13 Trianguli

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13 Trianguli
Observation data
Epoch J2000      Equinox J2000
Constellation Triangulum
Right ascension 02h 28m 48.49387s[1]
Declination +29° 55′ 54.3315″[1]
Apparent magnitude (V) 5.86[2]
Characteristics
Spectral type G0 V[1]
U−B color index +0.01[2]
B−V color index +0.58[2]
Astrometry
Radial velocity (Rv) +40.8[3] km/s
Proper motion (μ) RA: –66.53[1] mas/yr
Dec.: +71.93[1] mas/yr
Parallax (π) 31.84 ± 0.40[1] mas
Distance 102 ± 1 ly
(31.4 ± 0.4 pc)
Absolute magnitude (MV) 3.45[4]
Details
Mass 1.10 ± 0.03[4] M
Luminosity 3.72[4] L
Temperature 5,846[4] K
Metallicity [Fe/H] –0.24[5] dex
Rotational velocity (v sin i) 3[6] km/s
Age 6.45[4] Gyr
Other designations
13 Her, BD+29 423, GJ 99.1, HD 15335, HIP 11548, HR 720, SAO 75391.[2]

13 Trianguli is the Flamsteed designation for a star in the northern constellation of Triangulum. It has an apparent visual magnitude of 5.86,[2] so according to the Bortle scale it is faintly visible from dark suburban skies. Measurements made with the Hipparcos spacecraft show an annual parallax shift of 0.03184″,[1] which is equivalent to a distance of around 102 ly (31 pc) from the Sun.

A stellar classification of G0 V[1] indicates this is a main sequence star that is generating energy by fusing hydrogen into helium at its core. It has about 110% of the Sun's mass and shines with 3.72 times the luminosity of the Sun. The stellar atmosphere has an effective temperature of 5,846[4] K, giving it the yellow hue of a G-type star.[7] It appears to be older than the Sun, with an estimated age of 6.45 billion years.[4]

In 1994, an astrometric companion was reported at an angular separation of 0.020″. However, follow-up observations reported in 2005 not only failed to recover this object but also returned a null result on a search for planetary companions.[8] The star has been examined for an infrared excess that could indicate the presence of an orbiting debris disk, but no such excess was found.[5]

References

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Coordinates: Sky map 02h 28m 48.49s, +29° 55′ 54.33″