K2-60b and K2-107b. A Sub-Jovian and a Jovian Planet from the K2 Mission
Creators
- Eigmüller, Philipp1
- Csizmadia, Szilard1
- Smith, Alexis M. S.1
- Cabrera, Juan1
- Erikson, Anders1
- Gandolfi, Davide2
- Barragán, Oscar2
- Persson, Carina M.3
- Fridlund, Malcolm3
- Donati, Paolo4
- Cusano, Felice4
- Korth, Judith5
- Grziwa, Sascha5
- Prieto-Arranz, Jorge6
- Nespral, David6
- Deeg, Hans J.6
- Saario, Joonas7
- Cochran, William D.8
- Endl, Michael8
- Guenther, Eike W.9
- and others
- 1. Institute of Planetary Research, German Aerospace Center, Rutherfordstrasse 2, D-12489 Berlin (Germany)
- 2. Dipartimento di Fisica, Universitá di Torino, via P. Giuria 1, I-10125 Torino (Italy)
- 3. Department of Earth and Space Sciences, Chalmers University of Technology, Onsala Space Observatory, SE-439 92 Onsala (Sweden)
- 4. INAF—Osservatorio Astronomico di Bologna, Via Ranzani, 1, I-40127, Bologna (Italy)
- 5. Rheinisches Institut für Umweltforschung an der Universität zu Köln, Aachener Strasse 209, D-50931 Köln (Germany)
- 6. Instituto de Astrofísica de Canarias, E-38205 La Laguna, Tenerife (Spain)
- 7. Nordic Optical Telescope, Apartado 474, E-38700, Santa Cruz de La Palma (Spain)
- 8. Department of Astronomy and McDonald Observatory, University of Texas at Austin, 2515 Speedway, Stop C1400, Austin, TX 78712 (United States)
- 9. Thüringer Landessternwarte Tautenburg, Sternwarte 5, D-07778 Tautenberg (Germany)
Description
We report the characterization and independent detection of K2-60b, as well as the detection and characterization of K2-107b, two transiting hot gaseous planets from the K2 space mission. We confirm the planetary nature of the two systems and determine their fundamental parameters combining the K2 time-series data with FIES@NOT and HARPS-N@TNG spectroscopic observations. K2-60b has a radius of 0.683 ± 0.037 R Jup and a mass of 0.426 ± 0.037 M Jup and orbits a G4 V star with an orbital period of 3.00267 ± 0.00006 days. K2-107b has a radius of 1.44 ± 0.15 R Jup and a mass of 0.84 ± 0.08 M Jup and orbits an F9 IV star every 3.31392 ± 0.00002 days. K2-60b is among the few planets at the edge of the so-called "desert" of short-period sub-Jovian planets. K2-107b is a highly inflated Jovian planet orbiting an evolved star about to leave the main sequence.
Availability note (English)
Available from http://dx.doi.org/10.3847/1538-3881/aa5d0bAdditional details
Identifiers
Publishing Information
- Journal Title
- Astronomical Journal (New York, N.Y. Online)
- Journal Volume
- 153
- Journal Issue
- 3
- Journal Page Range
- [8 p.]
- ISSN
- 1538-3881
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 49009228
- Subject category
- S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
- Descriptors DEI
- DETECTION; MASS; ORBITS; PLANETS; SATELLITES; SPACE; STARS