KELT-6
13 03 55.6468
+30 38 24.2797
222
KELT-6
TYC 2532-556-1
BD+31 2447
2MASS J13035564+3038241
Gaia DR2 1464700950221781504
1.126
1.529
6272
10.337
9.745
9.137
10.81
9.30
9.08
-0.27
F8
4.90
KELT-6 b
TYC 2532-556-1 b
BD+31 2447 b
Gaia DR2 1464700950221781504 b
Confirmed planets
0.442
1.18
7.845582
0.080
0.029
88.81
2457124.50954
308
-36
KELT-6b is a Saturn-mass planet transiting a metal-poor host star. The planet candidate was originally discovered by the KELT-North survey. Follow up observations confirmed the planetary nature of the candidate using a combination of photometry, high-resolution imaging, high resolution spectroscopy and radial velocity measurements.
transit
15/08/27
2013
1
KELT-6 c
TYC 2532-556-1 c
BD+31 2447 c
Gaia DR2 1464700950221781504 c
Confirmed planets
1276
0.21
268.7
2457432
3.71
2.39
KELT-6c is a long-period giant planet, one of only a small number known where there is an inner transiting planet with a measured Rossiter-McLaughlin effect. Its presence was suspected based on a trend in the radial velocity data for the system and was finally confirmed in 2015 with data from the HARPS-N spectrograph.
RV
15/08/27
2015
0
Coma Berenices