K2-98b: A 32 M⊕ NEPTUNE-SIZE PLANET IN A 10 DAY ORBIT TRANSITING AN F8 STAR

被引:23
|
作者
Barragan, Oscar [1 ]
Grziwa, Sascha
Gandolfi, Davide
Fridlund, Malcolm
Endl, Michael
Deeg, Hans J. [2 ,3 ]
Cagigal, Manuel P. [14 ,15 ]
Lanza, Antonino F.
Moroni, Pier G. Prada [5 ,7 ,14 ,16 ]
Smith, Alexis M. S. [3 ,9 ,15 ]
Korth, Judith [2 ,4 ,5 ,10 ]
Bedell, Megan [9 ,13 ,16 ]
Cabrera, Juan [1 ,6 ,12 ,17 ]
Cochran, William D. [11 ,13 ]
Cusano, Felice [8 ]
Csizmadia, Szilard [3 ,5 ,9 ,15 ]
Eigmueller, Philipp [4 ,6 ,7 ,8 ,17 ]
Erikson, Anders [5 ,8 ,12 ,16 ]
Guenther, Eike W. [2 ,7 ,8 ,10 ,14 ]
Hatzes, Artie P. [1 ,2 ,11 ]
Nespral, David
Paetzold, Martin
Prieto-Arranz, Jorge
Rauer, Heike
机构
[1] Univ Torino, Dipartimento Fis, Via P Giuria 1, I-10125 Turin, Italy
[2] Univ Cologne, Rhein Inst Umweltforsch, Aachener Str 209, Cologne, Germany
[3] Heidelberg Univ, Zentrum Astron, D-69117 Heidelberg, Germany
[4] Leiden Univ, Leiden Observ, NL-2300 RA Leiden, Netherlands
[5] Onsala Space Observ, Chalmers Univ Technol, Dept Earth & Space Sci, S-43992 Onsala, Sweden
[6] Univ Texas, Dept Astron & McDonald Observ, Austin, TX 78712 USA
[7] Inst Astrof sica Canarias, San Cristobal la Laguna 38205, Spain
[8] Univ Laguna, Dept Astrof sica, San Cristobal la Laguna 38206, Spain
[9] Univ Cantabria, Dept Fis Aplicada, E-39005 Santander, Spain
[10] INAF Osservatorio Astrofisico Catania, Via S Sofia 78, Catania, Italy
[11] Univ Pisa, Phys Dept Fermi, Largo B Pontecorvo 3, Pisa, Italy
[12] Ist Nazl Fis Nucl, Largo B Pontecorvo 3, I-12489 Pisa, Italy
[13] Inst Planetary Res, German Aerosp Ctr, Rutherfordstr 2, D-12489 Berlin, Germany
[14] Univ Chicago, Dept Astron & Astrophys, 5640 S Ellis Ave, Chicago, IL 60637 USA
[15] INAF, Osservatorio Astronomico Bologna, Via Ranzani, Bologna, Italy
[16] Thuringer Landessternwarte Tautenburg, D-07778 Tautenburg, Germany
[17] TU Berlin, Ctr Astron & Astrophys, Hardenbergstr 36, D-10623 Berlin, Germany
来源
ASTRONOMICAL JOURNAL | 2016年 / 152卷 / 06期
基金
美国国家科学基金会; 美国国家航空航天局;
关键词
planets and satellites: detection; planets and satellites: individual K2-98b (EPIC 211391664b); stars: fundamental parameters; HOT JUPITERS; SUPER-EARTHS; EXOPLANETS; MASS; CANDIDATES; SPECTROGRAPH; PARAMETERS; BINARIES; SEARCH; TOOL;
D O I
10.3847/0004-6256/152/6/193
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
We report the discovery of K2-98b (EPIC 211391664b), a transiting Neptune-size planet monitored by the K2 mission during its Campaign 5. We combine the K2 time-series data with ground-based photometric and spectroscopic follow-up observations to confirm the planetary nature of the object and derive its mass, radius, and orbital parameters. K2-98b is a warm Neptune-like planet in a 10 day orbit around a V = 12.2 mag F-type star with M-star = 1.074 +/- 0.042 M-circle dot, R-star = 1.311(-0.048)(+0.083) R-circle dot, and age of 5.2(-1.0)(+1.2) Gyr We derive a planetary mass and radius of M-p = 32.2 +/- 8.1 M-circle plus and R-p = 4.3(-0.2)(+0.3) R-circle plus.K2-98b joins the relatively small group of Neptune-size planets whose mass and radius have been derived with a precision better than 25%. We estimate that the planet will be engulfed by its host star in similar to 3 Gyr, due to the evolution of the latter toward the red giant branch.
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页数:9
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