The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf
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BARRAGÁN, O.; D. J. ARMSTRONG; D. GANDOLFI; I. CARLEO; A. A. VIDOTTO; C. D’ANGELO VILLARREAL; A. OKLOPČIĆ; H. ISAACSON; D. ODDO; K. COLLINS; M. FRIDLUND; S. G. SOUSA; C. M. PERSSON; C. HELLIER; S. HOWELL; A. HOWARD; S. REDFIELD; N. EISNER; I. Y. GEORGIEVA; D. DRAGOMIR; D. BAYLISS; L. D. NIELSEN; B. KLEIN; S. AIGRAIN; M. ZHANG; J. TESKE; J. D. TWICKEN; J. JENKINS; M. ESPOSITO; V. VAN EYLEN; F. RODLER; V. ADIBEKYAN; J. ALARCON; D. R. ANDERSON; J. M. AKANA MURPHY; D. BARRADO; S. C. C. BARROS; B. BENNEKE; F. BOUCHY; E. M. BRYANT; R. P. BUTLER; J. BURT; J. CABRERA; S. CASEWELL; P. CHATURVEDI; R. CLOUTIER; W. D. COCHRAN; J. CRANE; I. CROSSFIELD; N. CROUZET; K. I. COLLINS; F. DAI; H. J. DEEG; A. DELINE; O. D. S. DEMANGEON; X. DUMUSQUE; P. FIGUEIRA; E. FURLAN; C. GNILKA; M. R. GOAD; E. GOFFO; F. GUTIÉRREZ-CANALES; A. HADJIGEORGHIOU; Z. HARTMAN; A. P. HATZES; M. HARRIS; B. HENDERSON; T. HIRANO; S. HOJJATPANAH; S. HOYER; P. KABÁTH; J. KORTH; J. LILLO-BOX; R. LUQUE; M. MARMIER; T. MOČNIK; A. MURESAN; F. MURGAS; E. NAGEL; H. L. M. OSBORNE; A. OSBORN; H. P. OSBORN; E. PALLE; M. RAIMBAULT; G. R. RICKER; R. A. RUBENZAHL; C. STOCKDALE; N. C. SANTOS; N. SCOTT; R. P. SCHWARZ; S. SHECTMAN; M. RAIMBAULT; S. SEAGER; D. SÉGRANSAN; L. M. SERRANO; Marek SKARKA; A. M. S. SMITH; J. ŠUBJAK; T. G. TAN; S. UDRY; C. WATSON; P. J. WHEATLEY; R. WEST; J. N. WINN; S. X. WANG; A. WOLFGANG a C. ZIEGLER
Vydání
Monthly Notices of the Royal Astronomical Society, Oxford University Press, 2022, 0035-8711
We present the discovery and characterization of two transiting planets observed by TESS in the light curves of the young and bright (V = 9.67) star HD73583 (TOI-560). We perform an intensive spectroscopic and photometric space- and ground-based follow-up in order to confirm and characterize the system. We found that HD73583 is a young (similar to 500 Myr) active star with a rotational period of 12.08 +/- 0.11 d, and a mass and radius of 0.73 +/- 0.02 M-circle dot and 0.65 +/- 0.02 R-circle dot, respectively. HD 73583 b (P-b = 6.3980420(-0.0000062)(+0.0000067 )d) has a mass and radius of 10.2(-3.1)(+3.4) M-circle plus and 2.79 +/- 0.10 R-circle plus, respectively, which gives a density of 2.58(-0.81)(+0.95) g cm(-3). HD 73583 c (P-c = 18.87974(-0.00074)(+0.00086) d) has a mass and radius of 9.7(-1.7)(+1.8) M-circle plus and 2.39(-0.09)(+0.10) R-circle plus, respectively, which translates to a density of 3.88(-0.80)(+0.91) g cm(-3). Both planets are consistent with worlds made of a solid core surrounded by a volatile envelope. Because of their youth and host star brightness, they both are excellent candidates to perform transmission spectroscopy studies. We expect ongoing atmospheric mass-loss for both planets caused by stellar irradiation. We estimate that the detection of evaporating signatures on H and He would be challenging, but doable with present and future instruments.
