TOI 122b and TOI 237b, two small warm planets orbiting inactive M dwarfs, found by \textit{TESS}
arXiv:2010.15905 · doi:10.3847/1538-3881/abc3b9
Abstract
We report the discovery and validation of TOI 122b and TOI 237b, two warm planets transiting inactive M dwarfs observed by \textit{TESS}. Our analysis shows TOI 122b has a radius of 2.720.18 R$_\rm{e}$ and receives 8.81.0 Earth's bolometric insolation, and TOI 237b has a radius of 1.440.12 R$_\rm{e}$ and receives 3.70.5 Earth insolation, straddling the 6.7 Earth insolation that Mercury receives from the sun. This makes these two of the cooler planets yet discovered by \textit{TESS}, even on their 5.08-day and 5.43-day orbits. Together, they span the small-planet radius valley, providing useful laboratories for exploring volatile evolution around M dwarfs. Their relatively nearby distances (62.230.21 pc and 38.110.23 pc, respectively) make them potentially feasible targets for future radial velocity follow-up and atmospheric characterization, although such observations may require substantial investments of time on large telescopes.
21 pages, 9 figures, 4 tables, accepted to AJ
References in corpus (58)
- Astropy: A Community Python Package for Astronomy
- emcee: The MCMC Hammer
- The NumPy array: a structure for efficient numerical computation
- Gaia Data Release 2. Summary of the contents and survey properties
- The Transiting Exoplanet Survey Satellite
- Analytic Lightcurves for Planetary Transit Searches
- The K2 Mission: Characterization and Early results
- Habitable Zones Around Main-Sequence Stars: New Estimates
- Understanding the Lomb-Scargle Periodogram
- Las Cumbres Observatory Global Telescope Network
- batman: BAsic Transit Model cAlculatioN in Python
- Kepler Presearch Data Conditioning II - A Bayesian Approach to Systematic Error Correction
- The Revised TESS Input Catalog and Candidate Target List
- On the Unique Solution of Planet and Star Parameters from an Extrasolar Planet Transit Light Curve
- Kepler Presearch Data Conditioning I - Architecture and Algorithms for Error Correction in Kepler Light Curves
- How to Constrain Your M Dwarf: measuring effective temperature, bolometric luminosity, mass, and radius
- AstroImageJ: Image Processing and Photometric Extraction for Ultra-Precise Astronomical Light Curves
- AstroImageJ: Image Processing and Photometric Extraction for Ultra-Precise Astronomical Light Curves (Expanded Edition)
- Probabilistic Forecasting of the Masses and Radii of Other Worlds
- Constraining the Age-Activity Relation for Cool Stars: The SDSS DR5 Low-Mass Star Spectroscopic Sample
- A Framework for Prioritizing the TESS Planetary Candidates Most Amenable to Atmospheric Characterization
- Theory of Low-Mass Stars and Substellar Objects
- The Transiting Exoplanet Survey Satellite: Simulations of planet detections and astrophysical false positives
- Design Considerations for a Ground-based Transit Search for Habitable Planets Orbiting M dwarfs
- Nominal values for selected solar and planetary quantities: IAU 2015 Resolution B3
- The Statistics of Albedo and Heat Recirculation on Hot Exoplanets
- The H emission of nearby M dwarfs and its relation to stellar rotation
- How to Constrain Your M dwarf II: the mass-luminosity-metallicity relation from 0.075 to 0.70
- Improving Stellar and Planetary Parameters of Transiting Planet Systems: The Case of TrES-2
- Kepler Data Validation I -- Architecture, Diagnostic Tests, and Data Products for Vetting Transiting Planet Candidates
- Data analysis recipes: Using Markov Chain Monte Carlo
- A Revised Exoplanet Yield from the Transiting Exoplanet Survey Satellite (TESS)
- The rotation and Galactic kinematics of mid M dwarfs in the Solar Neighborhood
- Kepler Data Validation II -- Transit Model Fitting and Multiple-Planet Search
- SOAR TESS Survey. I: Sculpting of TESS planetary systems by stellar companions
- LDTk: Limb Darkening Toolkit
- The Effective Temperature Scale of M dwarfs
- An Increase in the Mass of Planetary Systems around Lower-Mass Stars
- The cosmic shoreline: the evidence that escape determines which planets have atmospheres, and what this may mean for Proxima Centauri b
- Planets Around Low-Mass Stars (PALMS). IV. The Outer Architecture of M Dwarf Planetary Systems
- The Habitable-Zone Planet Finder: A Stabilized Fiber-Fed NIR Spectrograph for the Hobby-Eberly Telescope
- Ten years of speckle interferometry at SOAR
- TESS Discovery of an ultra-short-period planet around the nearby M dwarf LHS 3844
- The Dependence of Brown Dwarf Radii on Atmospheric Metallicity and Clouds: Theory and Comparison with Observations
- The L 98-59 System: Three Transiting, Terrestrial-Sized Planets Orbiting a Nearby M-dwarf
- Planetary system around the nearby M dwarf GJ 357 including a transiting, hot, Earth-sized planet optimal for atmospheric characterization
- A super-Earth and two sub-Neptunes transiting the nearby and quiet M dwarf TOI-270
- The Precision of Mass Measurements Required for Robust Atmospheric Characterization of Transiting Exoplanets
- MN48: a new Galactic bona fide luminous blue variable revealed by Spitzer and SALT
- Three Red Suns in the Sky: A Transiting, Terrestrial Planet in a Triple M Dwarf System at 6.9 Parsecs
- Multicolour photometry for exoplanet candidate validation
- Characterization of the L 98-59 multi-planetary system with HARPS: two confirmed terrestrial planets and a mass upper limit on the third
- A sub-Neptune sized planet transiting the M2.5-dwarf G 9-40: Validation with the Habitable-zone Planet Finder
- Predicted Number, Multiplicity, and Orbital Dynamics of TESS M Dwarf Exoplanets
- Near Infrared Monitoring of Ultracool Dwarfs: Prospects for Searching for Transiting Companions
- A super-Earth and sub-Neptune transiting the late-type M dwarf LP 791-18
- A hot terrestrial planet orbiting the bright M dwarf L 168-9 unveiled by TESS
- Energy Budgets for Terrestrial Extrasolar Planets
Cited by in corpus (13)
- New Perspectives on the Exoplanet Radius Gap from a Mathematica Tool and Visualized Water Equation of State
- A super-Earth and a mini-Neptune near the 2:1 MMR straddling the radius valley around the nearby mid-M dwarf TOI-2096
- NEMESIS: Exoplanet Transit Survey of Nearby M-Dwarfs in TESS FFIs I
- Characterisation of 92 Southern TESS Candidate Planet Hosts and a New Photometric [Fe/H] Relation for Cool Dwarfs
- The LHS 1678 System: Two Earth-Sized Transiting Planets and an Astrometric Companion Orbiting an M Dwarf Near the Convective Boundary at 20 pc
- The Atmospheres of Rocky Exoplanets II. Influence of surface composition on the diversity of cloud condensates
- TESS discovery of a super-Earth orbiting the M dwarf star TOI-1680
- Hundreds of TESS exoplanets might be larger than we thought
- TOI-1696 and TOI-2136: Constraining the Masses of Two Mini-Neptunes with HPF
- Gaia-TESS synergy: Improving the identification of transit candidates
- Earth-like planet predictor: A machine learning approach
- Hidden Gems in TESS: sherlock finds two new rocky planets around nearby M dwarfs
- The M-dwarf Ultraviolet Spectroscopic Sample I. Determining Stellar Parameters for Field Stars