Iota Aquarii: Difference between revisions
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m Robot - Moving category Aquarius constellation to Category:Aquarius (constellation) per CFD at Wikipedia:Categories for discussion/Log/2012 March 14. |
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[[Category:Bayer objects|Aquarii, Iota]] |
[[Category:Bayer objects|Aquarii, Iota]] |
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[[Category:Flamsteed objects|Aquarii, 33]] |
[[Category:Flamsteed objects|Aquarii, 33]] |
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[[Category:Aquarius constellation]] |
[[Category:Aquarius (constellation)]] |
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[[Category:B-type subgiants]] |
[[Category:B-type subgiants]] |
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Revision as of 16:47, 21 March 2012
Observation data Epoch J2000 Equinox J2000 | |
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Constellation | Aquarius |
Right ascension | 22h 06m 26.2297s |
Declination | –13° 52′ 10.845″ |
Apparent magnitude (V) | 4.281 |
Characteristics | |
Spectral type | B8V |
U−B color index | -0.29 |
B−V color index | -0.07 |
Astrometry | |
Radial velocity (Rv) | –10 km/s |
Proper motion (μ) | RA: 40.45 mas/yr Dec.: –57.16 mas/yr |
Parallax (π) | 18.9 ± 0.95 mas |
Distance | 173 ± 9 ly (53 ± 3 pc) |
Absolute magnitude (MV) | 3.219 |
Details | |
Radius | 2.7[1] R☉ |
Temperature | 11,284 ± 284[1] K |
Age | 30–60[2] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Iota Aquarii (ι Aqr, ι Aquarii) is a star in the constellation Aquarius.
Iota Aquarii is a blue-white B-type subgiant with an apparent magnitude of +4.29. It is approximately 173 light years from Earth.
References
- ^ a b Underhill, A. B.; et al. (1979), "Effective temperatures, angular diameters, distances and linear radii for 160 O and B stars", Monthly Notices of the Royal Astronomical Society, 189: 601–605, Bibcode:1979MNRAS.189..601U
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ignored (help) - ^ Ehrenreich, D.; et al. (2010), "Deep infrared imaging of close companions to austral A- and F-type stars", Astronomy and Astrophysics, 523: A73, Bibcode:2010A&A...523A..73E, doi:10.1051/0004-6361/201014763
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