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Imaging Young Giant Planets From Ground and Space
- Source :
- Publications of the Astronomical Society of the Pacific, Publications of the Astronomical Society of the Pacific, 2010, 122, pp.162-200. ⟨10.1086/651057⟩
- Publication Year :
- 2010
- Publisher :
- HAL CCSD, 2010.
-
Abstract
- High-contrast imaging can find and characterize gas giant planets around nearby young stars and the closest M stars, complementing radial velocity and astrometric searches by exploring orbital separations inaccessible to indirect methods. Ground-based coronagraphs are already probing within 25 AU of nearby young stars to find objects as small as ∼3 MJup∼3 MJup. This paper contrasts near-term and future ground-based capabilities with high-contrast imaging modes of the James Webb Space Telescope (JWST). Monte Carlo modeling reveals that JWST can detect planets with masses as small as 0.2 MJup0.2 MJup across a broad range of orbital separations. We present new calculations for planet brightness as a function of mass and age for specific JWST filters and extending to 0.1 MJup0.1 MJup.
- Subjects :
- Physics
Brightness
Gas giant
James Webb Space Telescope
Astrophysics::Instrumentation and Methods for Astrophysics
Giant planet
Astronomy
Astronomy and Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
Exoplanet
Radial velocity
Stars
Space and Planetary Science
Planet
Astrophysics::Solar and Stellar Astrophysics
Astrophysics::Earth and Planetary Astrophysics
[PHYS.ASTR]Physics [physics]/Astrophysics [astro-ph]
Astrophysics::Galaxy Astrophysics
Subjects
Details
- Language :
- English
- ISSN :
- 00046280 and 15383873
- Database :
- OpenAIRE
- Journal :
- Publications of the Astronomical Society of the Pacific, Publications of the Astronomical Society of the Pacific, 2010, 122, pp.162-200. ⟨10.1086/651057⟩
- Accession number :
- edsair.doi.dedup.....6158c30c9c45a90147080ce58e198116