HD 28109 hosts a trio of transiting Neptunian planets including a near-resonant pair, confirmed by ASTEP from Antarctica

• Published in: Monthly Notices of the Royal Astronomical Society
• Main Authors: Dransfield, Georgina, Dévora Pajares, Martín, Lissauer, Jack J.
• Format: Article in Journal/Newspaper
• Language: English
• Published: Oxford University Press 2022
• Subjects: Planets and satellites: detection; Planets and satellites: dynamical evolution and stability; Planets and satellites: fundamental parameters; Webb; Antarc*; Antarctica
• Online Access: http://hdl.handle.net/10481/76580; https://doi.org/10.1093/mnras/stac1383

We report on the disco v ery and characterization of three planets orbiting the F8 star HD 28109, which sits comfortably in TESS ’s continuous viewing zone. The two outer planets have periods of 56 . 0067 ±0 . 0003 d and 84 . 2597 + 0 . 0010 −0 . 0008 d, which implies a period ratio very close to that of the first-order 3:2 mean motion resonance, exciting transit timing variations (TTVs) of up to 60 min. These two planets were first identified by TESS , and we identified a third planet in the TESS photometry with a period of 22 . 8911 ±0 . 0004 d. We confirm the planetary nature of all three planetary candidates using ground-based photometry from Hazelwood , ASTEP , and LCO , including a full detection of the ∼9 h transit of HD 28109 c from Antarctica. The radii of the three planets are R b = 2 . 199 + 0 . 098 −0 . 10 R ⊕, R c = 4 . 23 ±0 . 11 R ⊕, and R d = 3 . 25 ±0 . 11 R ⊕; we characterize their masses using TTVs and precise radial velocities from ESPRESSO and HARPS, and find them to be M b = 18 . 5 + 9 . 1 −7 . 6 M ⊕, M c = 7 . 9 + 4 . 2 −3 . 0 M ⊕, and M d = 5 . 7 + 2 . 7 −2 . 1 M ⊕, making planet b a dense, massive planet while c and d are both underdense. We also demonstrate that the two outer planets are ripe for atmospheric characterization using transmission spectroscopy, especially given their position in the CVZ of James Webb Space Telescope . The data obtained to date are consistent with resonant (librating) and non-resonant (circulating) solutions; additional observations will show whether the pair is actually locked in resonance or just near-resonant. French polar agency IPEV ANR-15-IDEX-01 French polar agency PNRA ANR-15-IDEX-01 Italian polar agency IPEV ANR-15-IDEX-01 Italian polar agency PNRA ANR-15-IDEX-01 NASA Exoplanet Exploration Program NASA's Science Mission Directorate European Organisation for Astronomical Research in the Southern Hemisphere 0102.C-0503(A) National Science Foundation (NSF) European Space Agency European Commission Swiss National Science Foundation (SNSF) ...