HD 11964

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HD 11964
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Cetus
Right ascension 01h 57m 09.6074s[1]
Declination −10° 14′ 32.7318″[1]
Apparent magnitude (V) 7.51[2]
Characteristics
Spectral type G9VCN+1[3][2] + M0.0Ve[4]
Apparent magnitude (U) 7.705[citation needed]
Apparent magnitude (B) 8.117[2]
Apparent magnitude (R) 5.960[citation needed]
Apparent magnitude (I) 6.914[2]
Apparent magnitude (J) 6.508±0.019[2]
Apparent magnitude (H) 6.265±0.031[2]
Apparent magnitude (K) 6.168±0.017[2]
U−B color index 0.450
B−V color index 0.607±0.015[2]
V−R color index 0.455
R−I color index 0.405
Variable type Suspected[citation needed]
Distance
109.5 ± 0.1 ly
(33.57 ± 0.04 pc)
Absolute magnitude (MV)3.84[2]
Details
A
dex
HIP 9094, SAO 148123, WDS 01572-1015[9]
Database references
Exoplanet Archive
data
ARICNSdata

HD 11964 is a

extrasolar planets
have been confirmed to orbit the primary.

Properties

The primary, component A, is a

A wide

along a position angle of 134°, as of 2015.[12] It is a red dwarf with a class of M0V,[4] and has just 0.6 times the Sun's radius. It is radiating 0.085 times the Sun's luminosity at an effective temperature of 4,033 K.[1]

Planetary system

In August 2005, two planets were discovered orbiting the star, the innermost like Neptune and another like Jupiter orbiting at 3.34 AU. However, the second planet (

The HD 11964 planetary system[14]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
c ≥ 0.11 MJ 0.229 37.82 0.15
b ≥ 0.61±0.1 MJ 3.34±0.4 2,110±70 0.06±0.2

See also

  • HD 11977
  • List of extrasolar planets

References

External links