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Detecting Magnetic Fields in Exoplanets with Spectropolarimetry of the Helium Line at 1083 nm
Antonija Oklopčić, Makana Silva, Paulo Montero-Camacho +1
The magnetic fields of the solar system planets provide valuable insights into the planets' interiors and can have dramatic consequences for the evolution of their atmospheres and…
A New Window into Escaping Exoplanet Atmospheres: 10830 Å Line of Helium
Antonija Oklopčić, Christopher M. Hirata
Observational evidence for escaping exoplanet atmospheres has been obtained for a few exoplanets to date. It comes from strong transit signals detected in the ultraviolet, most not…
Solar system science with the Wide-Field InfraRed Survey Telescope (WFIRST)
B. J. Holler, S. N. Milam, J. M. Bauer +30
We present a community-led assessment of the solar system investigations achievable with NASA's next-generation space telescope, the Wide Field InfraRed Survey Telescope (WFIRST).…
How does the shape of the stellar spectrum affect the Raman scattering features in the albedo of exoplanets?
Antonija Oklopčić, Christopher M. Hirata, Kevin Heng
Diagnostic potential of the spectral signatures of Raman scattering imprinted in planetary albedo spectra at short optical wavelengths has been demonstrated in research on Solar Sy…
Raman Scattering by Molecular Hydrogen and Nitrogen in Exoplanetary Atmospheres
Antonija Oklopčić, Christopher M. Hirata, Kevin Heng
An important source of opacity in exoplanet atmospheres at short visible and near-UV wavelengths is Rayleigh scattering of light on molecules. It is accompanied by a related, albei…