BARRAGÁN, O.; D. J. ARMSTRONG; D. GANDOLFI; I. CARLEO; A. A. VIDOTTO; C. D’ANGELO VILLARREAL; A. OKLOPČIĆ; H. ISAACSON; D. ODDO; K. COLLINS; M. FRIDLUND; S. G. SOUSA; C. M. PERSSON; C. HELLIER; S. HOWELL; A. HOWARD; S. REDFIELD; N. EISNER; I. Y. GEORGIEVA; D. DRAGOMIR; D. BAYLISS; L. D. NIELSEN; B. KLEIN; S. AIGRAIN; M. ZHANG; J. TESKE; J. D. TWICKEN; J. JENKINS; M. ESPOSITO; V. VAN EYLEN; F. RODLER; V. ADIBEKYAN; J. ALARCON; D. R. ANDERSON; J. M. AKANA MURPHY; D. BARRADO; S. C. C. BARROS; B. BENNEKE; F. BOUCHY; E. M. BRYANT; R. P. BUTLER; J. BURT; J. CABRERA; S. CASEWELL; P. CHATURVEDI; R. CLOUTIER; W. D. COCHRAN; J. CRANE; I. CROSSFIELD; N. CROUZET; K. I. COLLINS; F. DAI; H. J. DEEG; A. DELINE; O. D. S. DEMANGEON; X. DUMUSQUE; P. FIGUEIRA; E. FURLAN; C. GNILKA; M. R. GOAD; E. GOFFO; F. GUTIÉRREZ-CANALES; A. HADJIGEORGHIOU; Z. HARTMAN; A. P. HATZES; M. HARRIS; B. HENDERSON; T. HIRANO; S. HOJJATPANAH; S. HOYER; P. KABÁTH; J. KORTH; J. LILLO-BOX; R. LUQUE; M. MARMIER; T. MOČNIK; A. MURESAN; F. MURGAS; E. NAGEL; H. L. M. OSBORNE; A. OSBORN; H. P. OSBORN; E. PALLE; M. RAIMBAULT; G. R. RICKER; R. A. RUBENZAHL; C. STOCKDALE; N. C. SANTOS; N. SCOTT; R. P. SCHWARZ; S. SHECTMAN; M. RAIMBAULT; S. SEAGER; D. SÉGRANSAN; L. M. SERRANO; Marek SKARKA; A. M. S. SMITH; J. ŠUBJAK; T. G. TAN; S. UDRY; C. WATSON; P. J. WHEATLEY; R. WEST; J. N. WINN; S. X. WANG; A. WOLFGANG a C. ZIEGLER. The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf. Monthly Notices of the Royal Astronomical Society. Oxford University Press, 2022, roč. 514, č. 2, s. 1606-1627. ISSN 0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stac638.
@article{1862938, author = {Barragán, O. and Armstrong, D. J. and Gandolfi, D. and Carleo, I. and Vidotto, A. A. and D’Angelo Villarreal, C. and Oklopčić, A. and Isaacson, H. and Oddo, D. and Collins, K. and Fridlund, M. and Sousa, S. G. and Persson, C. M. and Hellier, C. and Howell, S. and Howard, A. and Redfield, S. and Eisner, N. and Georgieva, I. Y. and Dragomir, D. and Bayliss, D. and Nielsen, L. D. and Klein, B. and Aigrain, S. and Zhang, M. and Teske, J. and Twicken, J. D. and Jenkins, J. and Esposito, M. and Van Eylen, V. and Rodler, F. and Adibekyan, V. and Alarcon, J. and Anderson, D. R. and Akana Murphy, J. M. and Barrado, D. and Barros, S. C. C. and Benneke, B. and Bouchy, F. and Bryant, E. M. and Butler, R. P. and Burt, J. and Cabrera, J. and Casewell, S. and Chaturvedi, P. and Cloutier, R. and Cochran, W. D. and Crane, J. and Crossfield, I. and Crouzet, N. and Collins, K. I. and Dai, F. and Deeg, H. J. and Deline, A. and Demangeon, O. D. S. and Dumusque, X. and Figueira, P. and Furlan, E. and Gnilka, C. and Goad, M. R. and Goffo, E. and GutiérrezandCanales, F. and Hadjigeorghiou, A. and Hartman, Z. and Hatzes, A. P. and Harris, M. and Henderson, B. and Hirano, T. and Hojjatpanah, S. and Hoyer, S. and Kabáth, P. and Korth, J. and LilloandBox, J. and Luque, R. and Marmier, M. and Močnik, T. and Muresan, A. and Murgas, F. and Nagel, E. and Osborne, H. L. M. and Osborn, A. and Osborn, H. P. and Palle, E. and Raimbault, M. and Ricker, G. R. and Rubenzahl, R. A. and Stockdale, C. and Santos, N. C. and Scott, N. and Schwarz, R. P. and Shectman, S. and Raimbault, M. and Seager, S. and Ségransan, D. and Serrano, L. M. and Skarka, Marek and Smith, A. M. S. and Šubjak, J. and Tan, T. G. and Udry, S. and Watson, C. and Wheatley, P. J. and West, R. and Winn, J. N. and Wang, S. X. and Wolfgang, A. and Ziegler, C.