A low-eccentricity migration pathway for a 13-h-period Earth analogue in a four-planet system
- Author(s):
- Serrano, L.M.; Gandolfi, D.; Mustill, A.J.; Barragán, O.; Korth, J.; Dai, F.; Redfield, S.; Fridlund, M.; Lam, K.W.F.; Díaz, M.R.; Grziwa, S.; Collins, K.A.; Livingston, J.H.; Cochran, W.D.; Hellier, C.; Bellomo, S.E.; Trifonov, T.; Rodler, F.; Alarcon, J.; Jenkins, J.M.; Latham, D.W.; Ricker, G.; Seager, S.; Vanderspeck, R.; Winn, J.N.; Albrecht, S.; Collins, K.I.; Csizmadia, S.; Daylan, T.; Deeg, H.J.; Esposito, M.; Fausnaugh, M.; Georgieva, I.; Goffo, E.; Guenther, E.; Hatzes, A.P.; Howell, S.B.; Jensen, E.L.N.; Luque, R.; Mann, A.W.; Murgas, F.; Osborne, H.L.M.; Palle, E.; Persson, C.M.; Rowden, P.; Rudat, A.; Smith, A.M.S.; Twicken, J.D.; Eylen, V. Van; Ziegler, C.
- Published
- 2022
- Publication type
- Article / Letter to editor
Astrophysics - Earth and Planetary Astrophysics
- Date issued
- 2022
- Language
- English
- Is part of
- Nature Astronomy (2022), Vol. 6, p. 736-750
- hdl
- 1887/3561580
- doi
- 10.1038/s41550-022-01641-y
- URL
- https://ui.adsabs.harvard.edu/abs/2022NatAs...6..736S
