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SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems

Authors :
Massachusetts Institute of Technology. Department of Aeronautics and Astronautics
Cahoy, Kerri
Boccaletti, Anthony
Schneider, Jean
Traub, Wes
Lagage, Pierre-Olivier
Stam, Daphne
Gratton, Raffaele
Trauger, John
Snik, Frans
Baudoz, Pierre
Galicher, Raphael
Reess, Jean-Michel
Mawet, Dimitri
Augereau, Jean-Charles
Patience, Jenny
Kuchner, Marc J.
Wyatt, Mark
Pantin, Eric
Maire, Anne-Lise
Vérinaud, Christophe
Ronayette, Samuel
Dubreuil, Didier
Min, Michiel
Rodenhuis, Michiel
Mesa, Dino
Belikov, Russ
Guyon, Olivier
Tamura, Motohide
Murakami, Naoshi
Beerer, Ingrid Mary
Massachusetts Institute of Technology. Department of Aeronautics and Astronautics
Cahoy, Kerri
Boccaletti, Anthony
Schneider, Jean
Traub, Wes
Lagage, Pierre-Olivier
Stam, Daphne
Gratton, Raffaele
Trauger, John
Snik, Frans
Baudoz, Pierre
Galicher, Raphael
Reess, Jean-Michel
Mawet, Dimitri
Augereau, Jean-Charles
Patience, Jenny
Kuchner, Marc J.
Wyatt, Mark
Pantin, Eric
Maire, Anne-Lise
Vérinaud, Christophe
Ronayette, Samuel
Dubreuil, Didier
Min, Michiel
Rodenhuis, Michiel
Mesa, Dino
Belikov, Russ
Guyon, Olivier
Tamura, Motohide
Murakami, Naoshi
Beerer, Ingrid Mary
Source :
MIT web domain
Publication Year :
2013

Abstract

SPICES (Spectro-Polarimetric Imaging and Characterization of Exoplanetary Systems) is a five-year M-class mission proposed to ESA Cosmic Vision. Its purpose is to image and characterize long-period extrasolar planets and circumstellar disks in the visible (450–900 nm) at a spectral resolution of about 40 using both spectroscopy and polarimetry. By 2020/2022, present and near-term instruments will have found several tens of planets that SPICES will be able to observe and study in detail. Equipped with a 1.5 m telescope, SPICES can preferentially access exoplanets located at several AUs (0.5–10 AU) from nearby stars (<25 pc) with masses ranging from a few Jupiter masses to Super Earths (∼2 Earth radii, ∼10 M[subscript ⊕]) as well as circumstellar disks as faint as a few times the zodiacal light in the Solar System.

Details

Database :
OAIster
Journal :
MIT web domain
Notes :
application/pdf, en_US
Publication Type :
Electronic Resource
Accession number :
edsoai.on1141893799
Document Type :
Electronic Resource