Detectability of Earth-like Planets in Circumstellar Habitable Zones of Binary Star Systems with Sun-like Components
Siegfried Eggl, Nader Haghighipour, Elke Pilat-Lohinger

TL;DR
This paper analyzes the potential for detecting Earth-like planets in habitable zones of binary star systems, especially alpha Centauri, by providing analytical tools and discussing how stellar interactions influence detectability.
Contribution
It introduces analytical expressions for signals and probabilities of detecting terrestrial planets in binary systems, highlighting how stellar interactions can aid detection.
Findings
Radial velocity and astrometric signals can be analytically estimated.
Stellar interactions may enhance planet detectability.
Detectability of Earth-like planets in alpha Centauri is feasible with current methods.
Abstract
Given the considerable percentage of stars that are members of binaries or stellar multiples in the Solar neighborhood, it is expected that many of these binaries host planets, possibly even habitable ones. The discovery of a terrestrial planet in the alpha Centauri system supports this notion. Due to the potentially strong gravitational interaction that an Earth-like planet may experience in such systems, classical approaches to determining habitable zones, especially in close S-Type binary systems, can be rather inaccurate. Recent progress in this field, however, allows to identify regions around the star permitting permanent habitability. While the discovery of alpha Cen Bb has shown that terrestrial planets can be detected in solar-type binary stars using current observational facilities, it remains to be shown whether this is also the case for Earth analogues in habitable zones. We…
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