Discovery and mass measurement of the hot, transiting, Earth-sized planet, GJ 3929 b
We report the discovery of GJ 3929 b, a hot Earth-sized planet orbiting the nearby M3.5 V dwarf star, GJ 3929 (G 180-18, TOI-2013). Joint modelling of photometric observations from TESS sectors 24 and 25 together with 73 spectroscopic observations from CARMENES and follow-up transit observations fro...
Saved in:
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
|---|---|
| Format: | Article (Journal) |
| Language: | English |
| Published: |
02 March 2022
|
| In: |
Astronomy and astrophysics
Year: 2022, Volume: 659, Pages: 1-23 |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/202142653 |
| Online Access: | Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1051/0004-6361/202142653 Verlag, lizenzpflichtig, Volltext: https://www.aanda.org/articles/aa/abs/2022/03/aa42653-21/aa42653-21.html |
| Author Notes: | J. Kemmer, S. Dreizler, D. Kossakowski, S. Stock, A. Quirrenbach, J.A. Caballero, P.J. Amado, K.A. Collins, N. Espinoza, E. Herrero, J.M. Jenkins, D.W. Latham, J. Lillo-Box, N. Narita, E. Pallé, A. Reiners, I. Ribas, G. Ricker, E. Rodríguez, S. Seager, R. Vanderspek, R. Wells, J. Winn, F.J. Aceituno, V.J.S. Béjar, T. Barclay, P. Bluhm, P. Chaturvedi, C. Cifuentes, K.I. Collins, M. Cortés-Contreras, B.-O. Demory, M.M. Fausnaugh, A. Fukui, Y. Gómez Maqueo Chew, D. Galadí-Enríquez, T. Gan, M. Gillon, A. Golovin, A.P. Hatzes, Th. Henning, C. Huang, S.V. Jeffers, A. Kaminski, M. Kunimoto, M. Kürster, M. J. López-González, M. Lafarga, R. Luque, J. McCormac, K. Molaverdikhani, D. Montes, J.C. Morales, V. M. Passegger, S. Reffert, L. Sabin, P. Schöfer, N. Schanche, M. Schlecker, U. Schroffenegger, R.P. Schwarz, A. Schweitzer, A. Sota, P. Tenenbaum, T. Trifonov, S. Vanaverbeke, and M. Zechmeister |
| Summary: | We report the discovery of GJ 3929 b, a hot Earth-sized planet orbiting the nearby M3.5 V dwarf star, GJ 3929 (G 180-18, TOI-2013). Joint modelling of photometric observations from TESS sectors 24 and 25 together with 73 spectroscopic observations from CARMENES and follow-up transit observations from SAINT-EX, LCOGT, and OSN yields a planet radius of <i>R<i/><sub>b<sub/> = 1.150 ± 0.040 <i>R<i/><sub>⊕<sub/>, a mass of <i>M<i/><sub>b<sub/> = 1.21 ± 0.42 <i>M<i/><sub>⊕<sub/>, and an orbital period of <i>P<i/><sub>b<sub/> = 2.6162745 ± 0.0000030 <i>d<i/>. The resulting density of <i>ρ<i/><sub>b<sub/> = 4.4 ± 1.6 g cm<sup>−3<sup/> is compatible with the Earth’s mean density of about 5.5 g cm<sup>−3<sup/>. Due to the apparent brightness of the host star (<i>J<i/> = 8.7 mag) and its small size, GJ 3929 b is a promising target for atmospheric characterisation with the JWST. Additionally, the radial velocity data show evidence for another planet candidate with <i>P<i/><sub>[c]<sub/> = 14.303 ± 0.035 d, which is likely unrelated to the stellar rotation period, <i>P<i/><sub>rot<sub/> = 122 ± 13 d, which we determined from archival HATNet and ASAS-SN photometry combined with newly obtained TJO data. |
|---|---|
| Item Description: | Gesehen am 08.04.2022 |
| Physical Description: | Online Resource |
| ISSN: | 1432-0746 |
| DOI: | 10.1051/0004-6361/202142653 |