Zeta Boötis
Template:Location mark Location of ζ Boötis (circled) | |
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Boötes |
| ζ Boo | |
| Right ascension | Template:RA[1] |
| Declination | Template:DEC[1] |
| Apparent magnitude (V) | 3.78[2] (4.46 + 4.55)[3] |
| HIP 71759 | |
| Right ascension | Template:RA[4] |
| Declination | Template:DEC[4] |
| Apparent magnitude (V) | 5.925[5] |
| Characteristics | |
| ζ Boo | |
| Spectral type | A1V[6] |
| U−B Template:Engvar | +0.05[2] |
| B−V Template:Engvar | +0.05[2] |
| HIP 71759 | |
| Spectral type | F0V[7] |
| B−V Template:Engvar | 0.227[5] |
| Variable type | δ Scuti[8] |
| Astrometry | |
| ζ Boo | |
| Radial velocity (Rv) | Script error: No such module "val".[9] km/s |
| Proper motion (μ) | RA: +51.95 mas/yr[1] Dec.: −11.08 mas/yr[1] |
| Parallax (π) | 18.56±0.76 mas[1] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | +0.13[10] |
| HIP 71759 | |
| Proper motion (μ) | RA: +54.399 mas/yr[4] Dec.: −15.481 mas/yr[4] |
| Parallax (π) | 19.3257±0.0511 mas[4] |
| Distance | Template:Rnd ± Template:Rnd ly (Template:Rnd ± Template:Rnd pc) |
| Absolute magnitude (MV) | 2.37[8] |
| Details[11] | |
| ζ Boo A | |
| Mass | Script error: No such module "val". Template:Solar mass |
| Radius | Script error: No such module "val". Template:Solar radius |
| Temperature | Script error: No such module "val". K |
| Age | Script error: No such module "val". Myr |
| ζ Boo B | |
| Mass | Script error: No such module "val". Template:Solar mass |
| Radius | Script error: No such module "val". Template:Solar radius |
| Temperature | Script error: No such module "val". K |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Age | Script error: No such module "val". Myr |
| HIP 71759 | |
| Mass | Script error: No such module "val".[8] Template:Solar mass |
| Radius | Script error: No such module "val".[8] Template:Solar radius |
| Luminosity | Script error: No such module "val".[8] Template:Solar luminosity |
| Surface gravity (log g) | Script error: No such module "val".[8] cgs |
| Temperature | Script error: No such module "val".[8] K |
| Metallicity [Fe/H] | {{{metal_fe2}}} dex |
| Other designations | |
| Template:Odlist[12] | |
| A: Template:Odlist[13] | |
| B: Template:Odlist[14] | |
| HIP 71759: Template:Odlist | |
| Database references | |
| SIMBAD | data |
| HIP 71759 | |
| SIMBAD | data |
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Zeta Boötis is a binary star system in the constellation of Boötes that forms a triple star system with HIP 71759. Its name is a Bayer designation that is Latinized from ζ Boötis, and abbreviated Zeta Boo or ζ Boo. They have the Flamsteed designation 30 Boötis. This system is visible to the naked eye as a point of light with an apparent visual magnitude of +3.78.[2] The individual magnitudes of the components differ slightly, with component A having a magnitude of 4.46 and component B at the slightly dimmer magnitude 4.55.[3] The system is located at a distance of approximately 180 light years based on parallax,[1] but is drifting closer to the Sun with a radial velocity of −9 km/s.[9]
Observations
The duplicity of this star was discovered by English astronomer William Herschel in 1796, and their changing positions have been tracked from 1823 onward.[15]
In 1976, T. W. Edwards found a stellar classification of A2III for both inner components, suggesting they may be evolved A-type giant stars. Helmut A. Abt reported a class of A2V in 1981, which matches an A-type main-sequence star.[16] Abt and Nidia Morrell updated the classification to A1V in 1995.[6]
Characteristics
The two components of the pair, Zeta Boötis A and B, are A-type main-sequence stars. Component A has 2.21 times the Sun's mass, 2.6 times the Sun's radius and an effective temperature of 8,800 K. Component B has 2.15 times the Sun's mass, 2.4 times the Sun's radius and an effective temperature of 8,750 K. Their estimated age is 560 million years.[11]
The stars take 125 years to orbit each other. The orbit of this pair has a very high eccentricity of 0.98045, bringing them within 0.818 au at their closest approach (periastron). Template:Asof, the eccentricity of this system is possibly the second-highest known, after HIP 26245, whose eccentricity is Script error: No such module "val".. The last periastron occurred during November 2023.[11] Considering the extreme nature of their orbit, it is unlikely that any exoplanets could have stable orbits around either star.[17]
Together with the star HIP 71759, Zeta Boötis make a triple star system. This distant star has an estimated orbital period of three million years, being at an observed distance of Template:Cvt from the inner pair. The orbit of this star is likely what forced the high eccentricity orbit of the inner pair, via the Kozai mechanism.[18] It has a class of F0V, matching an F-type main-sequence star.[7] It is a Delta Scuti variable with a brightness amplitude of 0.00134 magnitudes.[8]
Gallery
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Zeta Bootis imaged with the Nordic Optical Telescope on 13 May 2000 using the lucky imaging method. (The Airy discs around the stars is diffraction from the 2.56m telescope aperture.)
-
Typical short-exposure image of a binary star, as seen using speckle imaging through the Earth's atmosphere.
References
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- ↑ Template:Cite XHIP
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- ↑ Template:Cite simbad
- ↑ Template:Cite simbad
- ↑ Template:Cite simbad
- ↑ Script error: No such module "citation/CS1".
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- ↑ Script error: No such module "citation/CS1".
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External links
- Script error: No such module "citation/CS1".
- HR 5477
- Image Zeta Boötis
- CCDM J14411+1344
- Pages with script errors
- Pages with broken file links
- A-type giants
- A-type main-sequence stars
- F-type main-sequence stars
- Binary stars
- Kozai mechanism
- Boötes
- Bayer objects
- Bright Star Catalogue objects
- Durchmusterung objects
- Flamsteed objects
- Henry Draper Catalogue objects
- Hipparcos objects
- Astronomical objects discovered in 1796