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Title: The hunt for planet nine: atmosphere, spectra, evolution, and detectability

Journal Article · · Astrophysical Journal Letters
; ; ; ; ;  [1]; ;  [2];  [3];  [4]
  1. Department of Astronomy and Astrophysics, University of California, Santa Cruz, CA (United States)
  2. NASA Ames Research Center, Mountain View, CA (United States)
  3. University of Rostock, Rostock (Germany)
  4. Dordt College, Sioux Center, IA (United States)

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 T{sub eff}, from ∼35 to 50 K for masses of 5–20 M {sub ⊕}, and we also explore lower T{sub eff} values. Possible planetary radii could readily span from 2.7 to 6 R {sub ⊕}, depending on the mass fraction of any H/He envelope. Given its cold atmospheric temperatures, the planet encounters significant methane condensation, which dramatically alters the atmosphere away from simple Neptune-like expectations. We find that the atmosphere is strongly depleted in molecular absorption at visible wavelengths, suggesting a Rayleigh scattering atmosphere with a high geometric albedo approaching 0.75. We highlight two diagnostics for the atmosphere’s temperature structure: (1) the value of the methane mixing ratio above the methane cloud and (2) the wavelength at which cloud scattering can be seen, which yields the cloud-top pressure. Surface reflection may be seen if the atmosphere is thin. Due to collision-induced opacity of H{sub 2} in the infrared, the planet would be extremely blue instead of red in the shortest wavelength WISE colors if methane is depleted and would, in some cases, exist on the verge of detectability by WISE. For a range of models, thermal fluxes from ∼3 to 5 μm are ∼20 orders of magnitude larger than blackbody expectations. We report a search of the AllWISE Source Catalog for Planet Nine, but find no detection.

OSTI ID:
22869111
Journal Information:
Astrophysical Journal Letters, Vol. 824, Issue 2; Other Information: Country of input: International Atomic Energy Agency (IAEA); ISSN 2041-8205
Country of Publication:
United States
Language:
English