Detectability of Terrestrial Planets in Multi-Planet Systems: Preliminary Report
Wesley A. Traub, Charles Beichman, Andrew F. Boden, Alan P. Boss,, Stefano Casertano, Joseph Catanzarite, Debra Fischer, Eric. B. Ford, Andrew, Gould, Sam Halverson, Andrew Howard, Shigeru Ida, N. Jeremy Kasdin, Gregory, P. Laughlin, Harold F. Levison, Douglas Lin
TL;DR
This paper investigates the potential to detect Earth-like planets in multi-planet systems using astrometric and radial velocity methods through preliminary double-blind calculations.
Contribution
It presents initial findings on the detectability of terrestrial planets in multi-planet systems with specific observational techniques.
Findings
Preliminary results suggest possible detectability under certain conditions.
Double-blind calculations provide unbiased assessment of detection capabilities.
Astrometric and radial velocity methods show complementary strengths.
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.
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