Astron Soc,1998,30:1037.
[5] Stokes G H,Evans J B,Viggh H E M,et al.Lincoln Near-Earth asteroid program(LINEAR)[J].Icarus,2000,148:21-28.
[6] Jewitt D.Project Pan-STARRS and the outer solar system[J].Earth Moon Planets,2003,92:465-476.
[7] Sebring T A,Dunham E,Millis R L.The Discovery channel telescope:a wide-field telescope in Northern Arizona[C].Ground-Based Telescopes.Glasgow,UK:SPIE,2004.
[8] Abell P A,et al.LSST Science Book[M].Version 2.0.LSST Corporation,2009.
[9] Johnson L.International Asteroid Warning Network(IAWN)status report to STSC 2017[R/OL].https://www.cosmos.esa.int/documents/336356/1283810/IAWN_status_report_2017_Johnson.pdf.2019-02-03.
[10] 李婷,杨建峰,阮萍,等.月基光学天文望远镜(LOT)的杂散光分析[J].光子学报,2007,36:136-141.
[11] 张吉栋.基于LOLA数据的月球光照模型及应用研究[D].长春:吉林大学,2017.
[12] Meng X M,Han X H,Wei J Y,et al.NUV Star Catalog from the Lunar-based Ultraviolet Telescope Survey:First Release[J].Research in Astronomy and Astrophysics,2016,16(11):168.
[13] 彭华峰,陈鲸,张彬.天基光电望远镜极限星等探测能力研究[J].光电工程,2007,34(8):1-5.
[14] Wallace B,Pinkney F L,Scott R,et al.The near earth object surveillance satellite(NEOSSat)[C/OL].doi:10.1117/12.567077.
[15] 雷祥旭,桑吉章,李振伟.LEO空间目标地基甚短弧角度数据初轨确定[J].测绘地理信息,2019,44(2):71-73.
[16] 刘磊,曹建峰.基于天基光学测角的高轨空间目标轨道确定[J].光学学报,2021,41(19):1912002.
[17] 胡寿村,季江徽,赵玉晖,等.嫦娥二号飞越小行星试验中图塔蒂斯轨道确定与精度分析[J].中国科学:技术科学,2013,43:506-511.
文章导航

/