Delta Trianguli
Binary star in the constellation Triangulum
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Delta Trianguli, (also named Deltoton for component A),[12] 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.[13]
 | |
| 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 mas[1] |
| Distance | 35.2 ± 0.1 ly (10.78 ± 0.05 pc) |
| Absolute magnitude (MV) | 4.69[2] |
| Orbit[6] | |
| Name | Delta Trianguli B |
| Period (P) | 10.02 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° |
| Details | |
| A | |
| Mass | 0.884±0.059[7] M☉ |
| Radius | 0.98[8] R☉ |
| Surface gravity (log g) | 4.5[9] cgs |
| Temperature | 6,215[3] K |
| Metallicity [Fe/H] | −0.39[2] to −0.30[9] dex |
| Rotational velocity (v sin i) | 10.00[5] km/s |
| Age | 8.5[10] to 9.0[2] Gyr |
| B | |
| Mass | 0.785±0.044[7] M☉ |
| Temperature | 4,493[3] K |
| Other designations | |
| Deltoton, δ Tri, Delta Tri, 8 Trianguli, BD+33°395, GJ 92, HD 13974, HIP 10644, HR 660, SAO 55420, LHS 154, LTT 10770[11] | |
| Database references | |
| SIMBAD | data |
Naming
Delta Trianguli, Latinized from δ Trianguli and abbreviated Delta Tri, is the star's Bayer designation.
Deltoton was an ancient Greek name of the constellation Triangulum, so named because the capital Greek letter delta is shaped like a triangle.[14] The IAU Working Group on Star Names approved the name Deltoton for this star on 17 June 2025 and it is now so entered in the IAU Catalog of Star Names.[12] The name was chosen for Delta Trianguli A, because of the "obvious pun" in that its Bayer designation is Delta.[15]
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, the Chinese name for δ Trianguli itself is 天大將軍十一 (Tiān Dà Jiāng Jūn shíyī, English: the Eleventh Star of Heaven's Great General).[16]
Stellar components
Delta Trianguli A is a main sequence star with a stellar classification of G0V and a mass similar to the Sun.[13] The spectral characteristics of the smaller companion Delta Trianguli B are not well determined since the close orbit makes observations difficult,[17] 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;[13] 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 the line of sight from Earth.[6]
A 2008 search for a tertiary companion to this system using an adaptive optics system on the VLT proved unsuccessful.[18] 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]