J/AJ/165/88       Radial velocity follow up of TOI-561 b       (Brinkman+, 2023)

TOI-561 b; A Low-density Ultra-short-period "Rocky" Planet around a Metal-poor Star Brinkman C.L., Weiss L.M., Dai F., Huber D., Kite E.S., Valencia D., Bean J.L., Beard C., Behmard A., Blunt S., Brady M., Fulton B., Giacalone S., Howard A.W., Isaacson H., Kasper D., Lubin J., MacDougall M., Akana Murphy J.M., Plotnykov M., Polanski A.S., Rice M., Seifahrt A., Stefansson G., Sturmer J. <Astron. J., 165, 88 (2023)> =2023AJ....165...88B 2023AJ....165...88B
ADC_Keywords: Exoplanets; Stars, metal-deficient; Spectra, optical; Radial velocities Keywords: Exoplanets ; Extrasolar rocky planets ; Super Earths ; Exoplanet surface composition ; Exoplanet atmospheric composition Abstract: TOI-561 is a galactic thick-disk star hosting an ultra-short-period (0.45-day-orbit) planet with a radius of 1.37R⊕, making it one of the most metal-poor ([Fe/H]=-0.41) and oldest ({∼10Gyr) sites where an Earth-sized planet has been found. We present new simultaneous radial velocity (RVel) measurements from Gemini-N/MAROON-X and Keck/HIRES, which we combined with literature RVels to derive a mass of Mb=2.24±0.20M⊕. We also used two new sectors of TESS photometry to improve the radius determination, finding Rb=1.37±0.04R⊕ and confirming that TOI-561b is one of the lowest-density super-Earths measured to date (ρb=4.8±0.5g/cm3). 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 ({∼2300K) 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-561b 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 1.5R⊕. Description: Our analysis incorporates 102 total radial velocities (RVels) from the High Resolution Echelle Spectrograph (HIRES) on the W.M. Keck Observatory 10m telescope Keck I on Maunakea, Hawaii. Our analysis also incorporates 143 published RVels from the HARPS-N spectrograph installed on the 3.6m Telescopio Nazionale Galileo (TNG) at the Observatorio Roque de Los Muchachos in La Palma, Spain. MAROON-X is a new, state-of-the-art fiber-fed spectrograph mounted on the 8.1m Gemini North telescope on Maunakea, Hawaii. It operates in the red-optical (500-920nm) with resolving power R∼85000 and uses both red and blue arms to get two RVel measurements per exposure. Objects: ------------------------------------------------------------------- RA (2000) DE Designation(s) (Period) ------------------------------------------------------------------- 09 52 44.54 +06 12 58.9 TOI-561 = TIC 377064495 (P=0.4465690d) ------------------------------------------------------------------- File Summary: -------------------------------------------------------------------------------- FileName Lrecl Records Explanations -------------------------------------------------------------------------------- ReadMe 80 . This file table3.dat 37 316 Radial velocities -------------------------------------------------------------------------------- See also: J/ApJS/210/20 : Small Kepler planets radial velocities (Marcy+, 2014) J/ApJ/800/135 : HARPS-N radial velocities of KOI-69 (Dressing+, 2015) J/ApJ/822/86 : False positive probabilities Q1-Q17 DR24 KOIs (Morton+, 2016) J/AJ/154/109 : California-Kepler Survey. III. Planet radii (Fulton+, 2017) J/ApJ/844/102 : KICstar parallaxes from asteroseismology vs Gaia (Huber+, 2017) J/AJ/153/136 : Planets and host stars with Gaia parallaxes (Stassun+, 2017) J/A+A/653/A41 : L 98-59 (TOI-175) ESPRESSO observations (Demangeon+, 2021) J/AJ/161/56 : The TESS-Keck Survey. II. RVs of TOI-561 (Weiss+, 2021) J/AJ/162/55 : 65 Transit-timing variation planets properties (Yee+, 2021) J/MNRAS/511/4551 : TOI-561 CHEOPS light curves (Lacedelli+, 2022) J/AJ/163/168 : Photometry and radial velocity of LTT 1445A (Winters+, 2022) Byte-by-byte Description of file: table3.dat -------------------------------------------------------------------------------- Bytes Format Units Label Explanations -------------------------------------------------------------------------------- 1- 11 F11.3 d BJD [2458599/2459650] Barycentric Julian Date 13- 18 F6.2 m/s RVel [-12.4/12.6] Radial velocity 20- 23 F4.2 m/s e_RVel [0.6/6] Uncertainty in RVel 25- 37 A13 --- Inst Spectrograph; HARPS, HIRES, or MAROON -------------------------------------------------------------------------------- History: From electronic version of the journal
(End) Prepared by [AAS], Coralie Fix [CDS], 02-Jun-2023
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