Wolf 327b: A new member of the pack of ultra-short-period super-Earths around M dwarfs

DOI: 
10.1051/0004-6361/202348813
Publication date: 
11/04/2024
Main author: 
Murgas, F.
IAA authors: 
Peña-Moñino, L.;Pérez-Torres, M.;Schöfer, P.;Amado, P. J.
Authors: 
Murgas, F.;Pallé, E.;Orell-Miquel, J.;Carleo, I.;Peña-Moñino, L.;Pérez-Torres, M.;Watkins, C. N.;Jeffers, S. V.;Azzaro, M.;Barkaoui, K.;Belinski, A. A.;Caballero, J. A.;Charbonneau, D.;Cheryasov, D. V.;Ciardi, D. R.;Collins, K. A.;Cortés-Contreras, M.;de Leon, J.;Duque-Arribas, C.;Enoc, G.;Esparza-Borges, E.;Fukui, A.;Geraldía-González, S.;Gilbert, E. A.;Hatzes, A. P.;Hayashi, Y.;Henning, Th.;Herrero, E.;Jenkins, J. M.;Lillo-Box, J.;Lodieu, N.;Lund, M. B.;Luque, R.;Montes, D.;Nagel, E.;Narita, N.;Parviainen, H.;Polanski, A. S.;Reffert, S.;Schlecker, M.;Schöfer, P.;Schwarz, R. P.;Schweitzer, A.;Seager, S.;Stassun, K. G.;Tabernero, H. M.;Terada, Y.;Twicken, J. D.;Vanaverbeke, S.;Winn, J. N.;Zambelli, R.;Amado, P. J.;Quirrenbach, A.;Reiners, A.;Ribas, I.
Journal: 
Astronomy and Astrophysics
Publication type: 
Article
Volume: 
684
Pages: 
A83
Abstract: 
Planets with orbital periods shorter than 1 day are rare and have formation histories that are not completely understood. Small (R<SUB>p</SUB> &lt; 2 R<SUB>⊕</SUB>) ultra-short-period (USP) planets are highly irradiated, probably have rocky compositions with high bulk densities, and are often found in multi-planet systems. Additionally, USP planets found around small stars are excellent candidates for characterization using present-day instrumentation. Of the current full sample of approximately 5500 confirmed exoplanets, only 130 are USP planets and around 40 have mass and radius measurements. Wolf 327 (TOI-5747) is an M dwarf (R<SUB>*</SUB> = 0.406 ± 0.015 R<SUB>⊙</SUB>, M<SUB>*</SUB> = 0.405 ± 0.019 M<SUB>⊙</SUB>, T<SUB>eff</SUB> = 3542 ± 70 K, and V = 13 mag) located at a distance d = 28.5 pc. NASA's planet hunter satellite, TESS, detected transits in this star with a period of 0.573 day (13.7 h) and with a transit depth of 818 ppm. Ground-based follow-up photometry, high resolution imaging, and radial velocity (RV) measurements taken with the CARMENES spectrograph confirm the presence of this new USP planet. Wolf 327b is a super-Earth with a radius of R<SUB>p</SUB> = 1.24 ± 0.06 R<SUB>⊕</SUB> and a mass of M<SUB>p</SUB> = 2.53 ± 0.46 M<SUB>⊕</SUB>, yielding a bulk density of 7.24 ± 1.66 g cm<SUP>−3</SUP> and thus suggesting a rocky composition. Owing to its close proximity to its host star (a = 0.01 au), Wolf 327b has an equilibrium temperature of 996 ± 22 K. This planet has a mass and radius similar to K2-229b, a planet with an inferred Mercury-like internal composition. Planet interior models suggest that Wolf 327b has a large iron core, a small rocky mantle, and a negligible (if any) H/He atmosphere. <P />Radial velocity measurement table is available at the CDS via anonymous ftp to <A href="https://cdsarc.cds.unistra.fr/">cdsarc.cds.unistra.fr</A> (ftp://130.79.128.5) or via <A href="https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/684/A83">https://cdsarc.cds.unistra.fr/viz-bin/cat/J/A+A/684/A83</A>
Database: 
ADS
SCOPUS
URL: 
https://ui.adsabs.harvard.edu/#abs/2024A&A...684A..83M/abstract
ADS Bibcode: 
2024A&A...684A..83M
Keywords: 
techniques: photometric;techniques: radial velocities;planets and satellites: detection;planets and satellites: terrestrial planets;stars: individual: Wolf 327;stars: late-type;Astrophysics - Earth and Planetary Astrophysics;Astrophysics - Solar and Stellar Astrophysics