K2-141 b: A 5- M ⊗ super-Earth transiting a K7 v star every 6.7 h

We report on the discovery of K2-141 b (EPIC 246393474 b), an ultra-short-period super-Earth on a 6.7 h orbit transiting an active K7 V star based on data from K2 campaign 12. We confirmed the planet's existence and measured its mass with a series of follow-up observations: seeing-limited Muscat imaging, NESSI high-resolution speckle observations, and FIES and HARPS high-precision radial-velocity monitoring. K2-141 b has a mass of 5.31 ± 0.46 M ⊗ and radius of 1.54 -0.09 +0.10 R ⊗ , yielding a mean density of 8.00 -1.45 +1.83 g cm -3 and suggesting a rocky-iron composition. Models indicate that iron cannot exceed ∼70% of the total mass. With an orbital period of only 6.7 h, K2-141 b is the shortest-period planet known to date with a precisely determined mass.

[1]  D. F. Gray,et al.  The Observation and Analysis of Stellar Photospheres , 2021 .

[2]  Marshall C. Johnson,et al.  The Discovery and Mass Measurement of a New Ultra-short-period Planet: K2-131b , 2017, 1710.00076.

[3]  S. Csizmadia,et al.  K2-137 b: an Earth-sized planet in a 4.3-h orbit around an M-dwarf , 2017, 1707.04549.

[4]  R. P. Butler,et al.  K2-106, a system containing a metal-rich planet and a planet of lower density , 2017, 1705.04163.

[5]  A. Johansen,et al.  K2-111 b − a short period super-Earth transiting a metal poor, evolved old star , 2017, 1704.08284.

[6]  P. Cargile,et al.  Absence of a Metallicity Effect for Ultra-short-period Planets , 2017, 1704.00203.

[7]  Howard Isaacson,et al.  The California-Kepler Survey. III. A Gap in the Radius Distribution of Small Planets , 2017, 1703.10375.

[8]  M. Tamura,et al.  The K2-ESPRINT project. VI. K2-105 b, a hot Neptune around a metal-rich G-dwarf , 2017, 1701.01294.

[9]  E. Petigura,et al.  Precision Stellar Characterization of FGKM Stars using an Empirical Spectral Library , 2017, 1701.00922.

[10]  A. Bonomo,et al.  KEPLER-21b: A ROCKY PLANET AROUND A V = 8.25 mag STAR , 2016, 1609.07617.

[11]  Observatoire de la Côte d'Azur,et al.  Gaia Data Release 1. Summary of the astrometric, photometric, and survey properties , 2016, 1609.04172.

[12]  J. Portell,et al.  Gaia Data Release 1: Pre-processing and source list creation , 2016 .

[13]  S. Csizmadia,et al.  K2-99 : a subgiant hosting a transiting warm Jupiter in an eccentric orbit and a long-period companion , 2016, 1609.00239.

[14]  Antonino Francesco Lanza,et al.  K2-98b: A 32 M⊕ NEPTUNE-SIZE PLANET IN A 10 DAY ORBIT TRANSITING AN F8 STAR , 2016, 1608.01165.

[15]  J. Valenti,et al.  Spectroscopy Made Easy: Evolution , 2016, 1606.06073.

[16]  R. Gilliland,et al.  Hot super-Earths stripped by their host stars , 2016, Nature Communications.

[17]  S. Csizmadia,et al.  Mass determination of K2-19b and K2-19c from radial velocities and transit timing variations , 2016, 1604.01265.

[18]  Davide Gandolfi,et al.  TWO HOT JUPITERS FROM K2 CAMPAIGN 4 , 2016, 1601.07844.

[19]  Dimitar Sasselov,et al.  MASS–RADIUS RELATION FOR ROCKY PLANETS BASED ON PREM , 2015, 1512.08827.

[20]  Norio Narita,et al.  MuSCAT: a multicolor simultaneous camera for studying atmospheres of transiting exoplanets , 2015, 1509.03154.

[21]  L. Buchhave,et al.  THE METALLICITIES OF STARS WITH AND WITHOUT TRANSITING PLANETS , 2015, 1507.03557.

[22]  M. Paegert,et al.  THE K2-ESPRINT PROJECT. I. DISCOVERY OF THE DISINTEGRATING ROCKY PLANET K2-22b WITH A COMETARY HEAD AND LEADING TAIL , 2015, 1504.04379.

[23]  F. Allard,et al.  New evolutionary models for pre-main sequence and main sequence low-mass stars down to the hydrogen-burning limit , 2015, 1503.04107.

[24]  R. Angus,et al.  Calibrating gyrochronology using Kepler asteroseismic targets , 2015, 1502.06965.

[25]  R. Haywood,et al.  DETERMINING THE MASS OF KEPLER-78b WITH NONPARAMETRIC GAUSSIAN PROCESS ESTIMATION , 2015, 1501.00369.

[26]  A. Szentgyorgyi,et al.  THE MASS OF Kepler-93b AND THE COMPOSITION OF TERRESTRIAL PLANETS , 2014, 1412.8687.

[27]  Antonino Francesco Lanza,et al.  Kepler-423b: a half-Jupiter mass planet transiting a very old solar-like star , 2014, 1409.8245.

