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Mu2 Octantis
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Mu2 Octantis
Mu2 Octantis
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Octans
μ2 Oct A
Right ascension 20h 41m 44.102s[1]
Declination −75° 21′ 02.88″[1]
Apparent magnitude (V) +6.481±0.007[2]
μ2 Oct B
Right ascension 20h 41m 45.5181s[3]
Declination −75° 20′ 47.047″[3]
Apparent magnitude (V) +7.153±0.011[2]
Characteristics
μ2 Oct A
Spectral type G1V[4]
U−B color index +0.26[5]
B−V color index +0.62[5]
μ2 Oct B
Spectral type G1V[6]
Astrometry
μ2 Oct A
Radial velocity (Rv)−10.90±0.2[7] km/s
Proper motion (μ) RA: 156.404 mas/yr[1]
Dec.: −162.214 mas/yr[1]
Parallax (π)25.0327±0.0205 mas[1]
Distance130.3 ± 0.1 ly
(39.95 ± 0.03 pc)
Absolute magnitude (MV)3.28[4]
μ2 Oct B
Radial velocity (Rv)−10.94±0.15[3] km/s
Proper motion (μ) RA: +163.531 mas/yr[3]
Dec.: −171.346 mas/yr[3]
Parallax (π)25.0379±0.0167 mas[3]
Distance130.27 ± 0.09 ly
(39.94 ± 0.03 pc)
Orbit[4]
Semi-major axis (a)932 AU
Details[8]
μ2 Oct A
Mass1.330±0.013 M
Radius1.730+0.044
−0.039
 R
Luminosity3.73[4] L
Surface gravity (log g)4.24±0.03[4] cgs
Temperature6,059±52 K
Metallicity [Fe/H]+0.216±0.009 dex
Rotation22.5±2.9[9] days
Rotational velocity (v sin i)1.45[4] km/s
Age3.50+0.65
−0.27
 Gyr
μ2 Oct B
Mass1.190+0.017
−0.018
 M
Radius1.190+0.034
−0.010
 R
Temperature6,020±52 K
Metallicity [Fe/H]+0.267±0.009 dex
Age2.10+1.03
−0.34
 Gyr
Other designations
μ2 Oct, CCDM J20417-7521
μ2 Oct A: CD−75°1173, HD 196067, HIP 102125, HR 7864, SAO 257836, 2MASS J20414409-7521029
μ2 Oct B: CD−75°1174, HD 196068, HIP 102128, SAO 257837, 2MASS J20414550-7520471
Database references
A
SIMBADdata
Exoplanet Archivedata
Database references
B
SIMBADdata

Mu2 Octantis2 Oct) is a binary star system in the constellation Octans, whose primary and secondary stars have apparent magnitudes of +6.481 and 7.153, respectively.[2] Based on parallax measurements, it lies 130.3 light-years away.[1][3]

The two stars, HD 196067 and HD 196068 (also named μ2 Oct A and μ2 Oct B), are separated at 17 arcseconds in the sky, corresponding to 740 astronomical units (AU). The semimajor axis of the stars' orbit is 932 AU.[4]

Component A is a G-dwarf star with 1.33 and 1.73 times of the Sun's mass and radius, respectively. Component B also a G-type main-sequence star with a radius 1.19 times larger than the Sun. Their effective temperatures are similar. HD 196068 has a higher metallicity than its companion, the reasons for this are uncertain.[8]

Planetary system

[edit]

From 1998 to 2012, the system was observed using the CORALIE instrument, at the ESO's La Silla Observatory.[4]

In November 2012, a long-period, wide-orbiting planet was deduced by radial velocity around HD 196067. The planet has been pulled to an eccentric orbit by the B star HD 196068. The planet's true mass, as measured by astrometry, is 12.5 MJ, placing it right on the traditionally adopted boundary between planets and brown dwarfs.[10]

A second, innermost planet was detected using radial velocity observations with the CORALIE, HARPS, and ESPRESSO observatories. Despite its small orbit, it does not transit the host star.[9]

The μ2 Oct A planetary system[9]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
c ≥10.4±1.4 M🜨 4.601088±0.000192 0.24±0.12
b 12.5+2.5
−1.8
[10] MJ
5.10+0.22
−0.17
[10]
3,413.7±10.5 0.56292±0.00703 41.2+28
−9.1
[10]°

References

[edit]
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