Biology
Scientific paper
Dec 2003
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2003asbio...3..681v&link_type=abstract
Astrobiology, Volume 3, Issue 4, pp. 681-688.
Biology
11
Extrasolar Planets, Geodynamics, Habitable Zone, Orbital Stability, Planetary Climate
Scientific paper
We discuss the possibility of Earth-type planets in the planetary system of 55 Cancri, a nearby G8 V star, which is host to two, possibly three, giant planets. We argue that Earth-type planets around 55 Cancri are in principle possible. Several conditions are necessary. First, Earth-type planets must have formed despite the existence of the close-in giant planet(s). In addition, they must be orbitally stable in the region of habitability considering that the stellar habitable zone is relatively close to the star compared to the Sun because of 55 Cancri's low luminosity and may therefore be affected by the close-in giant planet(s). We estimate the likelihood of Earth-type planets around 55 Cancri based on the integrated system approach previously considered, which provides a way of assessing the long-term possibility of photosynthetic biomass production under geodynamic conditions.
Bounama Ch.
Cuntz Manfred
Franck Siegfried
von Bloh Werner
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