Digital Collections @ Dordt Faculty Work Comprehensive List 6-2016 Hunt for Planet Nine: Atmosphere, Spectra, Evolution, and Detectability Jonathan J. Fortney University of California, Santa Cruz Mark S. Marley NASA Ames Research Center Gregory Laughlin University of California, Santa Cruz Nadine Nettelmann University of Rostock Caroline V. Morley University of California, Santa Cruz See next page for additional authors Follow this and additional works at: https://digitalcollections.dordt.edu/faculty_work Part of the Astrophysics and Astronomy Commons Recommended Citation Fortney, J. J., Marley, M. S., Laughlin, G., Nettelmann, N., Morley, C. V., Lupu, R. E., Visscher, C., Jeremic, P., Khadder, W. G., & Hargrave, M. (2016). Hunt for Planet Nine: Atmosphere, Spectra, Evolution, and Detectability. Astrophysical Journal Letters, 824 (2) https://doi.org/10.3847/2041-8205/824/2/L25 This Article is brought to you for free and open access by Digital Collections @ Dordt. It has been accepted for inclusion in Faculty Work Comprehensive List by an authorized administrator of Digital Collections @ Dordt. For more information, please contact
[email protected]. Hunt for Planet Nine: Atmosphere, Spectra, Evolution, and Detectability Abstract We investigate the physical characteristics of the solar system's proposed Planet Nine using modeling tools with a heritage of studying Uranus and Neptune. For a range of plausible masses and interior structures, we find upper limits on the intrinsic , from ~35 to 50 K for masses of 5–20 M ⊕, and we also explore lower values. Possible planetary radii could readily span from 2.7 to 6 R ⊕, depending on the mass fraction of any H/He envelope.