TOI-6883

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TOI-6883
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Delphinus[1]
A
Right ascension 20h 41m 10.067s[2]
Declination +03° 38′ 19.25″[2]
Apparent magnitude (V) 9.48[3]
B
Right ascension 20h 41m 10.300s[4]
Declination +03° 38′ 24.88″[4]
Characteristics
Evolutionary stage Main sequence
Spectral type G
Astrometry
A
Proper motion (μ) RA: -56.677 mas/yr[2]
Dec.: -89.096 mas/yr[2]
Parallax (π)10.6121±0.0154 mas[2]
Distance307.3 ± 0.4 ly
(94.2 ± 0.1 pc)
B
Proper motion (μ) RA: -53.136 mas/yr[4]
Dec.: -101.579 mas/yr[4]
Parallax (π)11.8192±0.1557 mas[4]
Distance276 ± 4 ly
(85 ± 1 pc)
Details[5]
A
Mass1.082+0.055
−0.056
 M
Radius1.086±0.020 R
Luminosity1.168+0.065
−0.063
 L
Surface gravity (log g)4.402+0.013
−0.018
 cgs
Temperature5756+67
−66
 K
Metallicity [Fe/H]0.318±0.058 dex
Age3.8+2.6
−2.1
 Gyr
Other designations
BD+03 4397, TOI-6883
A: TIC 393818343
B: TIC 393818340[6]
Database references
SIMBADA
B
Exoplanet Archivedata

TOI-6883 is a wide visual binary star system located in the constellation of Delphinus, at a distance of approximately 94 parsecs (307 light-years) from Earth. It is composed of two Sun-like stars, TOI-6883A and TOI-6883B, separated by approximately 6.5 arcseconds, corresponding to ~616 astronomical units (AU).

Characteristics

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Both stars are classified as G-type main-sequence stars with masses and radii similar to that of the Sun. According to Conzo et al. 2025,[6] data from the Gaia mission (DR3) show:

  • Nearly identical parallaxes (~10.6 mas)
  • Consistent proper motions
  • A projected separation indicating an orbital period of ~15,300 years

These properties strongly support the idea that the two stars form a gravitationally-bound and dynamically stable binary system.[6]

However, the Gaia DR3 parallaxes and proper motions shown in VizieR differ from those reported by Conzo et al., and may suggest the two stars are at different distances.[4]

Planetary system

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The TOI-6883 system appears to have at least one planet: TOI-6883Ab is a hot Jupiter-type exoplanet orbiting the primary star TOI-6883A with a period of about 16.25 days. The planet was first detected via transit by the Transiting Exoplanet Survey Satellite (TESS) and later confirmed by ground-based photometric observations. Following the confirmation of the binary nature of the host star, the planet’s designation was updated from TOI-6883b to TOI-6883Ab in accordance with IAU naming conventions for multiple stellar systems.[6]

With a radius of ~1.1 Jupiter radii, the planet produces a transit depth of about 1.3%. The presence of the secondary star TOI-6883B may influence the planet’s long-term orbital evolution via dynamical mechanisms such as Kozai–Lidov oscillations.

The TOI-6883A planetary system[5]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b 4.34±0.15 MJ 0.1291+0.0021
−0.0022
16.24921+0.00010
−0.00011
0.6058±0.0023 89.57+0.30
−0.38
°
1.087+0.023
−0.021
 RJ

References

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  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 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. ^ Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  4. ^ a b c d e 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.
  5. ^ a b Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).
  6. ^ a b c d Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value).

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