Detectability of Terrestrial Planets in Multi-Planet Systems: Preliminary Report
Earth and Planetary Astrophysics
2015-05-13 v1 Instrumentation and Methods for Astrophysics
Abstract
We ask if Earth-like planets (terrestrial mass and habitable-zone orbit) can be detected in multi-planet systems, using astrometric and radial velocity observations. We report here the preliminary results of double-blind calculations designed to answer this question.
Cite
@article{arxiv.0904.0822,
title = {Detectability of Terrestrial Planets in Multi-Planet Systems: Preliminary Report},
author = {Wesley A. Traub and Charles Beichman and Andrew F. Boden and Alan P. Boss and Stefano Casertano and Joseph Catanzarite and Debra Fischer and Eric. B. Ford and Andrew Gould and Sam Halverson and Andrew Howard and Shigeru Ida and N. Jeremy Kasdin and Gregory P. Laughlin and Harold F. Levison and Douglas Lin and Valeri Makarov and James Marr and Matthew Muterspaugh and Sean N. Raymond and Dmitry Savransky and Michael Shao and Alessandro Sozzetti and Cengxing Zhai},
journal= {arXiv preprint arXiv:0904.0822},
year = {2015}
}
Comments
10 pages, 0 figures