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http://hdl.handle.net/20.500.12386/34760
Titolo: | SPICES: spectro-polarimetric imaging and characterization of exoplanetary systems. From planetary disks to nearby Super Earths | Autori: | 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, MARCO 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, Silvano SOZZETTI, Alessandro MURA, Alessandro 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. |
Data pubblicazione: | 2012 | Rivista: | EXPERIMENTAL ASTRONOMY | Numero: | 34 | Fascicolo: | 2 | Da pagina:: | 355 | 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<SUB>⊕</SUB>) as well as circumstellar disks as faint as a few times the zodiacal light in the Solar System. | URI: | http://hdl.handle.net/20.500.12386/34760 | URL: | https://link.springer.com/article/10.1007/s10686-012-9290-5 https://api.elsevier.com/content/abstract/scopus_id/84866927948 |
ISSN: | 0922-6435 | DOI: | 10.1007/s10686-012-9290-5 | Bibcode ADS: | 2012ExA....34..355B | Fulltext: | open |
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