}, article_number = {2}, doi = {https://doi.org/10.1093/mnras/stac638}, keywords = {techniques: photometric; techniques: radial velocities; planets and satellites: individual: HD 73583 (TOI-560); stars: activity}, language = {eng}, issn = {0035-8711}, journal = {Monthly Notices of the Royal Astronomical Society}, title = {The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf}, url = {https://academic.oup.com/mnras/article/514/2/1606/6548902}, volume = {514}, year = {2022} }
TY - JOUR ID - 1862938 AU - Barragán, O. - Armstrong, D. J. - Gandolfi, D. - Carleo, I. - Vidotto, A. A. - D’Angelo Villarreal, C. - Oklopčić, A. - Isaacson, H. - Oddo, D. - Collins, K. - Fridlund, M. - Sousa, S. G. - Persson, C. M. - Hellier, C. - Howell, S. - Howard, A. - Redfield, S. - Eisner, N. - Georgieva, I. Y. - Dragomir, D. - Bayliss, D. - Nielsen, L. D. - Klein, B. - Aigrain, S. - Zhang, M. - Teske, J. - Twicken, J. D. - Jenkins, J. - Esposito, M. - Van Eylen, V. - Rodler, F. - Adibekyan, V. - Alarcon, J. - Anderson, D. R. - Akana Murphy, J. M. - Barrado, D. - Barros, S. C. C. - Benneke, B. - Bouchy, F. - Bryant, E. M. - Butler, R. P. - Burt, J. - Cabrera, J. - Casewell, S. - Chaturvedi, P. - Cloutier, R. - Cochran, W. D. - Crane, J. - Crossfield, I. - Crouzet, N. - Collins, K. I. - Dai, F. - Deeg, H. J. - Deline, A. - Demangeon, O. D. S. - Dumusque, X. - Figueira, P. - Furlan, E. - Gnilka, C. - Goad, M. R. - Goffo, E. - Gutiérrez-Canales, F. - Hadjigeorghiou, A. - Hartman, Z. - Hatzes, A. P. - Harris, M. - Henderson, B. - Hirano, T. - Hojjatpanah, S. - Hoyer, S. - Kabáth, P. - Korth, J. - Lillo-Box, J. - Luque, R. - Marmier, M. - Močnik, T. - Muresan, A. - Murgas, F. - Nagel, E. - Osborne, H. L. M. - Osborn, A. - Osborn, H. P. - Palle, E. - Raimbault, M. - Ricker, G. R. - Rubenzahl, R. A. - Stockdale, C. - Santos, N. C. - Scott, N. - Schwarz, R. P. - Shectman, S. - Raimbault, M. - Seager, S. - Ségransan, D. - Serrano, L. M. - Skarka, Marek - Smith, A. M. S. - Šubjak, J. - Tan, T. G. - Udry, S. - Watson, C. - Wheatley, P. J. - West, R. - Winn, J. N. - Wang, S. X. - Wolfgang, A. - Ziegler, C. PY - 2022 TI - The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf JF - Monthly Notices of the Royal Astronomical Society VL - 514 IS - 2 SP - 1606-1627 EP - 1606-1627 PB - Oxford University Press SN - 00358711 KW - techniques: photometric KW - techniques: radial velocities KW - planets and satellites: individual: HD 73583 (TOI-560) KW - stars: activity UR - https://academic.oup.com/mnras/article/514/2/1606/6548902 N2 - We present the discovery and characterization of two transiting