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

Murgas, F., Pallé, E., Orell-Miquel, J., Carleo, I., Peña-Moñino, L., Pérez-Torres, M., et al. (2024). Wolf 327b: A new member of the pack of ultra-short-period super-Earths around M dwarfs. Astronomy and Astrophysics, 684, A83. doi:10.1051/0004-6361/202348813.

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Murgas, F., Author
Pallé, E., Author
Orell-Miquel, J., Author
Carleo, I., Author
Peña-Moñino, L., Author
Pérez-Torres, M., Author
Watkins, C. N., Author
Jeffers, S. V.1, Author           
Azzaro, M., Author
Barkaoui, K., Author
Belinski, A. A., Author
Caballero, J. A., Author
Charbonneau, D., Author
Cheryasov, D. V., Author
Ciardi, D. R., Author
Collins, K. A., Author
Cortés-Contreras, M., Author
de Leon, J., Author
Duque-Arribas, C., Author
Enoc, G., Author
Esparza-Borges, E., AuthorFukui, A., AuthorGeraldía-González, S., AuthorGilbert, E. A., AuthorHatzes, A. P., AuthorHayashi, Y., AuthorHenning, Th., AuthorHerrero, E., AuthorJenkins, J. M., AuthorLillo-Box, J., AuthorLodieu, N., AuthorLund, M. B., AuthorLuque, R., AuthorMontes, D., AuthorNagel, E., AuthorNarita, N., AuthorParviainen, H., AuthorPolanski, A. S., AuthorReffert, S., AuthorSchlecker, M., AuthorSchöfer, P., AuthorSchwarz, R. P., AuthorSchweitzer, A., AuthorSeager, S., AuthorStassun, K. G., AuthorTabernero, H. M., AuthorTerada, Y., AuthorTwicken, J. D., AuthorVanaverbeke, S., AuthorWinn, J. N., AuthorZambelli, R., AuthorAmado, P. J., AuthorQuirrenbach, A., AuthorReiners, A., AuthorRibas, I., Author more..
Affiliations:
1Department Solar and Stellar Interiors, Max Planck Institute for Solar System Research, Max Planck Society, ou_1832287              

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Free 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
 Abstract: Planets with orbital periods shorter than 1 day are rare and have formation histories that are not completely understood. Small (Rp < 2 R) 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* = 0.406 ± 0.015 R, M* = 0.405 ± 0.019 M, Teff = 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 Rp = 1.24 ± 0.06 R and a mass of Mp = 2.53 ± 0.46 M, yielding a bulk density of 7.24 ± 1.66 g cm−3 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>

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 Dates: 2024
 Publication Status: Issued
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 Rev. Type: -
 Identifiers: DOI: 10.1051/0004-6361/202348813
ISSN: 0004-6361
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Title: Astronomy and Astrophysics
Source Genre: Journal
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Pages: - Volume / Issue: 684 Sequence Number: - Start / End Page: A83 Identifier: -