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132 Tauri
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Star in the constellation Taurus
Taurus constellation map.svg center 280 right Red circle.svg 10 132 Tauri 40 292 Location of 132 Tauri (circled in red)
J2000
Taurus
05 49 00.96598
+24 34 03.1220
4.89 (5.07 + 9.09)
G9 III
1.021
+15.8 0.6
+10.44
−8.30
8.97
1.98
132 Tau Aa
2.74 0.11
4853 47 commas
0.18 0.05
132 Tau +24°970 2435 38751 27468 2002 77592 J05490+2434AB
132+Tau
132 Tauri is a binary star system in the constellation Taurus. It is faintly visible to the naked eye with an apparent visual magnitude of 4.89. Based upon a poorly constrained annual parallax shift of 8.97 1.98 mas, it is located roughly 360 light years from the Sun. The system is moving further away with a heliocentric radial velocity of +16 km/s. It lies near the ecliptic and thus is subject to occultation by the Moon. One such event was observed September 3, 1991.
This system forms a wide double star with an angular separation of 3.8 arcsec along a position angle of 230°, as of 1991. The brighter star, component A, has an apparent magnitude of 4.99 while the fainter secondary, component B, is of magnitude 9.09. The primary is itself an unresolved binary with a combined stellar classification of G9 III, which matches an aging G-type giant star that has exhausted the hydrogen at its core and evolved away from the main sequence.
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Category:G9III stars
Category:Suspected variables
Category:Taurus (constellation)
BD+24 0970
Tauri, 132
038751
027468
2002