recognition of biospheres
|
Earth's near-infrared fingerprint |
One of the central challenges in astrobiology is the detection of the signatures
of life over interstellar distances. In the case of contemporary terrestrial
life, the most distinctive signatures include the high concentration of
free oxygen (O2) and ozone
(O3) in the atmosphere and the green surface coloration due to
chlorophyll, all the result of the activity
of plants. Similar features in the spectra of extrasolar
planets, when it becomes possible to observe these, will provide strong
evidence of Earth-like biospheres.1 Less is known about the principal
signatures of the terrestrial biosphere prior to about one billion years
ago (see Earth, early history). Further
work is needed in this area so that techniques can be developed to search
for biospheres akin to that of the primitive Earth. See also Origins
Program. Reference
- Leger, A., Ollivier, M., Altwegg, K., and Woolf, N. "Is the Presence
of H2O and O3 in an Exoplanet a Reliable Signature
of a Biological Activity?," Astronomy & Astrophysics, 341,
304 (1998).
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