K2-137 b: an Earth-sized planet in a 4.3-hour orbit around an M-dwarf
| Autor: | Smith, A. M. S., Cabrera, J., Csizmadia, Sz., Dai, F., Gandolfi, D., Hirano, T., Winn, J. N., Albrecht, S., Alonso, R., Antoniciello, G., Barragán, O., Deeg, H., Eigmüller, Ph., Endl, M., Erikson, A., Fridlund, M., Fukui, A., Grziwa, S., Guenther, E. W., Hatzes, A. P., Hidalgo, D., Howard, A. W., Isaacson, H., Korth, J., Kuzuhara, M., Livingston, J., Narita, N., Nespral, D., Nowak, G., Palle, E., Pätzold, M., Persson, C. M., Petigura, E., Prieto-Arranz, J., Rauer, H., Ribas, I., Van Eylen, V. |
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| Rok vydání: | 2017 |
| Předmět: | |
| Zdroj: | MNRAS 474, 5523 (2018) |
| Druh dokumentu: | Working Paper |
| DOI: | 10.1093/mnras/stx2891 |
| Popis: | We report the discovery from K2 of a transiting terrestrial planet in an ultra-short-period orbit around an M3-dwarf. K2-137 b completes an orbit in only 4.3 hours, the second-shortest orbital period of any known planet, just 4 minutes longer than that of KOI 1843.03, which also orbits an M-dwarf. Using a combination of archival images, AO imaging, RV measurements, and light curve modelling, we show that no plausible eclipsing binary scenario can explain the K2 light curve, and thus confirm the planetary nature of the system. The planet, whose radius we determine to be 0.89 +/- 0.09 Earth radii, and which must have a iron mass fraction greater than 0.45, orbits a star of mass 0.463 +/- 0.052 Msol and radius 0.442 +/- 0.044 Rsol. Comment: 12 pages, 9 figures, accepted for publication in MNRAS |
| Databáze: | arXiv |
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