Coordinates: Sky map 19h 18m 57.5312s, +44° 38′ 50.6176″

KOI-5

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KOI-5
Observation data
Epoch J2000      Equinox
Constellation Cygnus[1]
Right ascension 19h 18m 57.5306s[2]
Declination +44° 38′ 50.619″[2]
Apparent magnitude (V) 11.78[3]
Characteristics
Spectral type G2V[4]
Astrometry
Radial velocity (Rv)−35.16[2] km/s
Proper motion (μ) RA: +3.216[2] mas/yr
Dec.: −10.925[2] mas/yr
Parallax (π)1.7436±0.0666 mas[2]
Distance1,870 ± 70 ly
(570 ± 20 pc)
Position (relative to KOI-5A)[3]
ComponentKOI-5B
Epoch of observation2016
Angular distance0.029±0.050
Position angle142.1±1.0°
Projected separation16[citation needed] AU
Position (relative to KOI-5A)[3]
ComponentKOI-5C
Epoch of observation2016
Angular distance0.141±0.050
Position angle304.3±2.2°
Projected separation78[citation needed] AU
Details[5]
KOI-5A
Mass1.13[6] M
Radius1.840±0.017 R
Luminosity3.86±0.17 L
Surface gravity (log g)4.19[7] cgs
Temperature5861[7] K
Age3.49±0.41 Gyr
KOI-5B
Mass1.09[6] 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.[3] KOI-5 A and B orbit each other every 29 years, and KOI-5 C orbits stars A and B every 400 years.[6] KOI-5C is physically associated with the core stellar pair with probability 99.98%.[8]

Planetary system

[edit | edit source]

Two planets orbiting one of KOI-5's stars were suspected since 2009 based on Kepler data, but 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.[6][9] 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.[10]

The KOI-5A planetary system[8][6][10]
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

[edit | edit source]
  1. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). Constellation record for this object at VizieR.
  2. ^ a b c d e f Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). Gaia DR3 record for this source at VizieR.
  3. ^ a b c d Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  4. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  5. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  6. ^ a b c d e AT LAST! CONFIRMATION OF KEPLER'S SECOND PLANETARY CANDIDATE
  7. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  8. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  9. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  10. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).