SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems. From planetary disks to nearby Super Earths

Boccaletti, Anthony; Schneider, Jean; Traub, Wes; Lagage, Pierre-Olivier; Stam, Daphne; Gratton, Raffaele; Trauger, John; Cahoy, Kerri; Snik, Frans; Baudoz, Pierre; Galicher, Raphael; Reess, Jean-Michel; Mawet, Dimitri; Augereau, Jean-Charles; Patience, Jenny; Kuchner, Marc; 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; SPICES Team; Mas, M.; Rouan, D.; Perrin, G.; Lacour, S.; Thébault, P.; Nguyen, N.; Ibgui, L.; Arenou, F.; Lestrade, J. F.; N'Diaye, M.; Dohlen, K.; Ferrari, M.; Hugot, E.; Beuzit, J.-L.; Lagrange, A.-M.; Martinez, P.; Barthelemey, M.; Mugnier, L.; Keller, C.; Marley, M.; Kalas, P.; Stapelfeldt, K.; Brown, R.; Kane, S.; Desidera, S.; Sozzetti, A.; Mura, A.; Martin, E. L.; Bouy, H.; Allan, A.; King, R.; Vigan, A.; Churcher, L.; Udry, S.; Matsuo, T.; Nishikawa, J.; Hanot, C.; Wolf, S.; Kaltenegger, L.; Klahr, H.; Pilat-Lohinger, E.

doi:10.1007/s10686-012-9290-5

Article (Scientific journals)

SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems. From planetary disks to nearby Super Earths

Boccaletti, Anthony; Schneider, Jean; Traub, Wes et al.

2012 • In Experimental Astronomy, 34, p. 355-384

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https://hdl.handle.net/2268/243765

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10.1007/s10686-012-9290-5

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Keywords :

Exoplanets; High contrast imaging; Astrophysics - Instrumentation and Methods for Astrophysics

Abstract :

[en] 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[SUB]⊕[/SUB]) as well as circumstellar disks as faint as a few times the zodiacal light in the Solar System.

Disciplines :

Space science, astronomy & astrophysics

Author, co-author :

Boccaletti, Anthony; LESIA, Paris Observatory, Meudon, France

Schneider, Jean; LUTH, Paris Observatory, Meudon, France

Traub, Wes; NASA-JPL, Pasadena, CA, USA

Lagage, Pierre-Olivier; SAp/CEA, Saclay, France

Stam, Daphne; SRON, Utrecht, The Netherlands

Gratton, Raffaele; INAF, Padova Observatory, Padova, Italy

Trauger, John; NASA-JPL, Pasadena, CA, USA

Cahoy, Kerri; NASA Ames Research Center, Moffett Field, CA, USA

Snik, Frans; Sterrekundig Instituut Utrecht, Utrecht, The Netherlands

Baudoz, Pierre; LESIA, Paris Observatory, Meudon, France

More authors (62 more)

Language :

English

Title :

SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems. From planetary disks to nearby Super Earths

Publication date :

01 October 2012

Journal title :

Experimental Astronomy

ISSN :

0922-6435

eISSN :

1572-9508

Publisher :

Kluwer Academic Publishers, Netherlands

Volume :

Pages :

355-384

Peer reviewed :

Peer Reviewed verified by ORBi

Additional URL :

https://ui.adsabs.harvard.edu/abs/2012ExA....34..355B

Available on ORBi :

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