Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Telescopium |
Right ascension | 19h 35m 12.98634s[1] |
Declination | −48° 05′ 57.1238″[1] |
Apparent magnitude (V) | 4.88±0.01[2] |
Characteristics | |
Spectral type | K0 III[3] |
B−V color index | +1.09[4] |
Astrometry | |
Radial velocity (Rv) | +22.3±0.8[5] km/s |
Proper motion (μ) | RA: −8.190 mas/yr[1] Dec.: −36.977 mas/yr[1] |
Parallax (π) | 8.6546 ± 0.1055 mas[1] |
Distance | 377 ± 5 ly (116 ± 1 pc) |
Absolute magnitude (MV) | −0.39[6] |
Details | |
Mass | 2.53±0.19[7] M☉ |
Radius | 19.7±1.0[8] R☉ |
Luminosity | 172+5 −4[1] L☉ |
Surface gravity (log g) | 1.88[9] cgs |
Temperature | 4,738±55[7] K |
Metallicity [Fe/H] | +0.01±0.04[7] dex |
Rotational velocity (v sin i) | 1.8±1.3[10] km/s |
Other designations | |
Database references | |
SIMBAD | data |
ι Telescopii, Latinized as Iota Telescopii and abbreviated Iota Tel, is a solitary star[13] located in the southern constellation Telescopium. It is faintly visible to the naked eye as an orange-hued star with an apparent visual magnitude of +4.88.[2] The star is located roughly 377 light years distant from the Solar System based on Gaia DR3 parallax measurements[1] and it is receding with a radial velocity of 22.3 km/s.[5] At its current distance, Iota Tel's brightness is diminished by 0.19 magnitudes[14] due to interstellar dust and it has an absolute magnitude of −0.39.[6]
This object is an aging red giant star with a stellar classification of K0 III.[3] At present it has 2.53 times the mass of the Sun,[7] but it has expanded to 19.7 times the radius of the Sun.[8] It is radiating 172 times the Sun's luminosity[1] from its swollen photosphere at an effective temperature of 4,738 K.[7] Iota Tel has a near solar metallicity at [Fe/H] = +0.01[7] and it spins slowly with a projected rotational velocity of 1.8 km/s.[10]
GaiaDR3
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was invoked but never defined (see the help page).De Medeiros2014
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was invoked but never defined (see the help page).SIMBAD
was invoked but never defined (see the help page).Eggleton2008
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