T Chamaeleontis
| Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
|---|---|
| Constellation | Chamaeleon |
| Right ascension | 11h 57m 13.52451s[2] |
| Declination | −79° 21′ 31.5305″[2] |
| Apparent magnitude (V) | 10.05 - 14.50[3] |
| Characteristics | |
| Evolutionary stage | T Tauri star[4] |
| Spectral type | K0e[5] |
| U−B color index | +0.63[6] |
| B−V color index | +1.14[6] |
| J−K color index | +1.67[7] |
| Variable type | Orion variable[8] |
| Astrometry | |
| Radial velocity (Rv) | 13.8±0.1[9] km/s |
| Proper motion (μ) | RA: −41.586 mas/yr[2] Dec.: −8.655 mas/yr[2] |
| Parallax (π) | 9.7356±0.0332 mas[2] |
| Distance | 335 ± 1 ly (102.7 ± 0.4 pc) |
| Absolute magnitude (MV) | +6.55[10] |
| Details | |
| Mass | 0.65[11] M☉ |
| Radius | 0.65±0.09[12] R☉ |
| Luminosity | 0.29[13] L☉ |
| Surface gravity (log g) | 4.50[13] cgs |
| Temperature | 5,111[14] K |
| Metallicity [Fe/H] | +0.09±0.15[15] dex |
| Rotational velocity (v sin i) | 39±3[16] km/s |
| Age | 12.7[17] Myr |
| Other designations | |
| T Cha, HIP 58285, TYC 9419-1187-1, GSC 09419-01187, 2MASS J11571348-7921313 | |
| Database references | |
| SIMBAD | data |
T Chamaeleontis (T Cha), also known as HIP 58285, is a T Tauri star located in the southern circumpolar constellation Chamaeleon. It has an apparent magnitude that ranges from 10.05 to 14.50,[3] which is below the limit for naked eye visibility. Gaia DR3 parallax measurements place the object 335 light years away[2] and it is currently receding with a heliocentric radial velocity of 13.8 km/s.[9] At its current distance, T Cha's average brightness is diminished by 0.31 magnitudes due to extinction from interstellar dust. It has an average absolute magnitude of +6.55.[10]
History
[edit | edit source]The object was first suspected to be a RW Aurigae-type star in 1949.[18] It was categorized as a T-Tauri star in 1975. In the same year, it was suspected to be variable and the variability was confirmed in 1976.[19] A 1993 paper said that it might be a weak-lined YY Orionis star.[20] T Cha might be either a member of the young ε Chamaeleontis association or the slightly older η Chamaeleontis association.[17][9] T Cha is an Orion variable that fluctuates between 10.05 and 14.5.[3][8]
Physical characteristics
[edit | edit source]T Cha has a stellar classification of K0e,[5] indicating that it is a K-type star with emission lines in its spectrum. It is currently on the T Tauri stage,[4] accreting matter at a rate of 3.16×10−9 to 1.26×10−8 M☉/yr.[21] It has 65% the mass of the Sun[11] but the radius is highly uncertain. Estimates range from 0.65 to 4.36 times the radius of the Sun.[22][12] It radiates 29% the luminosity of the Sun[13] from its photosphere at an effective temperature of 5,111 K,[14] giving it an orange hue. T Cha has a poorly constrained metallicity of [Fe/H] = +0.09[15] and it spins modestly with a projected rotational velocity of 39 km/s.[16]
References
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- ^ a b c d e Lua error in Module:Citation/CS1/Configuration at line 2172: attempt to index field '?' (a nil value). Gaia DR3 record for this source at VizieR.
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