Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Telescopium |
Right ascension | 18h 58m 27.79251s[1] |
Declination | −52° 56′ 19.1999″[1] |
Apparent magnitude (V) | 4.84±0.01[2] |
Characteristics | |
Spectral type | B9.5 IV/V[3] or B9 III[4] |
B−V color index | −0.05[5] |
Astrometry | |
Radial velocity (Rv) | −2±4.2[6] km/s |
Proper motion (μ) | RA: +13.365 mas/yr[1] Dec.: −8.805 mas/yr[1] |
Parallax (π) | 6.6117 ± 0.1718 mas[1] |
Distance | 490 ± 10 ly (151 ± 4 pc) |
Absolute magnitude (MV) | −1.51[7] |
Details | |
Mass | 2.81+0.36 −0.38[8] M☉ |
Radius | 5.53±0.28[9] R☉ |
Luminosity | 260+13 −12[1] L☉ |
Surface gravity (log g) | 3.56[10] cgs |
Temperature | 10,139[11] K |
Metallicity [Fe/H] | +0.19[11] dex |
Rotational velocity (v sin i) | 110[12][13] km/s |
Age | 268[14] Myr |
Other designations | |
Database references | |
SIMBAD | data |
λ Telescopii, Latinized as Lambda Telescopii, is a solitary,[17] bluish-white hued star located in the southern constellation of Telescopium. It has an apparent magnitude of 4.84,[2] making it readily visible to the naked eye under ideal conditions. Gaia DR3 parallax measurements imply a distance of 490 light years,[1] and it is currently approaching the Solar System with a somewhat constrained heliocentric radial velocity of −2 km/s.[6] At its current distance, the visual magnitude of Lambda Telescopii is diminished by an extinction of 0.25 due to interstellar dust[18] and it has an absolute magnitude of −1.51.[7]
The object has been given several stellar classifications over the years. Lambda Telescopii has been classified as B9 III (evolved giant star),[4] A0 V (A-type main-sequence star),[13] and B9 .5 IV/V.[3]
The accepted classification for Lambda Telescopii is B9.5 IV/V,[3] indicating that it is a late B-type star with the blended luminosity class of a subgiant and a main sequence star. Gaia DR3 stellar evolution models place it near the end of its main sequence lifetime.[1] The star is 268 million years old[14] with a relatively high rate of spin, showing a projected rotational velocity of 110 km/s.[12][13] Lambda Telescopii is metal enriched with an iron abundance 155% that of the Sun, or [Fe/H] = +0.19.[11] The star has 2.81 times the mass of the Sun[8] and it radiates 260 times the luminosity of the Sun[1] from its photosphere – which is 5.53 times the size of the Sun's – at an effective temperature of 10,193 K.[9] [11]
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