TESS DISCOVERY OF A TRANSITING SUPER-EARTH IN THE π MENSAE SYSTEM.
Huang CX, Burt J, Vanderburg A, Günther MN, Shporer A, Dittmann JA, Winn JN, Wittenmyer R, Sha L, Kane SR, Ricker GR, Vanderspek RK, Latham DW, Seager S, Jenkins JM, Caldwell DA, Collins KA, Guerrero N, Smith JC, Quinn SN, Udry S, Pepe F, Bouchy F, Ségransan D, Lovis C, Ehrenreich D, Marmier M, Mayor M, Wohler B, Haworth K, Morgan EH, Fausnaugh M, Ciardi DR, Christiansen J, Charbonneau D, Dragomir D, Deming D, Glidden A, Levine AM, McCullough PR, Yu L, Narita N, Nguyen T, Morton T, Pepper J, Pál A, Rodriguez JE; TESS team.
Huang CX, et al.
Astrophys J Lett. 2018 Dec 1;868(2):10.3847/2041-8213/aaef91. doi: 10.3847/2041-8213/aaef91. Epub 2018 Nov 30.
Astrophys J Lett. 2018.
PMID: 31360431
Free PMC article.
The solar-type host star is unusually bright (V = 5.7) and was already known to host a Jovian planet on a highly eccentric, 5.7-year orbit. The newly discovered planet has a size of 2.04 0.05 R () and an orbital period of 6.27 days. Radial-velocity data from the HARPS and …
The solar-type host star is unusually bright (V = 5.7) and was already known to host a Jovian planet on a highly eccentric, 5.7-year orbit. …