Planet HU Aqr (AB) c

Detailed information about planet HU Aqr (AB) c and its parameters.

Planet

Name
HU Aqr (AB) c
Planet Status
Candidate
Discovered in
2011
Update
2021-10-05
Mass
5.9 ( +0.1 -0.1 ) MJ
Mass*sin(i)
Semi-Major Axis
Orbital Period
Eccentricity
ω
Tperi
Radius
Inclination
Detection Method
Timing
Mass Meas. Method
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
Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference

2015 : The (O-C) may be also driven by oscillations of the gravitational quadrupole moment of the secondary, as predicted by the Lanza et al. modification of the Applegate mechanism. Gozdziewski et al. (2015), 21 May 2012: A previous orbital solution for the timing variations of the eclipses of HU Aqr(AB) led to two planets (Qian et al. 2011). A re-analysis by Gozdziewski et al. (2012), based on new data concludes that a better fit is obtained by a single circumbinary planet, here designated as HU Aqr(AB)b.
02 Dec 2011: Planet validated by new data fitting (Hinse et al. 2012)
13 Oct 2011: The planet parameters result from one of the models by Wittenmyer et al. (2011). According to these authors, "the improved orbital parameters correspond to planets that are dynamically unstable on unfeasibly short timescales (of order 104 years or less). Given these results, the observed signal might in fact be the result of the intrinsic properties of the eclipsing polar".

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Star

Name
HU Aqr (AB)
Distance
Spectral type
Catac. var.
Apparent magnitude V
15.0
Mass
Age
Effective temperature
Radius
Metallicity [Fe/H]
Detected Disc
Magnetic Field
RA2000
21:07:58.0
Dec2000
-05:17:41.0
Alternate Names

02 Dec 2011: HU Aqr(ab) is an eclipsing binary with a period 0.0868204066 ± 0.0000000014) day (Hinse et al. 2012)

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