Deciphering Spectral Fingerprints of Habitable Exoplanets
Artikel i vetenskaplig tidskrift, 2010
We discuss how to read a planet's spectrum to assess its habitability and search for the signatures of a biosphere. After a decade rich in giant exoplanet detections, observation techniques have advanced to a level where we now have the capability to find planets of less than 10 Earth masses (M-Earth) (so-called "super Earths''), which may be habitable. How can we characterize those planets and assess whether they are habitable? This new field of exoplanet search has shown an extraordinary capacity to combine research in astrophysics, chemistry, biology, and geophysics into a new and exciting interdisciplinary approach to understanding our place in the Universe. The results of a first-generation mission will most likely generate an amazing scope of diverse planets that will set planet formation, evolution, and our planet into an overall context.
atmosphere
red-edge
life
Habitable planets
search
earth-like planets
Exoplanet search
extrasolar terrestrial planets
infrared radiation
stars
Biomarkers
Planetary atmospheres
thermal emission
hd 189733b
Författare
L. Kaltenegger
Harvard-Smithsonian Center for Astrophysics
F. Selsis
Université de Bordeaux
M. Fridlund
European Space Research and Technology Centre (ESA ESTEC)
H. Lammer
Institut fur Weltraumforschung
C. Beichman
Jet Propulsion Laboratory, California Institute of Technology
W. Danchi
NASA Goddard Space Flight Center
C. Eiroa
Universidad Autonoma de Madrid (UAM)
T. Henning
Max-Planck-Gesellschaft
T. Herbst
Max-Planck-Gesellschaft
A. Leger
Université Paris-Sud
René Liseau
Chalmers, Institutionen för radio- och rymdvetenskap, Radioastronomi och astrofysik
J. Lunine
University of Arizona
F. Paresce
Istituto nazionale di astrofisica (INAF)
A. Penny
STFC Rutherford Appleton Laboratory
A. Quirrenbach
Landessternwarte Heidelberg-Königstuhl
H. Rottgering
Universiteit Leiden
J. Schneider
Observatoire de Paris-Meudon
D. Stam
Netherlands Institute for Space Research (SRON)
G. Tinetti
University College London (UCL)
G. J. White
STFC Rutherford Appleton Laboratory
Open University
Astrobiology
1531-1074 (ISSN)
Vol. 10 1 89-102Ämneskategorier
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
DOI
10.1089/ast.2009.0381