Kepler-28
KOI-870
KIC 6949607
19 28 32.8905
+42 25 45.9593
772.8
Kepler-28
KOI-870
KIC 6949607
2MASS J19283288+4225459
Gaia DR2 2125731464014361088
4590.0
0.75
0.70
0.34
13.334
12.767
12.719
K4V
Kepler-28 b
KOI-870.01
KOI-870 b
KIC 6949607 b
Gaia DR2 2125731464014361088 b
Confirmed planets
0.32806906
5.91
0.062
2454975.6227
This planet candidate was discovered with the Kepler spacecraft. Its host star gets periodically fainter whenever the planet is in front of the star. Because there are multiple phenomena that can create a signal that looks similar to a planetary transit, the candidates have to be confirmed with another method. For Kepler-28 the planetary nature of the companions has been confirmed by transit timing variations, caused by other planets in the system, and a stability analysis. However, the mass of the planets is not well constrained yet.
transit
12/01/26
2012
680.0
1
Kepler-28 c
KOI-870.02
KOI-870 c
KIC 6949607 c
Gaia DR2 2125731464014361088 c
Confirmed planets
0.30984
8.98
0.081
2454981.7277
This planet candidate was discovered with the Kepler spacecraft. Its host star gets periodically fainter whenever the planet is in front of the star. Because there are multiple phenomena that can create a signal that looks similar to a planetary transit, the candidates have to be confirmed with another method. For Kepler-28 the planetary nature of the companions has been confirmed by transit timing variations, caused by other planets in the system, and a stability analysis. However, the mass of the planets is not well constrained yet.
transit
12/08/06
2012
595.0
1
Cygnus