Prospects for Directly Imaging Young Giant Planets at Optical Wavelengths

Keyphrases

• Giant Planets 100%
• Optical Wavelength 100%
• WFIRST 100%
• Reflected Light 66%
• Direct Imaging 66%
• Self-luminous 66%
• Thermal Emission 33%
• Spectral Features 33%
• Space-based 33%
• Light Scattering 33%
• Wavelength Range 33%
• Heat of Formation 33%
• Photometric Imaging 33%
• Evolutionary Model 33%
• Contrast Ratio 33%
• Science Case 33%
• Wide Field Infrared Survey Telescope 33%
• Residual Heat 33%

Physics

• Extrasolar Gas Giants 100%
• Thermal Emission 50%
• Heat of Formation 50%