Planet HII 1348 (AB)b

Detailed information about planet HII 1348 (AB)b and its parameters.

Planet

Name
HII 1348 (AB)b
Planet Status
Confirmed
Discovered in
2012
Publication
Status
—
Update
2026-03-31
Mass
Mass*sin(i)
—
Semi-Major Axis
Orbital Period
—
Eccentricity
Angular distance
—
ω
Tperi
—
Radius
—
Inclination
Detection Method
Imaging
Mass Meas. Method
Spectrum
Radius Meas. Method
—
Primary transit
—
Secondary transit
—
λ
—
Impact Parameter b
—
Time Vr=0
—
Velocity Semiamplitude K
25.85 ( ± 0.334 ) m/s
Calculated temperature
—
Measured temperature
—
Hottest point longitude
—
Geometric albedo
—
Surface gravity log(g/gH)
—
Alternate Names
HII 1348 b
Data Source Type Result Value Result Figure Notes Reference
Molecule Data Source Type Result Value Result Figure Notes Reference

Spectral type M8. L = 7.24e-04 LSol (Geissler et al. 2012).

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Star

Name
HII 1348 (AB)
Distance
Spectral type
K5V+K5V
Apparent magnitude V
12.8
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
03:47:18.0
Dec2000
+24:23:27.0
Alternate Names
Cl Melotte 22 1348, BOV 18

HII 1348 is a highly eccentric double-lined spectroscopic binary (P = 94.805 d, e = 0.5543) with a nearly identical companion star (Queloz et al. 1998, Torres et al. 2021) and an outer circumbinary substellar companion. A third M dwarf companion star (HII 1348 C) lies 5155 AUs away and the triple system is in turn orbited by an additional, outer substellar object (HII 1348 D or (ABC)b).

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