From Wikipedia, the free encyclopedia
κ Boötis

Kappa Boötis
Observation data
Epoch J2000       Equinox J2000
Constellation Boötes
Right ascension 14h 13m 29.0078s
Declination +51° 47′ 23.874″
Characteristics
Spectral type A8IV
U−B color index 0.14
B−V color index 0.2
R−I color index 0.12
Variable type Delta Scuti variable
Astrometry
Radial velocity (Rv)-17.4 km/s
Proper motion (μ) RA: 61.39  mas/ yr
Dec.: -10.57  mas/ yr
Parallax (π)21.03 ± 0.83  mas
Distance155 ± 6  ly
(48 ± 2  pc)
Absolute magnitude (MV)4.74
Details
Mass3,1  M
Radius2,1  R
Luminosity40  L
Temperature7,500–10,000  K
Rotation127 Km/s
0,002295 Year
Other designations
Asellus Tertius, 17 Boötis, HR 5329+HR 5328, HD 124675+HD 124674, BD+52°1782, HIP 69483+HIP 69481, SAO 29046+SAO 29045.
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

Kappa Boötis (κ Bootis, κ Boö) is the 4th magnitude star in the constellation Boötes. It was the 3rd member of an former asterism, Asellus by Johann Bayer, so called Aselles tertius [1] ( Latin for "the third Ass", later Asellus Tertius. It is approximately 155 light years from the Earth.

Kappa Boötis is a binary star system viewable in small telescope, with components separated by an angular distance of 13.4 .

κ2 Boötis

κ2 Boötis

Kappa Boötis
Observation data
Epoch J2000       Equinox J2000
Constellation Boötes
Right ascension 14h 13m 29.0078s
Declination +51° 47′ 23.874″
Characteristics
Spectral type A8IV
U−B color index 0.14
B−V color index 0.2
R−I color index 0.12
Variable type Delta Scuti variable
Astrometry
Radial velocity (Rv)-17.4 km/s
Proper motion (μ) RA: 61.39  mas/ yr
Dec.: -10.57  mas/ yr
Parallax (π)21.03 ± 0.83  mas
Distance155 ± 6  ly
(48 ± 2  pc)
Absolute magnitude (MV)4.74
Details
Mass3,1  M
Radius2,1  R
Luminosity40  L
Temperature7,500–10,000  K
Rotation127 Km/s
0,002295 Year
Other designations
Asellus Tertius, 17 Boötis, HR 5329+HR 5328, HD 124675+HD 124674, BD+52°1782, HIP 69483+HIP 69481, SAO 29046+SAO 29045.
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

κ2 Boötis is the brighter / following component of this star system. It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +4.50 to +4.58 with a period of 1.83 hours. The companion star, κ¹ Boötis, has magnitude +6.58 and spectral class F1V.

κ1 Boötis

κ1 Boötis
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Boötes
Right ascension 14h 13m 27.7s
Declination +51° 47' 16"
Apparent magnitude (V) +4.53, +6.62
Distance155 ± 6  ly
(48 ± 2  pc)
Spectral typeF1V
Database references
SIMBAD data

Kappa1 Boötis is the dimmer / precceding component of this star system. It has apparent magnitude +4.54 and spectral class A8IV.

References

  1. ^ Allen, R. H., (1963). Star Names: Their Lore and Meaning ( Rep. ed.). New York, NY: Dover Publications Inc. p. 105. ISBN  0486210790.{{ cite book}}: CS1 maint: extra punctuation ( link) CS1 maint: multiple names: authors list ( link)
From Wikipedia, the free encyclopedia
κ Boötis

Kappa Boötis
Observation data
Epoch J2000       Equinox J2000
Constellation Boötes
Right ascension 14h 13m 29.0078s
Declination +51° 47′ 23.874″
Characteristics
Spectral type A8IV
U−B color index 0.14
B−V color index 0.2
R−I color index 0.12
Variable type Delta Scuti variable
Astrometry
Radial velocity (Rv)-17.4 km/s
Proper motion (μ) RA: 61.39  mas/ yr
Dec.: -10.57  mas/ yr
Parallax (π)21.03 ± 0.83  mas
Distance155 ± 6  ly
(48 ± 2  pc)
Absolute magnitude (MV)4.74
Details
Mass3,1  M
Radius2,1  R
Luminosity40  L
Temperature7,500–10,000  K
Rotation127 Km/s
0,002295 Year
Other designations
Asellus Tertius, 17 Boötis, HR 5329+HR 5328, HD 124675+HD 124674, BD+52°1782, HIP 69483+HIP 69481, SAO 29046+SAO 29045.
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

Kappa Boötis (κ Bootis, κ Boö) is the 4th magnitude star in the constellation Boötes. It was the 3rd member of an former asterism, Asellus by Johann Bayer, so called Aselles tertius [1] ( Latin for "the third Ass", later Asellus Tertius. It is approximately 155 light years from the Earth.

Kappa Boötis is a binary star system viewable in small telescope, with components separated by an angular distance of 13.4 .

κ2 Boötis

κ2 Boötis

Kappa Boötis
Observation data
Epoch J2000       Equinox J2000
Constellation Boötes
Right ascension 14h 13m 29.0078s
Declination +51° 47′ 23.874″
Characteristics
Spectral type A8IV
U−B color index 0.14
B−V color index 0.2
R−I color index 0.12
Variable type Delta Scuti variable
Astrometry
Radial velocity (Rv)-17.4 km/s
Proper motion (μ) RA: 61.39  mas/ yr
Dec.: -10.57  mas/ yr
Parallax (π)21.03 ± 0.83  mas
Distance155 ± 6  ly
(48 ± 2  pc)
Absolute magnitude (MV)4.74
Details
Mass3,1  M
Radius2,1  R
Luminosity40  L
Temperature7,500–10,000  K
Rotation127 Km/s
0,002295 Year
Other designations
Asellus Tertius, 17 Boötis, HR 5329+HR 5328, HD 124675+HD 124674, BD+52°1782, HIP 69483+HIP 69481, SAO 29046+SAO 29045.
Database references
SIMBAD data
Data sources:
Hipparcos Catalogue,
CCDM (2002),
Bright Star Catalogue (5th rev. ed.)

κ2 Boötis is the brighter / following component of this star system. It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +4.50 to +4.58 with a period of 1.83 hours. The companion star, κ¹ Boötis, has magnitude +6.58 and spectral class F1V.

κ1 Boötis

κ1 Boötis
Observation data
Epoch J2000.0       Equinox J2000.0
Constellation Boötes
Right ascension 14h 13m 27.7s
Declination +51° 47' 16"
Apparent magnitude (V) +4.53, +6.62
Distance155 ± 6  ly
(48 ± 2  pc)
Spectral typeF1V
Database references
SIMBAD data

Kappa1 Boötis is the dimmer / precceding component of this star system. It has apparent magnitude +4.54 and spectral class A8IV.

References

  1. ^ Allen, R. H., (1963). Star Names: Their Lore and Meaning ( Rep. ed.). New York, NY: Dover Publications Inc. p. 105. ISBN  0486210790.{{ cite book}}: CS1 maint: extra punctuation ( link) CS1 maint: multiple names: authors list ( link)

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