Iota Andromedae

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Iota Andromedae
Template:Location mark
Location of ι Andromedae (circled)
Observation data
Epoch J2000      Equinox J2000
Constellation Andromeda
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) +4.29[2]
Characteristics
Evolutionary stage main sequence
Spectral type B8 V[3][4]
U−B Template:Engvar –0.29[5]
B−V Template:Engvar –0.11[5]
Variable type constant[6]
Astrometry
Radial velocity (Rv)–0.5[2] km/s
Proper motion (μ) RA: +27.163 mas/yr[1]
Dec.: −1.246 mas/yr[1]
Parallax (π)6.4313±0.1375 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)−1.63[7]
Details
MassScript error: No such module "val".[4]
Script error: No such module "val".[8] Template:Solar mass
Radius4.6[9] Template:Solar radius
Luminosity638[7] Template:Solar luminosity
Surface gravity (log g)3.35[6] cgs
Temperature12,620[10] K
Metallicity [Fe/H]Script error: No such module "val".[6] dex
Rotational velocity (v sin i)70[11] km/s
Age116[4] Myr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[12]
Database references
SIMBADdata

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Iota Andromedae, also named Rasalnaqa,[13] is a single[14] star in the northern constellation of Andromeda. It has the Flamsteed designation 17 Andromedae, while Iota Andromedae is the Bayer designation as Latinized from ι Andromedae. This object is visible to the naked eye at night as a faint, blue-white hued star with an apparent visual magnitude of +4.29.[2] Based upon parallax measurements, it is located approximately 510 light years distant from the Sun.[1]

This object is a B-type main-sequence star with a stellar classification of B8 V. It is among the least variable stars observed during the Hipparcos mission.[6] The star is 116[4] million years old with 3.1[4] times the mass of the Sun and is spinning with a projected rotational velocity of 70 km/s.[11] It is radiating 638[7] times the luminosity of the Sun from its photosphere at an effective temperature of 12,620 K.[10] The star is somewhat metal-poor, although the abundance of helium is close to solar. The latter excludes it from membership among the class of peculiar stars.[6] Iota Andromedae is a debris disk candidate, showing an infrared excess at a wavelength of 18 μm.[15]

Name

In the catalogue of stars in the Calendarium of Al Achsasi al Mouakket, this star was designated Keff al-Salsalat (كف المسلسلة - kaf al-musalsala), which was translated into Latin as Manus Catenata, meaning hand of the chained woman (i.e. Andromeda).[16] This name originally referred to a group of three starsTemplate:Sndι Andromedae, κ Andromedae, and λ AndromedaeTemplate:Sndalso known in traditional Arabic astronomy as Ra’s al-Nāqa, the head of the she-camel.[17] The IAU Working Group on Star Names approved the name Rasalnaqa for ι Andromedae on 8 May 2025 and it is now so entered in the IAU Catalog of Star Names; the name Kaffalmusalsala was given to κ Andromedae.[13]

In Chinese, Script error: No such module "Lang". (Script error: No such module "Lang".), meaning Flying Serpent, refers to an asterism consisting of ι Andromedae, α Lacertae, 4 Lacertae, π2 Cygni, π1 Cygni, HD 206267, ε Cephei, β Lacertae, σ Cassiopeiae, ρ Cassiopeiae, τ Cassiopeiae, AR Cassiopeiae, 9 Lacertae, 3 Andromedae, 7 Andromedae, 8 Andromedae, λ Andromedae, κ Andromedae and ψ Andromedae. Consequently, the Chinese name for ι Andromedae itself is Script error: No such module "Lang". (Script error: No such module "Lang"., Template:Langx).[18]

References

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  18. Template:In lang AEEA (Activities of Exhibition and Education in Astronomy) 天文教育資訊網 2006 年 7 月 7 日 Template:Webarchive

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Template:Stars of Andromeda