TOI-561 b: A Low-density Ultra-short-period "Rocky" Planet around a Metal-poor Star

被引:21
|
作者
Brinkman, Casey L. [1 ]
Weiss, Lauren M. [2 ]
Dai, Fei [3 ]
Huber, Daniel [1 ]
Kite, Edwin S. [4 ]
Valencia, Diana [5 ,11 ]
Bean, Jacob L. [6 ]
Beard, Corey [7 ]
Behmard, Aida [8 ]
Blunt, Sarah [8 ]
Brady, Madison [6 ]
Fulton, Benjamin [9 ]
Giacalone, Steven [10 ]
Howard, Andrew W. [8 ]
Isaacson, Howard [10 ]
Kasper, David [6 ]
Lubin, Jack [7 ]
MacDougall, Mason
Murphy, Joseph Akana M.
Plotnykov, Mykhaylo [5 ,11 ]
Polanski, Alex S.
Rice, Malena
Seifahrt, Andreas [6 ]
Stefansson, Guomundur
Stuermer, Julian
机构
[1] Univ Hawaii, Inst Astron, 2680 Woodlawn Dr, Honolulu, HI 96822 USA
[2] Univ Notre Dame, Dept Phys & Astron, Notre Dame, IN 46556 USA
[3] Div Geol & Planetary Sci, 1200 E Calif Blvd, Pasadena, CA 91125 USA
[4] Univ Chicago, Dept Geophys Sci, Chicago, IL 60637 USA
[5] Univ Toronto, Ctr Planetary Sci, 1265 Mil Trail, Toronto, ON M1C 1A4, Canada
[6] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
[7] Univ Calif Irvine, Dept Phys & Astron, Irvine, CA 92697 USA
[8] CALTECH, Dept Astron, Pasadena, CA 91125 USA
[9] Caltech IPAC, NASA Exoplanet Sci Inst, MC 314-6, 1200 E Calif Blvd, Pasadena, CA 91125 USA
[10] Univ Calif Berkeley, Dept Astron, 501 Campbell Hall, Berkeley, CA 94720 USA
[11] MIT, Kavli Inst Astrophys & Space Res, Cambridge, MA 02139 USA
来源
ASTRONOMICAL JOURNAL | 2023年 / 165卷 / 03期
基金
美国国家航空航天局; 美国国家科学基金会;
关键词
SUPER-EARTH ATMOSPHERES; POWERED MASS-LOSS; RADIUS DISTRIBUTION; KEPLER PLANETS; EXOPLANET; ASTROPY; SYSTEMS; HOT; ASTEROSEISMOLOGY; EVAPORATION;
D O I
10.3847/1538-3881/acad83
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
TOI-561 is a galactic thick-disk star hosting an ultra-short-period (0.45-day-orbit) planet with a radius of 1.37 R (circle plus), making it one of the most metal-poor ([Fe/H] = -0.41) and oldest (approximate to 10 Gyr) sites where an Earth-sized planet has been found. We present new simultaneous radial velocity (RV) measurements from Gemini-N/MAROON-X and Keck/HIRES, which we combined with literature RVs to derive a mass of M ( b ) = 2.24 +/- 0.20 M (circle plus). We also used two new sectors of TESS photometry to improve the radius determination, finding R ( b ) = 1.37 +/- 0.04 R (circle plus) and confirming that TOI-561 b is one of the lowest-density super-Earths measured to date (rho ( b ) = 4.8 +/- 0.5 g cm(-3)). This density is consistent with an iron-poor rocky composition reflective of the host star's iron and rock-building element abundances; however, it is also consistent with a low-density planet with a volatile envelope. The equilibrium temperature of the planet (similar to 2300 K) suggests that this envelope would likely be composed of high mean molecular weight species, such as water vapor, carbon dioxide, or silicate vapor, and is likely not primordial. We also demonstrate that the composition determination is sensitive to the choice of stellar parameters and that further measurements are needed to determine whether TOI-561 b is a bare rocky planet, a rocky planet with an optically thin atmosphere, or a rare example of a nonprimordial envelope on a planet with a radius smaller than 1.5 R (circle plus).
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页数:15
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