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Lego Figure holding a lego telescope. Photo

Jens Hoeijmakers

ASSOCIATE SENIOR LECTURER

Lego Figure holding a lego telescope. Photo

Redshifted Sodium Transient near Exoplanet Transit

Author

  • Apurva V. Oza
  • Julia V. Seidel
  • H. Jens Hoeijmakers
  • Athira Unni
  • Aurora Y. Kesseli
  • Carl A. Schmidt
  • Thirupathi Sivarani
  • Aaron Bello-Arufe
  • Andrea Gebek
  • Moritz Meyer zu Westram
  • Sérgio G. Sousa
  • Rosaly M.C. Lopes
  • Renyu Hu
  • Katherine de Kleer
  • Chloe Fisher
  • Sébastien Charnoz
  • Ashley D. Baker
  • Samuel P. Halverson
  • Nick M. Schneider
  • Angelica Psaridi
  • Aurélien Wyttenbach
  • Santiago Torres
  • Ishita Bhatnagar
  • Robert E. Johnson

Summary, in English

Neutral sodium (Na i) is an alkali metal with a favorable absorption cross section such that tenuous gases are easily illuminated at select transiting exoplanet systems. We examine both the time-averaged and time-series alkali spectral flux individually, over 4 nights at a hot Saturn system on a ∼2.8 day orbit about a Sun-like star WASP-49 A. Very Large Telescope/ESPRESSO observations are analyzed, providing new constraints. We recover the previously confirmed residual sodium flux uniquely when averaged, whereas night-to-night Na i varies by more than an order of magnitude. On HARPS/3.6 m Epoch II, we report a Doppler redshift at v Γ,NaD = + 9.7 ± 1.6 km s−1 with respect to the planet’s rest frame. Upon examining the lightcurves, we confirm night-to-night variability, on the order of ∼1%-4% in NaD, rarely coinciding with exoplanet transit, not readily explained by stellar activity, starspots, tellurics, or the interstellar medium. Coincident with the ∼+10 km s−1 Doppler redshift, we detect a transient sodium absorption event dF NaD/F = 3.6% ± 1% at a relative difference of ΔF NaD(t) ∼ 4.4% ± 1%, lasting Δt NaD ≳ 40 minutes. Since exoplanetary alkali signatures are blueshifted due to the natural vector of radiation pressure, estimated here at roughly ∼−5.7 km s−1, the radial velocity is rather at +15.4 km s−1, far larger than any known exoplanet system. Given that the redshift magnitude v Γ is in between the Roche limit and dynamically stable satellite orbits, the transient sodium may be a putative indication of a natural satellite orbiting WASP-49 A b.

Department/s

  • eSSENCE: The e-Science Collaboration
  • Astrophysics

Publishing year

2024-10-01

Language

English

Publication/Series

Astrophysical Journal Letters

Volume

973

Issue

2

Document type

Journal article

Publisher

IOP Publishing

Topic

  • Astronomy, Astrophysics and Cosmology

Status

Published

ISBN/ISSN/Other

  • ISSN: 2041-8205