The Far Future of Exoplanet Direct Characterization
Artikel i vetenskaplig tidskrift, 2010
We describe future steps in the direct characterization of habitable exoplanets subsequent to medium and large mission projects currently underway and investigate the benefits of spectroscopic and direct imaging approaches. We show that, after third- and fourth-generation missions have been conducted over the course of the next 100 years, a significant amount of time will lapse before we will have the capability to observe directly the morphology of extrasolar organisms.
signatures
Exo-moons
Surface features
Direct imaging
Habitable exoplanets
High-resolution spectroscopy
Far future missions
extra-solar planets
search
imager
Författare
J. Schneider
Observatoire de Paris-Meudon
A. Leger
Université Paris-Sud
M. Fridlund
Europeiska rymdorganisationen (ESA)
G. J. White
Open University
STFC Rutherford Appleton Laboratory
C. Eiroa
Universidad Autonoma de Madrid (UAM)
T. Henning
Max-Planck-Gesellschaft
T. Herbst
Max-Planck-Gesellschaft
H. Lammer
Institut fur Weltraumforschung
René Liseau
Chalmers, Institutionen för radio- och rymdvetenskap, Radioastronomi och astrofysik
F. Paresce
Istituto nazionale di astrofisica (INAF)
A. Penny
STFC Rutherford Appleton Laboratory
Royal Observatory
A. Quirrenbach
Landessternwarte Heidelberg-Königstuhl
H. Rottgering
Universiteit Leiden
F. Selsis
Université de Bordeaux
C. Beichman
California Institute of Technology (Caltech)
W. Danchi
National Aeronautics and Space Administration (NASA)
L. Kaltenegger
Harvard-Smithsonian Center for Astrophysics
J. Lunine
University of Arizona
D. Stam
Netherlands Institute for Space Research (SRON)
G. Tinetti
University College London (UCL)
Astrobiology
1531-1074 (ISSN)
Vol. 10 1 121-126Ämneskategorier (SSIF 2011)
Astronomi, astrofysik och kosmologi
Fundament
Grundläggande vetenskaper
DOI
10.1089/ast.2009.0371