An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561

G. Lacedelli*, L. Malavolta, L. Borsato, G. Piotto, D. Nardiello, A. Mortier, M. Stalport, A. Collier Cameron, E. Poretti, Lars A. Buchhave, M. López-Morales, V. Nascimbeni, T. G. Wilson, S. Udry, D. W. Latham, A. S. Bonomo, M. Damasso, X. Dumusque, J. M. Jenkins, C. LovisK. Rice, D. Sasselov, J. N. Winn, G. Andreuzzi, R. Cosentino, D. Charbonneau, L. Di Fabrizio, A. F. Martinez Fiorenzano, A. Ghedina, A. Harutyunyan, F. Lienhard, G. Micela, E. Molinari, I. Pagano, F. Pepe, D. F. Phillips, M. Pinamonti, G. Ricker, G. Scandariato, A. Sozzetti, C. A. Watson

*Corresponding author for this work

Research output: Contribution to journalJournal articleResearchpeer-review

19 Downloads (Pure)

Abstract

Based on HARPS-N radial velocities (RVs) and TESS photometry, we present a full characterisation of the planetary system orbiting the late G dwarf TOI-561. After the identification of three transiting candidates by TESS, we discovered two additional external planets from RV analysis. RVs cannot confirm the outer TESS transiting candidate, which would also make the system dynamically unstable. We demonstrate that the two transits initially associated with this candidate are instead due to single transits of the two planets discovered using RVs. The four planets orbiting TOI-561 include an ultra-shortperiod (USP) super-Earth (TOI-561 b) with period Pb=0.45 d, mass Mb=1.59±0.36 M⊕ and radius Rb=1.42±0.07R⊕, and three mini-Neptunes: TOI-561 c, with Pc=10.78 d,Mc=5.40±0.98 M⊕, Rc=2.88±0.09 R⊕;TOI-561 d, with Pd=25.6 d, Md=11.9±1.3 M⊕,Rd=2.53±0.13 R⊕; and TOI-561 e, with Pe=77.2d, Me=16.0±2.3 M⊕, Re=2.67±0.11R⊕. Having a density of 3.0±0.8 g cm−3, TOI-561 b is the lowest density USP planet known to date. Our N-body simulations confirm the stability of the system and predict a strong, anti-correlated, long-term transit time variation signal between planets d and e. The unusual density ofthe inner super-Earth and the dynamical interactions between the outer planets make TOI-561 an interesting follow-up target.
Original languageEnglish
JournalMonthly Notices of the Royal Astronomical Society
Volume501
Pages (from-to)4148–4166
ISSN0035-8711
DOIs
Publication statusPublished - 2021

Keywords

  • Planets and satellites: detection
  • Planets and satellites: composition
  • Star: individual: TOI-561 (TIC 377064495, Gaia DR2 3850421005290172416)
  • Techniques: photometric –
  • Techniques: radial velocities

Fingerprint

Dive into the research topics of 'An unusually low density ultra-short period super-Earth and three mini-Neptunes around the old star TOI-561'. Together they form a unique fingerprint.

Cite this