Epsilon Telescopii

ε Telescopii
Observation data
Epoch J2000.0      Equinox J2000.0 (ICRS)
Constellation Telescopium
Right ascension 18h 11m 13.7612s
Declination −45° 57 15.882
Apparent magnitude (V) 4.50±0.01
Characteristics
Evolutionary stage red giant branch
Spectral type K0 III
U−B color index +0.78
B−V color index +1.01
Astrometry
Radial velocity (Rv)−26.3±0.8 km/s
Proper motion (μ) RA: −18.837 mas/yr
Dec.: −38.102 mas/yr
Parallax (π)8.0405±0.321 mas
Distance410 ± 20 ly
(124 ± 5 pc)
Absolute magnitude (MV)−1.00
Details
Mass3.9 M
Radius20 R
Luminosity256 L
Surface gravity (log g)2.32±0.12 cgs
Temperature4,996±42 K
Metallicity [Fe/H]−0.07±0.04 dex
Rotational velocity (v sin i)6.1 km/s
Other designations
ε Tel, CD−45°12251, FK5 1473, HD 166063, HIP 89112, HR 6783, SAO 228777
Database references
SIMBADdata

Epsilon Telescopii, Latinized from ε Telescopii, is a solitary, orange-hued star in the southern constellation of Telescopium. It is visible to the naked eye with an apparent visual magnitude of +4.53. Based upon an annual parallax shift of 7.80 mas as seen from Earth, it is located roughly 410 light years from the Sun, give or take 20 light years.

This an evolved K-type giant with a stellar classification of K0 III. It displays an infrared excess, suggesting the presence of an orbiting disk of dust. The star is radiating 293 times the Sun's luminosity from its photosphere at an effective temperature of 4,996 K. It has a 13th magnitude optical companion at an angular separation of 16.30 arcseconds along a position angle of 233°, as of 2000.