Exoplanets - search methods, discoveries, and prospects for astrobiology

TL;DR

This paper reviews methods for discovering exoplanets, summarizes key discoveries, and discusses prospects for assessing their habitability and potential for supporting life, emphasizing relevance to astrobiology.

Contribution

It provides a comprehensive overview of exoplanet search techniques, recent discoveries, and future prospects for studying habitability and life potential from afar.

Findings

Exoplanet detection methods include transit and radial velocity techniques.

Over 260 exoplanets known as of 2008, with increasing discovery rate.

Potential habitability depends on factors like liquid water and planetary composition.

Abstract

Whereas the Solar System has Mars and Europa as the best candidates for finding fossil/extant life as we know it - based on complex carbon compounds and liquid water - the 263 (non-pulsar) planetary systems around other stars as known at 15 September 2008 could between them possess many more planets where life might exist. Moreover, the number of these exoplanetary systems is growing steadily, and with this growth there is an increase in the number of planets that could bear carbon-liquid water life. In this brief review the main methods by which exoplanets are being discovered are outlined, and then the discoveries that have so far been made are presented. Habitability is then discussed, and an outline presented of how a planet could be studied from afar to determine whether it is habitable, and whether it is indeed inhabited. This review is aimed at the astrobiology community, which spans many disciplines, few of which involve exoplanets. It is therefore at a basic level and concentrates on the major topics.