Delta Trianguli

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Delta Trianguli
Diagram showing star positions and boundaries of the Triangulum constellation and its surroundings
Cercle rouge 100%.svg

Location of δ Trianguli (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Triangulum
Right ascension 02h 17m 03.23016s[1]
Declination +34° 13′ 27.2260″[1]
Apparent magnitude (V) +4.865[2]
Characteristics
Spectral type G0V / G9V to K4V[3]
U−B color index +0.02[4]
B−V color index +0.61[4]
Astrometry
Radial velocity (Rv) −5.70[5] km/s
Proper motion (μ) RA: 1151.83[1] mas/yr
Dec.: −246.89[1] mas/yr
Parallax (π) 92.73 ± 0.39[1] mas
Distance 35.2 ± 0.1 ly
(10.78 ± 0.05 pc)
Absolute magnitude (MV) 4.69[2]
Details
Mass 1.0/0.8[6] M
Radius 0.98[7] R
Surface gravity (log g) 4.5[8] cgs
Temperature 6,215/4,493[3] K
Metallicity [Fe/H] −0.39[2] to −0.30[8] dex
Rotational velocity (v sin i) 10.00[5] km/s
Age 8.5[9] to 9.0[2] Gyr
Orbit[10]
Companion Delta Trianguli B
Period (P) 10.0200 days
Semi-major axis (a) 9.80 ± 0.06 mas
Eccentricity (e) 0.020 ± 0.005
Inclination (i) 167 ± 3°
Longitude of the node (Ω) 15 ± 9°
Other designations
δ Trianguli, δ Tri, Delta Tri, 8 Trianguli, BD+33°395, Gliese 92, HD 13974, HIP 10644, HR 660, LFT 198, LHS 154, LTT 10770, SAO 55420.[11]

Delta Trianguli (Delta Tri, δ Trianguli, δ Tri) is a spectroscopic binary star system approximately 35 light-years (11 pc) away in the constellation of Triangulum. The primary star is a yellow dwarf, while the secondary star is thought to be an orange dwarf. It has an apparent magnitude of +4.87 and forms an optical (line-of-sight) triple with Gamma Trianguli and 7 Trianguli.[6]

Stellar components

Delta Trianguli A is a main sequence star with a stellar classification of G0V and a mass similar to the Sun.[6] The spectral characteristics of the smaller companion Delta Trianguli B are not well determined since the close orbit makes observations difficult,[12] with estimates of the spectral class ranging from G9V to K4V.[3] The Delta Trianguli stars orbit their center of mass with an estimated separation of 0.106 AU;[6] it is certainly less than one AU.[3] The orbital period is 10.02 days and the eccentricity of the orbit is only 0.020. The orbit is inclined about 167° to our line of sight.[10]

A 2008 search for a tertiary companion to this system using an adaptive optics system on the VLT proved unsuccessful.[13] Examination of the system in infrared light at 70 μm shows no excess emission that would otherwise indicate the presence of a disk of orbiting dust.[3]

Naming

In Chinese, 天大將軍 (Tiān Dà Jiāng Jūn), meaning Heaven's Great General, refers to an asterism consisting of δ Trianguli γ Andromedae, φ Persei, 51 Andromedae, 49 Andromedae, χ Andromedae, υ Andromedae, τ Andromedae, 56 Andromedae, β Trianguli and γ Trianguli. Consequently, δ Trianguli itself is known as 天大將軍十一 (Tiān Dà Jiāng Jūn shíyī, English: the Eleventh Star of Heaven's Great General.).[14]

See also

References

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  14. (Chinese) AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 10 日

External links

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