HD 31093

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Template:Short description

HD 31093
Observation data
Epoch J2000      Equinox J2000
Constellation Caelum[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 5.83±0.01[3]
Characteristics
Spectral type A1V + A4V[4]
U−B Template:Engvar +0.09[5]
B−V Template:Engvar +0.08[5]
Astrometry
Radial velocity (Rv)+24±1.8[6] km/s
Proper motion (μ) RA: Script error: No such module "val".[2] mas/yr
Dec.: Script error: No such module "val".[2] mas/yr
Parallax (π)12.17±0.41 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)+1.25[1] (combined)
Orbit
Period (P)43.36±4.34[7] yr
Semi-major axis (a)0.248±0.015[7]
Eccentricity (e)0.852[7]
Inclination (i)107±1[4]°
Longitude of the node (Ω)20±2[4]°
Argument of periastron (ω)
(secondary)
109±2[4]°
Details
HD 31093 A
Mass1.85 ± 0.21[4] Template:Solar mass
HD 31093 B
Mass1.58 ± 0.18[4] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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HD 31093, also known as HR 1559, is a visual binary located in the southern constellation Caelum, the chisel. The components have a combined apparent magnitude of 5.83,[3] making it faintly visible to the naked eye. Based on parallax measurements from the Hipparcos spacecraft, the system is estimated to be 268 light years distant.[2] They appear to be receding from the Solar System with a heliocentric radial velocity of Script error: No such module "val"..[6]

The components have stellar classifications of A1 and A4 V, indicating that both of them are A-type main-sequence stars. Since the components have a separation of <templatestyles src="Fraction/styles.css" />14 arcseconds, it is difficult to distinguish individually through a telescope. The primary has a mass 1.85 times that of the Sun while the secondary has a mass of Template:Solar mass.[4] They take 43 years to circle each other in an eccentric orbit.[7]

References

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External links

Template:Stars of Caelum