HD 191220

Last updated
HD 191220
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Octans
Right ascension 20h 24m 54.91771s [1]
Declination −83° 18 38.2301 [1]
Apparent magnitude  (V)6.14±0.01 [2]
Characteristics
Spectral type A2/3 mA8-F0 [3]
U−B color index +0.13 [4]
B−V color index +0.20 [4]
Astrometry
Radial velocity (Rv)0.1±1.3 [5]  km/s
Proper motion (μ)RA: +23.223  mas/yr [1]
Dec.: +6.228  mas/yr [1]
Parallax (π)13.331 ± 0.0247  mas [1]
Distance 244.7 ± 0.5  ly
(75.0 ± 0.1  pc)
Absolute magnitude  (MV)+1.76 [6]
Details
Mass 2.06±0.40 [7]   M
Radius 2.17±0.06 [8]   R
Luminosity 15.57 [9]   L
Surface gravity (log g)4.12±0.06 [10]   cgs
Temperature 7,706±126 [11]   K
Metallicity [Fe/H]−0.02 [12]   dex
Age 979±166 [1]   Myr
Other designations
45 G. Octantis [13] , CD−83°253, CPD−83°695, GC  28176, HD  191220, HIP  100697, HR  7698, SAO  258856 [14]
Database references
SIMBAD data

HD 191220, also known as HR 7698, is a solitary white hued star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 6.14, [2] placing it near the limit for naked eye visibility. The object is located relatively close at a distance of 245 light years based on Gaia DR3 parallax measurements [1] but is slowly receding with a heliocentric radial velocity of 0.1  km/s . [5] At its current distance, HD 191220's brightness is diminished by 0.22 magnitudes due to interstellar dust. [15]

This is a chemically peculiar Am star [16] with a stellar classification of A2/3mA8-F0, [3] an A-type star with the metallic lines of a star with a class of A8-F0. It has double the mass of the Sun and 2.2 times its girth. [7] It radiates 15.57 times the luminosity of the Sun [9] from its photosphere at an effective temperature of 7,706  K . [11] HD 191220 is estimated to be nearly a billion years old [12] and has a near solar metallicity — what astronomers dub a star's abundance of chemical elements heavier than helium. [12]

Related Research Articles

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<span class="mw-page-title-main">HD 98617</span> Double star in the constellation Chamaeleon

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HD 43899, also designated as HR 2263, is a solitary, orange hued star located in the southern constellation Columba, the dove. It has an apparent magnitude of 5.53, allowing it to be faintly visible to the naked eye. Based on parallax measurements from the Gaia spacecraft, the object is estimated to be 284 light years distant. It appears to be rapidly receding with a heliocentric radial velocity of 66.5 km/s. Eggen (1993) lists HD 43899 as an old disk star and its kinematics match with that of the ζ Herculis moving group.

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References

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