Planet V4046 Sgr (AB)c

Detailed information about planet V4046 Sgr (AB)c and its parameters.

Planet

Name
V4046 Sgr (AB)c
Planet Status
Candidate
Discovered in
2019
Publication
Status
Published in a refereed paper
Update
2025-08-19
Mass
Mass*sin(i)
Semi-Major Axis
Orbital Period
Eccentricity
Angular distance
ω
Tperi
Radius
Inclination
Detection Method
Other
Mass Meas. Method
Theoretical
Radius Meas. Method
Primary transit
Secondary transit
λ
Impact Parameter b
Time Vr=0
Velocity Semiamplitude K
Calculated temperature
Measured temperature
Hottest point longitude
Geometric albedo
Surface gravity log(g/gH)
Alternate Names
HD 319139 (AB)c
Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference

Ruiz-Rodriguez et al. (2019): An inner ring may indicate the presence of a second circumbinary planet in the system, interior to 15 au.
Weber et al. (2022) deem very likely the presence of two planets at 9 and 20 AUs.

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Star

Name
V4046 Sgr (AB)
Distance
Spectral type
K5+K7
Apparent magnitude V
10.7
Apparent magnitude I
Apparent magnitude J
Apparent magnitude H
Apparent magnitude K
Mass
Age
Effective temperature
Radius
Metallicity [Fe/H]
Detected Disc
Imaging
Magnetic Field
RA2000
18:14:10.0
Dec2000
-32:47:34.0
Alternate Names
HD 319139

Eclipsing binary (P = 2.42 d) with m1 = 0.9 ± 0.05 MSol, r1 = 1.64 RSol, T1 = 4350 K and m2 = 0.85 ± 0.04 MSol, r2 = 1.033 RSol, T2 = 4060 K. Separation about 0.041 AUs.
A massive (0.1 MSol), 300 AU-wide circumbinary disk with gaps and rings shaped by forming planets surrounds the close binary (Martinez-Brunner et al. 2022).
V4046 Sgr is also part of a triple or quadruple system including GSC 07396-00759 (spT M1e), about 2.82 arcseconds away (~12,350 AUs), itself likely spectroscopic binary with nearly equal components and it too hosting an edge-on debris disk as large as 70 AUs (Kastner et al. 2011).

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