Iota Arae
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 17h 23m 16.07624s[1] |
Declination | −47° 28′ 05.5057″[1] |
Apparent magnitude (V) | 5.18 - 5.26[2] |
Characteristics | |
Spectral type | B2 IIIne[3] |
U−B color index | −0.82[4] |
B−V color index | −0.11[4] |
R−I color index | −0.08 |
Variable type | BE[2] |
Absolute magnitude (MV) | −2.06[6] |
Details | |
Myr | |
Database references | |
SIMBAD | data |
Iota Arae,
Bortle Dark-Sky Scale
, this means the star is visible to the naked eye from suburban skies.
This is an
absorption lines
to widen and become nebulous, as indicated by the 'n' notation in the stellar class.
Iota Arae has around 8.3 times the mass of the Sun and is shining brightly with 10,864 times the Sun's luminosity. This energy is being radiated into space from the
B-type star.[11]
The General Catalog of Variable Stars classifies it as a BE variable star, ranging from visual magnitude 5.18 to 5.26 with a period of 13.36 hours.[2] In a study of the Hipparcos data, it was found to vary in brightness by 0.054 in magnitude with no clear period.[12]
References
- ^ S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ Bibcode:2009yCat....102025S.
- ^ doi:10.1086/150069.
- ^ Bibcode:1985A&AS...61..387K.
- Bibcode:1967IAUS...30...57E.
- S2CID 119257644.
- ^ S2CID 118629873.
- ^ hdl:11336/37946.
- ^ "iot Ara". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2010-07-30.
- ^ "MAST: Barbara A. Mikulski Archive for Space Telescopes". Space Telescope Science Institute. Retrieved 8 December 2021.
- Commonwealth Scientific and Industrial Research Organisation. December 21, 2004. Archived from the originalon February 22, 2012. Retrieved 2012-01-16.
- .