Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Corona Borealis |
Right ascension | 16h 01m 26.56488s[1] |
Declination | +29° 51′ 03.8243″[1] |
Apparent magnitude (V) | 4.96[2] |
Characteristics | |
Spectral type | A0 IIIp(HgMnEu)s[3] |
U−B color index | −0.15[2] |
B−V color index | −0.06[2] |
Astrometry | |
Radial velocity (Rv) | −20.8±0.4[4] km/s |
Proper motion (μ) | RA: −38.31[1] mas/yr Dec.: −6.56[1] mas/yr |
Parallax (π) | 10.46 ± 0.24 mas[1] |
Distance | 312 ± 7 ly (96 ± 2 pc) |
Absolute magnitude (MV) | +0.08[5] |
Orbit[6] | |
Period (P) | 35.474 d |
Eccentricity (e) | 0.56 |
Periastron epoch (T) | 2441566.96 JD |
Argument of periastron (ω) (secondary) | 156° |
Semi-amplitude (K1) (primary) | 2.3 km/s |
Details | |
ι CrB A | |
Luminosity | 90[7] L☉ |
Surface gravity (log g) | 3.84±0.16[8] cgs |
Temperature | 10,727±278[8] K |
Metallicity [Fe/H] | −0.01±0.12[8] dex |
Rotational velocity (v sin i) | 18[9] km/s |
Other designations | |
Database references | |
SIMBAD | data |
Iota Coronae Borealis, Latinized from ι Coronae Borealis, is a binary star[6] system in the constellation Corona Borealis. It is visible to the naked eye with a combined apparent visual magnitude of is 4.96.[2] Based upon an annual parallax shift of 10.46 mas as seen from the Earth,[1] it is located about 312 light years from the Sun.
This is a single-lined spectroscopic binary with an orbital period of 35.5 days and an eccentricity of 0.56.[6] The visible member, component A, has a stellar classification of A0 IIIp(HgMnEu)s,[3] indicating it is a chemically peculiar mercury-manganese star with narrow absorption lines. The secondary member, component B, appears to be an A-type star.[11]
vanLeeuwen2007
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was invoked but never defined (see the help page).Mcdonald2012
was invoked but never defined (see the help page).Prugniel2011
was invoked but never defined (see the help page).Royer2002
was invoked but never defined (see the help page).SIMBAD
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was invoked but never defined (see the help page).