Planet DQ Her (AB)b

Detailed information about planet DQ Her (AB)b and its parameters.

Planet

Name
DQ Her (AB)b
Planet Status
Candidate
Discovered in
2009
Publication
Status
—
Update
2024-06-21
Mass
Mass*sin(i)
—
Semi-Major Axis
Orbital Period
Eccentricity
0.0
Angular distance
0.03245 arcsec
ω
—
Tperi
—
Radius
—
Inclination
Detection Method
Other
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

09 Feb 2011: The candidate DQ Her(ab)c is suggested by Dai & Qian (2009) as a plausible explanation of the periodic variations of the eclipses of DQ Her(ab). The mass value is given by assuming that the 3rd body orbit is coplanar with the DQ Her(ab) orbit inclined by 86.5 deg.

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Star

Name
DQ Her (AB)
Distance
200.0 pc
Spectral type
Nova
Apparent magnitude V
15.16
Apparent magnitude I
—
Apparent magnitude J
—
Apparent magnitude H
—
Apparent magnitude K
—
Mass
Age
—
Effective temperature
—
Radius
—
Metallicity [Fe/H]
—
Detected Disc
—
Magnetic Field
—
RA2000
18:07:30.0
Dec2000
+45:51:33.0
Alternate Names
—

09 Feb 2011: DQ Her (ab) is an eclipsing binary with masses 0.4 and 0.8 mSun and period 4h39m. (Dai & Qian 2009). Following Beuermann et al. (2010) for the designation of the binary NN ser, we designated the two components by a and b and the binary by (ab).

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