[28]  Nuno C. Santos,et al.  SOAP 2.0: A TOOL TO ESTIMATE THE PHOTOMETRIC AND RADIAL VELOCITY VARIATIONS INDUCED BY STELLAR SPOTS AND PLAGES , 2014, 1409.3594.

[29]  A. Vanderburg,et al.  A Technique for Extracting Highly Precise Photometry for the Two-Wheeled Kepler Mission , 2014, 1408.3853.

[30]  Andrew Szentgyorgyi,et al.  THE KEPLER-10 PLANETARY SYSTEM REVISITED BY HARPS-N: A HOT ROCKY WORLD AND A SOLID NEPTUNE-MASS PLANET , 2014, 1405.7881.

[31]  Michael C. Kotson,et al.  A STUDY OF THE SHORTEST-PERIOD PLANETS FOUND WITH KEPLER , 2014, 1403.2379.

[32]  T. Mazeh,et al.  ROTATION PERIODS OF 34,030 KEPLER MAIN-SEQUENCE STARS: THE FULL AUTOCORRELATION SAMPLE , 2014, 1402.5694.

[33]  J. Fortney,et al.  UNDERSTANDING THE MASS–RADIUS RELATION FOR SUB-NEPTUNES: RADIUS AS A PROXY FOR COMPOSITION , 2013, 1311.0329.

[34]  Andrew Szentgyorgyi,et al.  An Earth-sized planet with an Earth-like density , 2013, Nature.

[35]  A. Ofir Optimizing the search for transiting planets in long time series , 2013, 1307.7330.

[36]  L. Rogers,et al.  THE ROCHE LIMIT FOR CLOSE-ORBITING PLANETS: MINIMUM DENSITY, COMPOSITION CONSTRAINTS, AND APPLICATION TO THE 4.2 hr PLANET KOI 1843.03 , 2013, 1307.4080.

[37]  E. Mamajek,et al.  INTRINSIC COLORS, TEMPERATURES, AND BOLOMETRIC CORRECTIONS OF PRE-MAIN-SEQUENCE STARS , 2013, 1307.2657.

[38]  A. Collier Cameron,et al.  Planets and Stellar Activity: Hide and Seek in the CoRoT-7 system , 2013, Proceedings of the International Astronomical Union.

[39]  James E. Owen,et al.  KEPLER PLANETS: A TALE OF EVAPORATION , 2013, 1303.3899.

[40]  Robert L. Kurucz,et al.  ATLAS12: Opacity sampling model atmosphere program , 2013 .

[41]  Cambridge,et al.  A Detailed Model Grid for Solid Planets from 0.1 through 100 Earth Masses , 2013, 1301.0818.

[42]  G. Bruce Berriman,et al.  Astrophysics Source Code Library , 2012, ArXiv.

[43]  J. B. Laird,et al.  An abundance of small exoplanets around stars with a wide range of metallicities , 2012, Nature.

[44]  Daniel Foreman-Mackey,et al.  emcee: The MCMC Hammer , 2012, 1202.3665.

[45]  G. Fontaine,et al.  A compact system of small planets around a former red-giant star , 2011, Nature.

[46]  D. Ciardi,et al.  SPECKLE CAMERA OBSERVATIONS FOR THE NASA KEPLER MISSION FOLLOW-UP PROGRAM , 2011 .

[47]  Guillaume Hebrard,et al.  THE MASS OF CoRoT-7b , 2011, 1105.3372.

[48]  G. Torres ON THE USE OF EMPIRICAL BOLOMETRIC CORRECTIONS FOR STARS , 2010, 1008.3913.

[49]  D. Kipping Morphological Lightcurve Distortions due to Finite Integration Time , 2010, 1004.3741.

[50]  A. Gimenez,et al.  Accurate masses and radii of normal stars: modern results and applications , 2009, 0908.2624.

[51]  B. Skiff,et al.  VizieR Online Data Catalog , 2009 .

[52]  F. Allard,et al.  VOSA: Virtual Observatory SED Analyzer. An application to the Collinder 69 open cluster , 2008, 0808.0270.

[53]  L. Testi,et al.  The Star Formation in the L1615/L1616 Cometary Cloud , 2008, 0807.0532.

[54]  J. Valenti,et al.  Spectroscopic Properties of Cool Stars (SPOCS). I. 1040 F, G, and K Dwarfs from Keck, Lick, and AAT Planet Search Programs , 2005 .

[55]  E. Agol,et al.  Analytic Light Curves for Planetary Transit Searches , 2002, astro-ph/0210099.

[56]  G. Kov'acs,et al.  A box-fitting algorithm in the search for periodic transits , 2002, astro-ph/0206099.

[57]  J. Valenti,et al.  Spectroscopy Made Easy: A New Tool for Fitting Observations with Synthetic Spectra , 1996 .

[58]  J. Mathis,et al.  The relationship between infrared, optical, and ultraviolet extinction , 1989 .

[59]  R. Fisher Statistical methods for research workers , 1927, Protoplasma.

[60]  H. C. Stempels,et al.  FIES: The high-resolution Fiber-fed Echelle Spectrograph at the Nordic Optical Telescope , 2014 .