Serrano, LM, Gandolfi, D, Hoyer, S, Brandeker, A, Hooton, MJ, Sousa, S, Murgas, F, Ciardi, DR, Howell, SB, Benz, W, Billot, N, Floren, H-G, Bekkelien, A, Bonfanti, A, Krenn, A, Mustill, AJ, Wilson, TG, Osborn, H, Parviainen, H, Heidari, N, Palle, E, Fridlund, M, Adibekyan, V, Fossati, L, Deleuil, M, Knudstrup, E, Collins, KA, Lam, KWF, Grziwa, S, Salmon, S, Albrecht, SH, Alibert, Y, Alonso, R, Anglada-Escude, G, Barczy, T, Barrado y Navascues, D, Barros, SCC, Baumjohann, W, Beck, M, Beck, T, Bieryla, A, Bonfils, X, Boyd, PT, Broeg, C, Cabrera, J, Charnoz, S, Chazelas, B, Christiansen, JL, Cameron, AC, Cortes-Zuleta, P, Csizmadia, S, Davies, MB, Deline, A, Delrez, L, Demangeon, ODS, Demory, B-O, Dunlavey, A, Ehrenreich, D, Erikson, A, Fortier, A, Fukui, A, Garai, Z, Gillon, M, Gudel, M, Hebrard, G, Heng, K, Huang, CX, Isaak, KG, Jenkins, JM, Kiss, LL, Laskar, J, Latham, DW, des Etangs, AL, Lendl, M, Levine, AM, Lovis, C, Lund, MB, Magrin, D, Maxted, PFL, Narita, N, Nascimbeni, V, Olofsson, G, Ottensamer, R, Pagano, I, Pessanha, ACSV, Peter, G, Piotto, G, Pollacco, D, Queloz, D, Ragazzoni, R, Rando, N, Ratti, F, Rauer, H, Ribas, I, Ricker, G, Rowden, P, Santos, NC, Scandariato, G, Seager, S, Segransan, D, Simon, AE, Smith, AMS, Steller, M, Szabo, GM, Thomas, N, Twicken, JD, Udry, S, Ulmer, B, Van Grootel, V, Vanderspek, R, Viotto, V and Walton, N (2022) The HD 93963 A transiting system: A 1.04d super-Earth and a 3.65 d sub-Neptune discovered by TESS and CHEOPS. ASTRONOMY & ASTROPHYSICS, 667. ISSN 0004-6361

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Abstract

We present the discovery of two small planets transiting HD 93963A (TOI-1797), a GOV star (M* = 1.109 ± 0.043M⊙, R* = 1.043 ± 0.009 R⊙) in a visual binary system. We combined TESS and CHEOPS space-borne photometry with MuSCAT 2 ground-based photometry, ‘Alopeke and PHARO high-resolution imaging, TRES and FIES reconnaissance spectroscopy, and SOPHIE radial velocity measurements. We validated and spectroscopically confirmed the outer transiting planet HD 93963 A c, a sub-Neptune with an orbital period of Pc ≈ 3.65 d that was reported to be a TESS object of interest (TOI) shortly after the release of Sector 22 data. HD 93963 A c has amass of Mc = 19.2 ± 4.1 M⊕ and a radius of Rc = 3.228 ± 0.059 R⊕, implying a mean density of ρc = 3.1 ± 0.7 g cm-3. The inner object, HD 93963 A b, is a validated 1.04 d ultra-short period (USP) transiting super-Earth that we discovered in the TESS light curve and that was not listed as a TOI, owing to the low significance of its signal (TESS signal-to-noise ratio ≈6.7, TESS + CHEOPS combined transit depth Db = 141.5−8.3+8.5 ppm). We intensively monitored the star with CHEOPS by performing nine transit observations to confirm the presence of the inner planet and validate the system. HD 93963 A b is the first small (Rb = 1.35 ± 0.042 R⊕) USP planet discovered and validated by TESS and CHEOPS. Unlike planet c, HD 93963 Ab is not significantly detected in our radial velocities (Mb = 7.8 ± 3.2 M⊕). The two planets are on either side of the radius valley, implying that they could have undergone completely different evolution processes. We also discovered a linear trend in our Doppler measurements, suggesting the possible presence of a long-period outer planet. With a V-band magnitude of 9.2, HD 93963 A is among the brightest stars known to host a USP planet, making it one of the most favourable targets for precise mass measurement via Doppler spectroscopy and an important laboratory to test formation, evolution, and migration models of planetary systems hosting ultra-short period planets.

Item Type: Article
Additional Information: Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. This article is published in open access under the Subscribe-to-Open model. Subscribe to A&A to support open access publication.
Subjects: Q Science > Q Science (General)
Q Science > QB Astronomy
Q Science > QB Astronomy > QB460 Astrophysics
Q Science > QC Physics
Divisions: Faculty of Natural Sciences > School of Chemical and Physical Sciences
Related URLs:
Depositing User: Symplectic
Date Deposited: 07 Dec 2022 15:27
Last Modified: 07 Dec 2022 15:27
URI: https://eprints.keele.ac.uk/id/eprint/11771

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