The Astrophysical Journal Letters (Jan 2024)

Prominent Mid-infrared Excess of the Dwarf Planet (136472) Makemake Discovered by JWST/MIRI Indicates Ongoing Activity

  • Csaba Kiss,
  • Thomas G. Müller,
  • Anikó Farkas-Takács,
  • Attila Moór,
  • Silvia Protopapa,
  • Alex H. Parker,
  • Pablo Santos-Sanz,
  • Jose Luis Ortiz,
  • Bryan J. Holler,
  • Ian Wong,
  • John Stansberry,
  • Estela Fernández-Valenzuela,
  • Christopher R. Glein,
  • Emmanuel Lellouch,
  • Esa Vilenius,
  • Csilla E. Kalup,
  • Zsolt Regály,
  • Róbert Szakáts,
  • Gábor Marton,
  • András Pál,
  • Gyula M. Szabó

DOI
https://doi.org/10.3847/2041-8213/ad8dcb
Journal volume & issue
Vol. 976, no. 1
p. L9

Abstract

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We report on the discovery of a very prominent mid-infrared (18–25 μ m) excess associated with the trans-Neptunian dwarf planet (136472) Makemake. The excess, detected by the Mid-Infrared Instrument of the James Webb Space Telescope, along with previous measurements from the Spitzer and Herschel space telescopes, indicates the occurrence of temperatures of ∼150 K, much higher than what solid surfaces at Makemake’s heliocentric distance could reach by solar irradiation. We identify two potential explanations: a continuously visible, currently active region powered by subsurface upwelling and possibly cryovolcanic activity covering ≤1% of Makemake’s surface or an as-yet-undetected ring containing very small carbonaceous dust grains, which have not been seen before in trans-Neptunian or Centaur rings. Both scenarios point to unprecedented phenomena among trans-Neptunian objects and could greatly impact our understanding of these distant worlds.

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