KOI-5

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KOI-5
Observation data
Epoch J2000      Equinox
Constellation Cygnus
Right ascension 19h 18m 57.5312s
Declination +44° 38′ 50.6176″
Distance
1,870 ± 70 ly
(570 ± 20 pc)
Position (relative to KOI-5A)[2]
ComponentKOI-5B
Projected separation
16[citation needed] AU
Position (relative to KOI-5A)[2]
ComponentKOI-5C
Projected separation
78[citation needed] AU
Details
Gyr
KOI-5B
Mass1.09[4] M
Other designations
TOI-1241, 2MASS J19185753+4438507, KIC 8554498, Gaia EDR3 2126945668448657664
KOI-5A:
KOI-5B:
Database references
SIMBADdata

KOI-5 is a

triple star system
composed of three stars: KOI-5 A, KOI-5 B and KOI-5 C, orbiting 1,870±70 light-years away.

The two dim stellar companions to KOI-5A were discovered in 2016.[2] KOI-5 A and B orbit each other every 29 years, and KOI-5 C orbits stars A and B every 400 years.[4] KOI-5C is physically associated with the core stellar pair with probability 99.98%.[6]

Planetary system

Two planets orbiting one of KOI-5's stars were suspected since 2009 based on

KOI-5Ab was confirmed only in January 2021 after TESS determined the planet is orbiting KOI-5A. The exoplanet has caused interest in the scientific community because its orbital plane is misaligned with the closer star, suggesting it gave KOI-5Ab a gravitational kick during its development, resulting in the misalignment and inward migration to the current orbit.[4][7]
However, the confirmation of this planet has yet to be published in any peer-reviewed journal.

A second candidate planet was initially suspected, but was later found to be a false positive.[8]

The KOI-5A planetary system[6][4][8]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 0.179 MJ 0.0596060 5 7.07 R🜨

References

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