Searching for life with the Terrestrial Planet Finder:: Lagrange point options for a formation flying interferometer

被引:26
作者
Beichman, C
Gómez, G
Lo, M
Masdemont, J
Romans, L
机构
[1] CALTECH, Jet Prop Lab, Pasadena, CA 91109 USA
[2] Univ Barcelona, Dept Matemat APlicada & Anal, E-08007 Barcelona, Spain
[3] Univ Politecn Catalunya, Dept Matemat Aplicada, E-08028 Barcelona, Spain
来源
ASTRONOMY AT IR/SUBMM AND THE MICROWAVE BACKGROUND | 2004年 / 34卷 / 03期
基金
美国国家航空航天局;
关键词
astronomical search for origins; searching for life; Terrestrial Planet Finder; TPF; halo orbit; L-2; heliocentric orbit;
D O I
10.1016/j.asr.2003.05.032
中图分类号
V [航空、航天];
学科分类号
08 ; 0825 ;
摘要
Whether life exists beyond Earth is a fundamental question. To answer this and related questions requires access to space, making the search for life within our solar system and beyond a quest that only the National Aeronautics and Space Administration (NASA), along with its international partners, can answer. The Terrestrial Planet Finder (TPF) is one of the key missions in NASA's Astronomical Search for Origins. In this paper, we describe the mission design for TPF assuming a distributed spacecraft concept using formation flight around both a halo orbit about the Sun-Earth L-2 as well as a heliocentric orbit. Although the mission architecture is still under study, the next two years will include study of four design concepts and a down select to two concepts around 2005. TPF is anticipating a Phase A start around 2007 and a launch sometime around 2015. (C) 2004 COSPAR. Published by Elsevier Ltd. All rights reserved.
引用
收藏
页码:637 / 644
页数:8
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