Kepler-296
KOI-1422
KIC 11497958
19 06 09.602
+49 26 14.37
558.5
0.217
80
217.3
Kepler-296 A
KOI-1422 A
KIC 11497958 A
2MASS J19060960+4926143 A
13.73
12.93
3740
-0.08
0.480
0.498
M2V
Kepler-296 c
Kepler-296 Ac
KOI-1422 c
KOI-1422.01
KIC 11497958 c
KIC 11497958.01 c
2MASS J19060960+4926143 c
0.178
5.8416366
0.0521
2454968.9229
89.4
Confirmed planets

Planets in binary systems, S-type

Kepler-296 Ac has been discovered by the Kepler spacecraft and was originally classified as a planet candidate. A new statistical analysis led by a team at NASA Ames Research Center has validated the planet with more than 99 percent confidence. Although many parameters of Kepler-296 Ac are still unknown, the object is highly unlikely to be a false positive. Statistical analysis indicates that all five transiting planets in the system orbit the primary star Kepler-296 A.
2014
15/05/11
transit
1
Kepler-296 d
Kepler-296 Ad
KOI-1422 d
KOI-1422.02
KIC 11497958 d
KIC 11497958.02 d
2MASS J19060960+4926143 d
0.186
19.850291
0.118
2454966.6496
89.7
Confirmed planets

Planets in binary systems, S-type

Kepler-296 Ad has been discovered by the Kepler spacecraft and was originally classified as a planet candidate. A new statistical analysis led by a team at NASA Ames Research Center has validated the planet with more than 99 percent confidence. Although many parameters of Kepler-296 Ad are still unknown, the object is highly unlikely to be a false positive. Statistical analysis indicates that all five transiting planets in the system orbit the primary star Kepler-296 A.
2014
15/05/11
transit
1
Kepler-296 b
Kepler-296 Ab
KOI-1422 b
KOI-1422.03
KIC 11497958 b
KIC 11497958.03 b
2MASS J19060960+4926143 b
0.144
10.864384
0.079
2454964.1285
89.0
Confirmed planets

Planets in binary systems, S-type

Kepler-296 Ab has been discovered by the Kepler spacecraft and was originally classified as a planet candidate. A new statistical analysis led by a team at NASA Ames Research Center has validated the planet with more than 99 percent confidence. Although many parameters of Kepler-296 Ab are still unknown, the object is highly unlikely to be a false positive. This planet was originally thought to have a period three times smaller than the actual value. Statistical analysis indicates that all five transiting planets in the system orbit the primary star Kepler-296 A.
2014
15/05/11
transit
1
Kepler-296 f
Kepler-296 Af
KOI-1422 f
KOI-1422.04
KIC 11497958 f
KIC 11497958.04 f
2MASS J19060960+4926143 f
0.161
63.33627
0.255
2454995.6069
89.7
Confirmed planets

Planets in binary systems, S-type

Kepler-296 Af has been discovered by the Kepler spacecraft and was originally classified as a planet candidate. A new statistical analysis led by a team at NASA Ames Research Center has validated the planet with more than 99 percent confidence. Although many parameters of Kepler-296 Af are still unknown, the object is highly unlikely to be a false positive. Statistical analysis indicates that all five transiting planets in the system orbit the primary star Kepler-296 A. This planet receives an incident flux from its host star 0.62 times that received by Earth from the Sun.
2014
15/05/11
transit
1
Kepler-296 e
Kepler-296 Ae
KOI-1422 e
KOI-1422.05
KIC 11497958 e
KIC 11497958.05 e
2MASS J19060960+4926143 e
0.136
34.14211
0.169
2454969.0350
89.7
Planets in binary systems, S-type

Confirmed planets

Kepler-296 Ae has been discovered by the Kepler spacecraft and was originally classified as a planet candidate. A new statistical analysis led by a team at NASA Ames Research Center has validated the planet with more than 99 percent confidence. Although many parameters of Kepler-296 Ae are still unknown, the object is highly unlikely to be a false positive. Statistical analysis indicates that all five transiting planets in the system orbit the primary star Kepler-296 A. This planet receives an incident flux from its host star 1.41 times greater than that the Earth receives from the Sun.
2014
15/05/11
transit
1
Kepler-296 B
KOI-1422 B
KIC 11497958 B
2MASS J19060960+4926143 B
14.83
14.07
3440
-0.08
0.322
0.326