ASTRONOMICAL SEARCHES FOR EARTH-LIKE PLANETS AND SIGNS OF LIFE

• Published in: Annual review of astronomy and astrophysics 1998-01, Vol.36 (1), p.507-537
• Main Authors: Woolf, Neville, Angel, J. Roger
• Format: Article
• Language: English
• Subjects: exobiology; extrasolar; origins; terrestrial
• ISSN: 0066-4146; 1545-4282
• DOI: 10.1146/annurev.astro.36.1.507

If Earth-like planets orbit nearby stars, they could be detectable with specially designed telescopes. Direct observations would be very revealing, particularly low resolution infrared spectra, which could establish habitability on the basis of temperature and atmospheric water. Abundant, primitive life based on organized molecular structure might reveal itself, as on Earth, by an atmospheric composition modified in ways unlikely to be from inorganic processes. The technical challenge is to detect and obtain spectra of an object with M bol ∼ 28 that is very close to a star and some 5 × 10 9 times less luminous. Indirect methods, used to detect Jupiter-mass planets, do not seem to offer an easy intermediate step to finding Earth-like planets. However, the direct detection techniques needed for spectroscopy also offer a viable method for discovery by imaging. Thermal infrared wavelengths, in which a planet emits most energy, are the most favorable. A robust search for planets of ∼100 nearby solar-type stars, with spectroscopic follow-up of Earth-like candidates, could be made with an interferometer ∼75 m in length. In visible light, the Next Generation Space Telescope (NGST) could, with the addition of a high resolution correction instrument, see Earth-like planets around a dozen or so of the nearest stars. Both infrared and optical instruments are possible within the range of current space agency plans.