2025
Two Earth-size Planets and an Earth-size Candidate Transiting the nearby Star HD 101581
KUNIMOTO, Michelle; Zifan LIN; Sarah MILLHOLLAND; Alexander VENNER; Natalie R HINKEL et al.Základní údaje
Originální název
Two Earth-size Planets and an Earth-size Candidate Transiting the nearby Star HD 101581
Autoři
KUNIMOTO, Michelle; Zifan LIN; Sarah MILLHOLLAND; Alexander VENNER; Natalie R HINKEL; Avi SHPORER; Andrew VANDERBURG; Jeremy BAILEY; Rafael BRAHM; Jennifer A BURT; R Paul BUTLER; Brad CARTER; David R CIARDI; Karen A COLLINS; Kevin I COLLINS; Knicole D COLON; Jeffrey D CRANE; Tansu DAYLAN; Matias R DIAZ; John P DOTY; Fabo FENG; Eike W GUENTHER; Jonathan HORNER; Steve B HOWELL; Jan JANÍK ORCID; Hugh R A JONES; Petr KABATH; Shubham KANODIA; Colin LITTLEFIELD; Hugh P OSBORN; Simon O'TOOLE; Martin PAEGERT; Pavel PINTR; Richard P SCHWARZ; Steve SHECTMAN; Gregor SRDOC; Keivan G STASSUN; Johanna K TESKE; Joseph D TWICKEN; Leonardo VANZI; Sharon X WANG; Robert A WITTENMYER; Jon M JENKINS; George R RICKER; Sara SEAGER a Joshua WINN
Vydání
Astronomical Journal, IOP Publishing Ltd, 2025, 0004-6256
Další údaje
Jazyk
angličtina
Typ výsledku
Článek v odborném periodiku
Obor
10308 Astronomy
Stát vydavatele
Spojené státy
Utajení
není předmětem státního či obchodního tajemství
Odkazy
Impakt faktor
Impact factor: 5.100 v roce 2024
Označené pro přenos do RIV
Ano
Kód RIV
RIV/00216224:14310/25:00140489
Organizační jednotka
Přírodovědecká fakulta
UT WoS
EID Scopus
Klíčová slova anglicky
exoplanets; Earth-size candidate; star HD 101581
Příznaky
Mezinárodní význam, Recenzováno
Změněno: 31. 3. 2025 09:15, Mgr. Marie Novosadová Šípková, DiS.
Anotace
V originále
We report the validation of multiple planets transiting the nearby (d = 12.8 pc) K5V dwarf HD 101581 (GJ 435, TOI-6276, TIC 397362481). This system consists of at least two Earth-size planets whose orbits are near a mutual 4:3 mean-motion resonance, HD 101581 b ( R-p=0.956(-0.061)(+0.063 )R(circle plus) , P = 4.47 days) and HD 101581c ( R-p=0.990(-0.070)(+0.070 )R(circle plus) , P = 6.21 days). Both planets were discovered in Sectors 63 and 64 TESS observations and statistically validated with supporting ground-based follow-up. We also identify a signal that probably originates from a third transiting planet, TOI-6276.03 ( R-p=0.982(-0.098)(+0.114 )R(circle plus), P = 7.87 days). These planets are remarkably uniform in size and their orbits are evenly spaced, representing a prime example of the "peas-in-a-pod" architecture seen in other compact multiplanet systems. At V = 7.77, HD 101581 is the brightest star known to host multiple transiting planets smaller than 1.5 R (circle plus). HD 101581 is a promising system for atmospheric characterization and comparative planetology of small planets.