Confronting compositional confusion through the characterization of the sub-Neptune orbiting HD 77946

L. Palethorpe, A. Anna John, A. Mortier, J. Davoult, T. G. Wilson, K. Rice, A. C. Cameron, Y. Alibert, L. A. Buchhave, L. Malavolta, J. Cadman, M. López-Morales, X. Dumusque, A. M. Silva, S. N. Quinn, V. Van Eylen, S. Vissapragada, L. Affer, D. Charbonneau, R. CosentinoA. Ghedina, R. D. Haywood, D. W. Latham, F. Lienhard, A. F.Martínez Fiorenzano, M. Pedani, F. Pepe, M. Pinamonti, A. Sozzetti, M. Stalport, S. Udry, A. Vanderburg

Research output: Contribution to journalJournal articleResearchpeer-review

9 Downloads (Pure)

Abstract

We report on the detailed characterization of the HD 77946 planetary system. HD 77946 is an F5 (M*  = 1.17 M, R*  = 1.31 R) star, which hosts a transiting planet recently discovered by NASA’s Transiting Exoplanet Survey Satellite (TESS), classified as TOI-1778 b. Using TESS photometry, high-resolution spectroscopic data from HARPS-N, and photometry from CHEOPS, we measure the radius and mass from the transit and radial velocity observations, and find that the planet, HD 77946 b, orbits with period Pb  =  d, has a mass of Mb = 8.38 ± 1.32 M, and a radius of R. From the combination of mass and radius measurements, and the stellar chemical composition, the planet properties suggest that HD 77946 b is a sub-Neptune with a ∼1  per cent H/He atmosphere. However, a degeneracy still exists between water-world and silicate/iron-hydrogen models, and even though interior structure modelling of this planet favours a sub-Neptune with a H/He layer that makes up a significant fraction of its radius, a water-world composition cannot be ruled out, as with K, water may be in a supercritical state. The characterization of HD 77946 b, adding to the small sample of well-characterized sub-Neptunes, is an important step forwards on our journey to understanding planetary formation and evolution pathways. Furthermore, HD 77946 b has one of the highest transmission spectroscopic metrics for small planets orbiting hot stars, thus transmission spectroscopy of this key planet could prove vital for constraining the compositional confusion that currently surrounds small exoplanets.

Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume529
Issue number4
Pages (from-to)3323-3341
ISSN0035-8711
DOIs
Publication statusPublished - 2024

Keywords

  • Planets and satellites: composition
  • Planets and satellites: fundamental parameters
  • Stars: individual (HD 77946)
  • Techniques: photometric
  • Techniques: radial velocities
  • Techniques: spectroscopic

Fingerprint

Dive into the research topics of 'Confronting compositional confusion through the characterization of the sub-Neptune orbiting HD 77946'. Together they form a unique fingerprint.

Cite this