Zeta Boötis

Zeta Boötis

Starbox begin
name=ζ Boötis
Starbox image


caption = ζ Boötis
Starbox observe
epoch=J2000
ra=14h 41m 08.5s
dec= +13° 43′ 42″
appmag_v=4.83
constell=Boötes
Starbox character
class=A2III
r-i =
v-r =
b-v =
u-b =
variable=
Starbox astrometry
radial_v=-5.5
prop_mo_ra=52.36
prop_mo_dec=-12.71
parallax=18.07
p_error=1.24
absmag_v=4.9
Starbox detail
mass=3,1
radius=2,1
luminosity=40 | temperature=7,500–10,000
metal=
gravity=
rotation=
age=
Starbox visbin
name=CCDM 14411+1344 B
period=123.44
axis=0.595
eccentricity=0.957
inclination=142
node=129.99
periastron=1897.59

Starbox visbin
name=CCDM 14411+1344 C
period=
axis=103.8
eccentricity=
inclination=259
node=
periastron=

Starbox catalog
names=30 Boötis, HR 5478+HR 5477, HD 129247+HD 129246, BD+14°2770, HIP 71795, SAO 101145, GC 19777, ADS 9343, CCDM 14411+1344.
Starbox reference
Simbad=HD+129246
ARICNS =
Starbox reference
Simbad=ADS+9343

Zeta Boötis (ζ Boo / ζ Boötis) is a bright speckle binary in the constellation of Boötes. It also has the Flamsteed designation 30 Boötis. It is approximately 181 light years from Earth and has a combined apparent magnitude of +3.78.

The angular separation of the components is currently about 0.8" (this varies slightly with orbital period). As the separation is close to the seeing limit of most astronomical observations, ζ Boötis is often used to test the performance of new high resolution imaging techniques.

Both components, are white A-type giants with apparent magnitudes of +4.43 and +4.83.

Components

Reference

* [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?HR%205477 HR 5477]
* [http://aladin.u-strasbg.fr/AladinPreview?-c=14+41+08.5%2B13+43+42&ident=HD+129246&submit=Aladin+previewer Image Zeta Boötis]
* [http://webviz.u-strasbg.fr/viz-bin/VizieR-S?CCDM%20J14411%2b1344B CCDM J14411+1344]

External links

* [http://simbad.u-strasbg.fr/sim-id.pl?protocol=html&Ident=zet+boo&NbIdent=1&Radius=10&Radius.unit=arcmin&CooFrame=FK5&CooEpoch=2000&CooEqui=2000&output.max=all&o.catall=on&output.mesdisp=N&Bibyear1=1983&Bibyear2=2005&Frame1=FK5&Frame2=FK4&Frame3=G&Equi1=2000.0&Equi2=1950.0&Equi3=2000.0&Epoch1=2000.0&Epoch2=1950.0&Epoch3=2000.0 Zeta Boötis's record on Simbad]
* [http://www.alcyone.de/cgi-bin/search.pl?object=HR5477 HR 5477]


Wikimedia Foundation. 2010.

Игры ⚽ Нужно решить контрольную?

Look at other dictionaries:

  • Zeta Bootis — A/B Imagen de Zeta Bootis obtenida con el Telescopio Óptico Nórdico. Constelación …   Wikipedia Español

  • Eta Boötis — Location of η Boötis Observation data Epoch J2000      Equinox J2000 …   Wikipedia

  • DE Boötis — A/B Observation data Epoch 2000      Equinox 2000 Constellation Boötes Right ascension 14h 53m 23.8s Declination +19° 09 10.1 …   Wikipedia

  • Courant d'étoiles de la Grande Ourse — Le courant de la Grande Ourse, également connu sous le nom de Collinder 285, est le courant stellaire le plus proche de la Terre, il s agit d une association d étoiles partageant des caractéristiques communes telles que l âge, la cinématique et… …   Wikipédia en Français

  • Дзета Волопаса — ABC Кратная звезда Изображение Дзета Волопаса сделанное с помощью Северного оптического телескопа Наблюдательные данные (Эпоха J2000.0) …   Википедия

  • List of Star Trek planets (M–Q) — Contents 1 M 2 N 3 O 4 P 5 Q 6 …   Wikipedia

  • Asociación estelar de la Osa Mayor — Saltar a navegación, búsqueda La Asociación estelar de la Osa Mayor es la asociación estelar más cercana a la Tierra, es decir, un grupo de estrellas con velocidades similares en el espacio, que se cree tienen un origen común. Su núcleo está a… …   Wikipedia Español

  • Diffraction — Computer generated intensity pattern formed on a screen by diffraction from a square aperture …   Wikipedia

  • Lists of stars — Lists= The following are lists of stars:By location::* List of stars by constellationBy name::* List of star names:* List of traditional star names #x2013; according to western culture, including::* List of Arabic star names:* List of Chinese… …   Wikipedia

  • Astronomical seeing — Schematic diagram illustrating how optical wavefronts from a distant star may be perturbed by a layer of turbulent mixing in the atmosphere. The vertical scale of the wavefronts plotted is highly exaggerated. Astronomical seeing refers to the… …   Wikipedia

Share the article and excerpts

Direct link
Do a right-click on the link above
and select “Copy Link”