planets observed by TESS in the light curves of the young and bright (V = 9.67) star HD73583 (TOI-560). We perform an intensive spectroscopic and photometric space- and ground-based follow-up in order to confirm and characterize the system. We found that HD73583 is a young (similar to 500 Myr) active star with a rotational period of 12.08 +/- 0.11 d, and a mass and radius of 0.73 +/- 0.02 M-circle dot and 0.65 +/- 0.02 R-circle dot, respectively. HD 73583 b (P-b = 6.3980420(-0.0000062)(+0.0000067 )d) has a mass and radius of 10.2(-3.1)(+3.4) M-circle plus and 2.79 +/- 0.10 R-circle plus, respectively, which gives a density of 2.58(-0.81)(+0.95) g cm(-3). HD 73583 c (P-c = 18.87974(-0.00074)(+0.00086) d) has a mass and radius of 9.7(-1.7)(+1.8) M-circle plus and 2.39(-0.09)(+0.10) R-circle plus, respectively, which translates to a density of 3.88(-0.80)(+0.91) g cm(-3). Both planets are consistent with worlds made of a solid core surrounded by a volatile envelope. Because of their youth and host star brightness, they both are excellent candidates to perform transmission spectroscopy studies. We expect ongoing atmospheric mass-loss for both planets caused by stellar irradiation. We estimate that the detection of evaporating signatures on H and He would be challenging, but doable with present and future instruments. ER -
BARRAGÁN, O.; D. J. ARMSTRONG; D. GANDOLFI; I. CARLEO; A. A. VIDOTTO; C. D’ANGELO VILLARREAL; A. OKLOPČI$\backslash$'C; H. ISAACSON; D. ODDO; K. COLLINS; M. FRIDLUND; S. G. SOUSA; C. M. PERSSON; C. HELLIER; S. HOWELL; A. HOWARD; S. REDFIELD; N. EISNER; I. Y. GEORGIEVA; D. DRAGOMIR; D. BAYLISS; L. D. NIELSEN; B. KLEIN; S. AIGRAIN; M. ZHANG; J. TESKE; J. D. TWICKEN; J. JENKINS; M. ESPOSITO; V. VAN EYLEN; F. RODLER; V. ADIBEKYAN; J. ALARCON; D. R. ANDERSON; J. M. AKANA MURPHY; D. BARRADO; S. C. C. BARROS; B. BENNEKE; F. BOUCHY; E. M. BRYANT; R. P. BUTLER; J. BURT; J. CABRERA; S. CASEWELL; P. CHATURVEDI; R. CLOUTIER; W. D. COCHRAN; J. CRANE; I. CROSSFIELD; N. CROUZET; K. I. COLLINS; F. DAI; H. J. DEEG; A. DELINE; O. D. S. DEMANGEON; X. DUMUSQUE; P. FIGUEIRA; E. FURLAN; C. GNILKA; M. R. GOAD; E. GOFFO; F. GUTIÉRREZ-CANALES; A. HADJIGEORGHIOU; Z. HARTMAN; A. P. HATZES; M. HARRIS; B. HENDERSON; T. HIRANO; S. HOJJATPANAH; S. HOYER; P. KABÁTH; J. KORTH; J. LILLO-BOX; R. LUQUE; M. MARMIER; T. MOČNIK; A. MURESAN; F. MURGAS; E. NAGEL; H. L. M. OSBORNE; A. OSBORN; H. P. OSBORN; E. PALLE; M. RAIMBAULT; G. R. RICKER; R. A. RUBENZAHL; C. STOCKDALE; N. C. SANTOS; N. SCOTT; R. P. SCHWARZ; S. SHECTMAN; M. RAIMBAULT; S. SEAGER; D. SÉGRANSAN; L. M. SERRANO; Marek SKARKA; A. M. S. SMITH; J. ŠUBJAK; T. G. TAN; S. UDRY; C. WATSON; P. J. WHEATLEY; R. WEST; J. N. WINN; S. X. WANG; A. WOLFGANG a C. ZIEGLER. The young HD 73583 (TOI-560) planetary system: two 10-M⊕ mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf. \textit{Monthly Notices of the Royal Astronomical Society}. Oxford University Press, 2022, roč.~514, č.~2, s.~1606-1627. ISSN~0035-8711. Dostupné z: https://doi.org/10.1093/mnras/stac638.