Vega - α Lyrae

IMAGE DETAILS

Object ............................................ Vega - α Lyr
Constellation ..............................  Lyrae
Distance + Ap. Magnitude.......   25  Light Years (7.68 parsec) - 0.03
RA / DEC ..................................... 18h:36m.56sec / +38 47m.01sec
Spectral type/B-V Color index  A0V / +0.00
Mass / Radius ............................. 2.14 solar / 2.36 solar

Temperature ................................ 9600 Kelvin

Date + Time ...............................   25 / 9 /2012 - 17:45 UTC
Location ....................................  "Nunki Observatory" - Skiathos
Optics .........................................
 
Celestron C11 HD f/10
Tools ..........................................   Maxim dl
Camera .....................................   SBIG ST-2000XM with CFW10 (Astrodon filters)
Exposure Time.......................     Luminance: 120 X 0.5sec RGB: 80 X 1sec (each)
More Details ...........................    Environment Temperature : 21oC Camera Temperature 0οC
Mount .......................................   Paramount ME
Guiding ....................................   Unguided
Processing Details ................    Photoshop , Maxim ,
Notes ........................................   Weather: 8/10 - Transparence: 2/6 - Humidity : 78%

Target details .........................    
Vega (α Lyr, α Lyrae, Alpha Lyrae) is the brightest star in the constellation Lyra, the fifth brightest star in the night sky and the second brightest star in the northern celestial hemisphere, after Arcturus. It is a relatively close star at only 25 light-years from Earth, and, together with Arcturus and Sirius, one of the most luminous stars in the Sun's neighborhood.Vega has been extensively studied by astronomers, leading it to be termed "arguably the next most important star in the sky after the Sun."Vega was the northern pole star around 12,000 BC and will be so again around AD 13,727.
Vega is only about a tenth of the age of the Sun, but since it is 2.1 times as massive its expected lifetime is also one tenth of that of the Sun; both stars are at present approaching the midpoint of their life expectancies. Vega has an unusually low abundance of the elements with a higher atomic number than that of helium.Vega is also a suspected variable star that may vary slightly in magnitude in a periodic manner. It is rotating rapidly with a velocity of 274 km/s at the equator. This is causing the equator to bulge outward because of centrifugal effects, and, as a result, there is a variation of temperature across the star's photosphere that reaches a maximum at the poles. From Earth, Vega is being observed from the direction of one of these poles.
Based on an observed excess emission of infrared radiation, Vega appears to have a circumstellar disk of dust. This dust is likely to be the result of collisions between objects in an orbiting debris disk, which is analogous to the Kuiper belt in the Solar System. Stars that display an infrared excess because of dust emission are termed Vega-like stars.Irregularities in Vega's disk also suggest the presence of at least one planet, likely to be about the size of Jupiter,in orbit around Vega.

 

Nikos Paschalis