17 Lyrae

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Template:Short description

17 Lyrae AB
Template:Location mark
Location of 17 Lyrae (circled)
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Lyra
AB
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 5.221[2]
A
Right ascension Template:RA[3]
Declination Template:DEC[3]
Apparent magnitude (V) 5.26[4]
B
Right ascension Template:RA[5]
Declination Template:DEC[5]
Apparent magnitude (V) 9.1[6]
Characteristics
Spectral type F0V[7]
U−B Template:Engvar +0.044[8]
B−V Template:Engvar +0.351[8]
Astrometry
A
Proper motion (μ) RA: +114.276[3] mas/yr
Dec.: +18.316[3] mas/yr
Parallax (π)22.8557±0.0782 mas[3]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
B
Proper motion (μ) RA: +120.597[5] mas/yr
Dec.: +9.110[5] mas/yr
Parallax (π)22.8407±0.0190 mas[5]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Orbit[9]
PrimaryA
Period (P)42.857 days
Eccentricity (e)0.0
Semi-amplitude (K1)
(primary)		13.10 km/s
Details
A
Mass1.6[9] Template:Solar mass
Radius2.5[3] Template:Solar radius
Luminosity16.4[10] Template:Solar luminosity
Surface gravity (log g)3.57[8] cgs
Temperature6,887[10] K
Metallicity [Fe/H]0.0[11] dex
Rotational velocity (v sin i)138[10] km/s
Age1.4[11] Gyr
B
Mass0.73[12] Template:Solar mass
Surface gravity (log g)4.61[12] cgs
Temperature5,266[12] K
Metallicity [Fe/H]−0.46[12] dex
Other designations
17 Lyrae, HR 7261, BD+32°3326, HD 178449, SAO 67835, HIP 93917, GC 26340, CCDM J19075+3231, IDS 19036+3221
Database references
SIMBADdata

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17 Lyrae is a multiple star system in the constellation Lyra, 143 light years away from Earth.

Components

The 17 Lyrae system contains two visible components, designated A and B, separated by 2.48" in 1997. The primary star is a single-lined spectroscopic binary with a period of 42.9 days.[8]

There was once thought to be a fourth star in the system, the red dwarf binary Kuiper 90, designated 17 Lyrae C, until it was evident that the star's parallax and proper motions were too different for it to be part of the system.[13] The separation between 17 Lyrae AB and C is increasing rapidly, from less than 2' in 1881 to nearly 5' in 2014.[14]

A number of other visual companions have been catalogued. The closest is the 11th magnitude star at 39", and the brightest is BD+32 3325 just over 2' away.[14]

Properties

The primary component, 17 Lyrae A, is a 5th magnitude main sequence star of the spectral type F0, meaning it has a surface temperature of about 6,750 K. It is about 60% more massive than the sun and 16 times more luminous. It has been catalogued as an Am star but is now believed to be a relatively normal quickly-rotating star.[8]

The visible companion 17 Lyrae B is a 9th magnitude star of an unknown spectral type. The spectroscopic companion cannot be detected in the spectrum and its properties are uncertain. Faint sharp spectral lines contrasting with the broadened lines of the primary may originate in a shell of material around the stars.[8]

References

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  5. ↑ a b c d e Template:Cite Gaia DR3
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  8. ↑ a b c d e f Script error: No such module "Citation/CS1".
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  10. ↑ a b c Script error: No such module "Citation/CS1".
  11. ↑ a b Script error: No such module "Citation/CS1".
  12. ↑ a b c d Script error: No such module "Citation/CS1".
  13. ↑ Script error: No such module "Citation/CS1".
  14. ↑ a b Script error: No such module "Citation/CS1".

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External links

Template:Stars of Lyra

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