HD 11928

Last updated
HD 11928
Triangulum constellation map.svg
Red circle.svg
Location of HD 11928 on the map (circled)
Observation data
Epoch J2000.0        Equinox J2000.0 (ICRS)
Constellation Triangulum
Right ascension 01h 57m 43.74417s [1]
Declination +27° 48 15.7579 [1]
Apparent magnitude  (V)5.84 - 5.85 [2]
Characteristics
Evolutionary stage AGB [3]
Spectral type M2 III [4]
B−V color index +1.60 [5]
Variable type suspected [2]
Astrometry
Radial velocity (Rv)−1.93±0.22 [6]  km/s
Proper motion (μ)RA: +12.974  mas/yr [1]
Dec.: −60.043  mas/yr [1]
Parallax (π)6.1432 ± 0.1953  mas [1]
Distance 530 ± 20  ly
(163 ± 5  pc)
Absolute magnitude  (MV)+0.11 [7]
Details
Radius 52.68 [8]   R
Luminosity 485±17 [9]   L
Surface gravity (log g)1.024 [10]   cgs
Temperature 3,656±72 [11]   K
Other designations
NSV  15408, AG+27°211, BD+27°310, GC  2357, HD  11928, HIP  9132, HR  564, SAO  75048 [12]
Database references
SIMBAD data

HD 11928 (HR 564; NSV 15408) is a solitary star [13] located in the northern constellation of Triangulum. It is faintly visible to the naked eye as a red-hued point of light with an apparent magnitude of 5.85. [14] Gaia DR3 parallax measurements imply a distance of 530 light-years and it is drifting closer with a heliocentric radial velocity of −1.93  km/s . [6] At its current distance, HD 11928's brightness is diminished by an interstellar extinction of 0.13 magnitudes [15] and it has an absolute magnitude of +0.11. [7]

HD 11928 has a stellar classification of M2 III, [4] indicating that is an evolved M-type giant star. It is currently an asymptotic giant branch star that is generating energy via the fusion of hydrogen and helium shells around an inert carbon core. At present it has expanded to 52.68 times the radius of the Sun [8] and it radiates 485 times the luminosity of the Sun [9] from its photosphere at an effective temperature of 3,656  K . [11]

In 1997, the Hipparcos satellite observed that the star varied from 5.89 to 5.93 in the Hipparcos passband. [16] Further observations from Koen & Eyer reveal that HD 11928 flucates between 5.84 and 5.85 in the visual passband within 50.7 days. [17] As of 2004 however, its variability has not been confirmed, [18] but it is still suspected to be variable.

Related Research Articles

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<span class="mw-page-title-main">14 Trianguli</span> Star in the constellation Triangulum

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HD 208741, also known as HR 8380, is a yellowish-white hued star located in the southern circumpolar constellation Octans. It has an apparent magnitude of 5.91, making it faintly visible to the naked eye. Parallax measurements place it at a distance of 211 light years, and it is currently receding with a heliocentric radial velocity of 8 km/s.

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<span class="mw-page-title-main">AF Columbae</span> Star in the constellation of Columba

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<span class="mw-page-title-main">HD 40091</span> Star in the constellation Columba

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<span class="mw-page-title-main">HD 197630</span> Star in the constellation of Microscopium

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<span class="mw-page-title-main">HD 168592</span> Star in the constellation of Corona Australis

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<span class="mw-page-title-main">HD 175219</span> K-type giant; Corona Australis

HD 175219, also known as HR 7122, is a solitary, orange hued star located in the southern constellation Corona Australis. It has an apparent magnitude of 5.35, allowing it to be faintly visible to the naked eye. The object is located relatively close at a distance of 314 light years based on Gaia DR3 parallax measurements but is drifting closer with a heliocentric radial velocity of −21.1 km/s. At its current distance, HD 175219's brightness is diminished by 0.26 magnitudes due to interstellar dust. It has an absolute magnitude of +0.57.

<span class="mw-page-title-main">HD 196917</span> Suspected variable star in Microscopium

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References

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