| ŠUBJAK, J., M. ENDL, P. CHATURVEDI, R. KARJALAINEN, W. D. COCHRAN, M. ESPOSITO, D. GANDOLFI, K. W. F. LAM, K. STASSUN, Jiří ŽÁK, N. LODIEU, H. M. J. BOFFIN, P. J. MACQUEEN, A. HATZES, E. W. GUENTHER, I. GEORGIEVA, S. GRZIWA, H. SCHMERLING, Marek SKARKA, Martin BLAŽEK, Marie KARJALAINEN, Magdalena ŠPOKOVÁ, H. ISAACSON, A. W. HOWARD, C. J. BURKE, V. Van EYLEN, B. FALK, M. FRIDLUND, E. GOFFO, J. M. JENKINS, J. KORTH, J. J. LISSAUER, J. H. LIVINGSTON, R. LUQUE, A. MURESAN, H. P. OSBORN, E. PALLÉ, C. M. PERSSON, S. REDFIELD, G. R. RICKER, S. SEAGER, L. M. SERRANO, A. M. S. SMITH a Petr KABÁTH. TOI-1268b: The youngest hot Saturn-mass transiting exoplanet. Astronomy & Astrophysics. EDP Sciences, 2022, roč. 662, June, s. 1-21. ISSN 0004-6361. Dostupné z: https://dx.doi.org/10.1051/0004-6361/202142883. |
Další formáty:
BibTeX
LaTeX
RIS
@article{1840478,
author = {Šubjak, J. and Endl, M. and Chaturvedi, P. and Karjalainen, R. and Cochran, W. D. and Esposito, M. and Gandolfi, D. and Lam, K. W. F. and Stassun, K. and Žák, Jiří and Lodieu, N. and Boffin, H. M. J. and MacQueen, P. J. and Hatzes, A. and Guenther, E. W. and Georgieva, I. and Grziwa, S. and Schmerling, H. and Skarka, Marek and Blažek, Martin and Karjalainen, Marie and Špoková, Magdalena and Isaacson, H. and Howard, A. W. and Burke, C. J. and Eylen, V. Van and Falk, B. and Fridlund, M. and Goffo, E. and Jenkins, J. M. and Korth, J. and Lissauer, J. J. and Livingston, J. H. and Luque, R. and Muresan, A. and Osborn, H. P. and Pallé, E. and Persson, C. M. and Redfield, S. and Ricker, G. R. and Seager, S. and Serrano, L. M. and Smith, A. M. S. and Kabáth, Petr},
article_number = {June},
doi = {http://dx.doi.org/10.1051/0004-6361/202142883},
keywords = {techniques: spectroscopic; techniques: radial velocities; techniques: photometric; planetary systems; planets and satellites: gaseous planets; planets and satellites: atmospheres},
language = {eng},
issn = {0004-6361},
journal = {Astronomy & Astrophysics},
title = {TOI-1268b: The youngest hot Saturn-mass transiting exoplanet},
url = {https://arxiv.org/abs/2201.13341},
volume = {662},
year = {2022}
}
TY - JOUR
ID - 1840478
AU - Šubjak, J. - Endl, M. - Chaturvedi, P. - Karjalainen, R. - Cochran, W. D. - Esposito, M. - Gandolfi, D. - Lam, K. W. F. - Stassun, K. - Žák, Jiří - Lodieu, N. - Boffin, H. M. J. - MacQueen, P. J. - Hatzes, A. - Guenther, E. W. - Georgieva, I. - Grziwa, S. - Schmerling, H. - Skarka, Marek - Blažek, Martin - Karjalainen, Marie - Špoková, Magdalena - Isaacson, H. - Howard, A. W. - Burke, C. J. - Eylen, V. Van - Falk, B. - Fridlund, M. - Goffo, E. - Jenkins, J. M. - Korth, J. - Lissauer, J. J. - Livingston, J. H. - Luque, R. - Muresan, A. - Osborn, H. P. - Pallé, E. - Persson, C. M. - Redfield, S. - Ricker, G. R. - Seager, S. - Serrano, L. M. - Smith, A. M. S. - Kabáth, Petr
PY - 2022
TI - TOI-1268b: The youngest hot Saturn-mass transiting exoplanet
JF - Astronomy & Astrophysics
VL - 662
IS - June
SP - 1-21
EP - 1-21
PB - EDP Sciences
SN - 00046361
KW - techniques: spectroscopic
KW - techniques: radial velocities
KW - techniques: photometric
KW - planetary systems
KW - planets and satellites: gaseous planets
KW - planets and satellites: atmospheres
UR - https://arxiv.org/abs/2201.13341
N2 - We report the discovery of TOI-1268b, a transiting Saturn-mass planet from the TESS space mission. With an age of less than 1 Gyr, derived from various age indicators, TOI-1268b is the youngest Saturn-mass planet known to date; it contributes to the small sample of well-characterised young planets. It has an orbital period of P = 8.1577080 ± 0.0000044 days, and transits an early K-dwarf star with a mass of M* = 0.96 ± 0.04 M⊙, a radius of R* = 0.92 ± 0.06 R⊙, an effective temperature of Teff = 5300 ± 100 K, and a metallicity of 0.36 ± 0.06 dex. By combining TESS photometry with high-resolution spectra acquired with the Tull spectrograph at the McDonald Observatory, and the high-resolution spectrographs at the Tautenburg and Ondřejov Observatories, we measured a planetary mass of Mp = 96.4 ± 8.3 M⊕ and a radius of Rp = 9.1 ± 0.6 R⊕. TOI-1268 is an ideal system for studying the role of star-planet tidal interactions for non-inflated Saturn-mass planets. We used system parameters derived in this paper to constrain the planet’s tidal quality factor to the range of 104.5–5.3. When compared with the sample of other non-inflated Saturn-mass planets, TOI-1268b is one of the best candidates for transmission spectroscopy studies.
ER -
ŠUBJAK, J., M. ENDL, P. CHATURVEDI, R. KARJALAINEN, W. D. COCHRAN, M. ESPOSITO, D. GANDOLFI, K. W. F. LAM, K. STASSUN, Jiří ŽÁK, N. LODIEU, H. M. J. BOFFIN, P. J. MACQUEEN, A. HATZES, E. W. GUENTHER, I. GEORGIEVA, S. GRZIWA, H. SCHMERLING, Marek SKARKA, Martin BLAŽEK, Marie KARJALAINEN, Magdalena ŠPOKOVÁ, H. ISAACSON, A. W. HOWARD, C. J. BURKE, V. Van EYLEN, B. FALK, M. FRIDLUND, E. GOFFO, J. M. JENKINS, J. KORTH, J. J. LISSAUER, J. H. LIVINGSTON, R. LUQUE, A. MURESAN, H. P. OSBORN, E. PALLÉ, C. M. PERSSON, S. REDFIELD, G. R. RICKER, S. SEAGER, L. M. SERRANO, A. M. S. SMITH a Petr KABÁTH. TOI-1268b: The youngest hot Saturn-mass transiting exoplanet. \textit{Astronomy \&{} Astrophysics}. EDP Sciences, 2022, roč.~662, June, s.~1-21. ISSN~0004-6361. Dostupné z: https://dx.doi.org/10.1051/0004-6361/202142883.
|
