Gamma Trianguli Australis

From Infogalactic: the planetary knowledge core
Jump to: navigation, search
Gamma Trianguli Australis
Diagram showing star positions and boundaries of the Triangulum Australe constellation and its surroundings
Cercle rouge 100%.svg

Location of γ Trianguli Australis (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Triangulum Australe
Right ascension 15h 18m 54.58198s[1]
Declination –68° 40′ 46.3654″[1]
Apparent magnitude (V) +2.87[2]
Characteristics
Spectral type A1 V[3][4]
U−B color index –0.02[5]
B−V color index +0.00[5]
Astrometry
Radial velocity (Rv) –3.0[2] km/s
Proper motion (μ) RA: –66.58[1] mas/yr
Dec.: –32.31[1] mas/yr
Parallax (π) 17.74 ± 0.12[1] mas
Distance 184 ± 1 ly
(56.4 ± 0.4 pc)
Details
Radius 5.86[6] R
Temperature 9,400[6] K
Rotational velocity (v sin i) 199[4] km/s
Age 260[7] Myr
Other designations
CD–68 1503, FK 560, HD 135382, HIP 74946, HR 5671, SAO 253097.[8]

Gamma Trianguli Australis (γ TrA, γ Trianguli Australis) is a star in the constellation Triangulum Australe. Along with Alpha and Beta Trianguli Australis it forms a prominent triangular asterism that gives the constellation its name (Latin for southern triangle). It is the third brightest member of this constellation with an apparent visual magnitude of +2.87.[2] based upon parallax measurements, Gamma Trianguli Australis is located at a distance of about 184 light-years (56 parsecs) from Earth.[1]

The spectrum of this star matches a stellar classification of A1 V,[3][4] which identifies it as an A-type main sequence star that is generating energy through the nuclear fusion of hydrogen at its core. An unusual abundance of the element europium demonstrates it to be a peculiar, or Ap star.[9] Most stars of this type are slow rotators,[10] but Gamma Trianguli Australis displays a very high rate of rotation with a projected rotational velocity of 199 km s−1.[4] It has an estimated age of 260 million years.[7]

This system shows an excess emission of infrared radiation, suggesting that there is a circumstellar disk of dust orbiting this star. The mean temperature of the emission is 50 K, corresponding to a separation from the star of 481 AU.[6]

Modern legacy

γ TrA appears on the flag of Brazil, symbolising the state of Paraná.[11]

References

  1. 1.0 1.1 1.2 1.3 1.4 1.5 Lua error in package.lua at line 80: module 'strict' not found.
  2. 2.0 2.1 2.2 Lua error in package.lua at line 80: module 'strict' not found.
  3. 3.0 3.1 Lua error in package.lua at line 80: module 'strict' not found.
  4. 4.0 4.1 4.2 4.3 Lua error in package.lua at line 80: module 'strict' not found.
  5. 5.0 5.1 Lua error in package.lua at line 80: module 'strict' not found.
  6. 6.0 6.1 6.2 Lua error in package.lua at line 80: module 'strict' not found.
  7. 7.0 7.1 Lua error in package.lua at line 80: module 'strict' not found.
  8. Lua error in package.lua at line 80: module 'strict' not found.
  9. Lua error in package.lua at line 80: module 'strict' not found.
  10. Lua error in package.lua at line 80: module 'strict' not found.
  11. Lua error in package.lua at line 80: module 'strict' not found.