The Astrophysical Journal Letters (Jan 2023)

JWST-TST DREAMS: Quartz Clouds in the Atmosphere of WASP-17b

  • David Grant,
  • Nikole K. Lewis,
  • Hannah R. Wakeford,
  • Natasha E. Batalha,
  • Ana Glidden,
  • Jayesh Goyal,
  • Elijah Mullens,
  • Ryan J. MacDonald,
  • Erin M. May,
  • Sara Seager,
  • Kevin B. Stevenson,
  • Jeff A. Valenti,
  • Channon Visscher,
  • Lili Alderson,
  • Natalie H. Allen,
  • Caleb I. Cañas,
  • Knicole Colón,
  • Mark Clampin,
  • Néstor Espinoza,
  • Amélie Gressier,
  • Jingcheng Huang,
  • Zifan Lin,
  • Douglas Long,
  • Dana R. Louie,
  • Maria Peña-Guerrero,
  • Sukrit Ranjan,
  • Kristin S. Sotzen,
  • Daniel Valentine,
  • Jay Anderson,
  • William O. Balmer,
  • Andrea Bellini,
  • Kielan K. W. Hoch,
  • Jens Kammerer,
  • Mattia Libralato,
  • C. Matt Mountain,
  • Marshall D. Perrin,
  • Laurent Pueyo,
  • Emily Rickman,
  • Isabel Rebollido,
  • Sangmo Tony Sohn,
  • Roeland P. van der Marel,
  • Laura L. Watkins

DOI
https://doi.org/10.3847/2041-8213/acfc3b
Journal volume & issue
Vol. 956, no. 2
p. L32

Abstract

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Clouds are prevalent in many of the exoplanet atmospheres that have been observed to date. For transiting exoplanets, we know if clouds are present because they mute spectral features and cause wavelength-dependent scattering. While the exact composition of these clouds is largely unknown, this information is vital to understanding the chemistry and energy budget of planetary atmospheres. In this work, we observe one transit of the hot Jupiter WASP-17b with JWST’s Mid-Infrared Instrument Low Resolution Spectrometer and generate a transmission spectrum from 5 to 12 μ m. These wavelengths allow us to probe absorption due to the vibrational modes of various predicted cloud species. Our transmission spectrum shows additional opacity centered at 8.6 μ m, and detailed atmospheric modeling and retrievals identify this feature as SiO _2 (s) (quartz) clouds. The SiO _2 (s) clouds model is preferred at 3.5–4.2 σ versus a cloud-free model and at 2.6 σ versus a generic aerosol prescription. We find the SiO _2 (s) clouds are composed of small ∼0.01 μ m particles, which extend to high altitudes in the atmosphere. The atmosphere also shows a depletion of H _2 O, a finding consistent with the formation of high-temperature aerosols from oxygen-rich species. This work is part of a series of studies by our JWST Telescope Scientist Team (JWST-TST), in which we will use Guaranteed Time Observations to perform Deep Reconnaissance of Exoplanet Atmospheres through Multi-instrument Spectroscopy (DREAMS).

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