Delta Trianguli

Delta Trianguli

Template:Location mark Location of δ Trianguli (circled)
Observation data Epoch J2000.0      Equinox J2000.0
Constellation	Triangulum
Right ascension	Template:RA
Declination	Template:DEC
Apparent magnitude (V)	+4.865
Characteristics
Spectral type	G0V + G9V to K4V
U−B Template:Engvar	+0.02
B−V Template:Engvar	+0.61
Astrometry
Radial velocity (Rv)	−5.70 km/s
Proper motion (μ)	RA: 1151.83 mas/yr Dec.: −246.89 mas/yr
Parallax (π)	92.73±0.39 mas
Distance	Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)	4.69
Details
A
Mass	Template:Val Template:Solar mass
Radius	0.98 Template:Solar radius
Surface gravity (log g)	4.5 cgs
Temperature	6,215 K
Metallicity [Fe/H]	−0.39 to −0.30 dex
Rotational velocity (v sin i)	10.00 km/s
Age	8.5 to 9.0 Gyr
B
Mass	Template:Val Template:Solar mass
Temperature	4,493 K
Metallicity [Fe/H]	{{{metal_fe2}}} dex
Other designations
Template:Odlist
Database references
SIMBAD	data

Delta Trianguli, also named Deltoton, is a spectroscopic binary star system approximately Template:Convert 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.

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. 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. The name was chosen for this star because of the "obvious pun" in that its Bayer designation is Delta.

In Chinese, (), 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 (, Template:Langx).

Stellar components

Delta Trianguli A is a main sequence star with a stellar classification of G0V and a mass similar to the Sun. The spectral characteristics of the smaller companion Delta Trianguli B are not well determined since the close orbit makes observations difficult, with estimates of the spectral class ranging from G9V to K4V. The Delta Trianguli stars orbit their center of mass with an estimated separation of 0.106 AU; it is certainly less than one AU. 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.

A 2008 search for a tertiary companion to this system using an adaptive optics system on the VLT proved unsuccessful. 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.

See also

• V4046 Sagittarii