BQ Ari

Aries · 02/09/2017 - 22:00 UTC · Officina Stellare Advanced RILA 400 f/5.25

Light curve of BQ Ari
Comparison and check stars, BQ Ari
BQ Ari

About the target

EW- W Ursae Majoris-type eclipsing variables. These are eclipsers with periods usually shorter than 1 day, consisting of ellipsoidal components almost in contact and having light curves for which it is impossible to specify the exact times of onset and end of eclipses. The depths of the primary and secondary minima are almost equal or differ insignificantly. Light amplitudes are usually <0.8 mag. in V. The components generally belong to spectral types F-G and later.

'The Artistic Image above, reproduced courtesy of Mark A. Garlick / markgarlick.com (opens in a new tab). No unauthorized use".

© Nikos Paschalis

Observing log

Object
BQ ARI
Constellation
Aries
V. Magnitude + Variability
10.28-10.55/ EW
RA / DEC
02h:48m.40sec / +13°44m.48sec
Period
0.282336 days
Comparison star
GSC 648:868
Check star
GSC 646:726
Date + Time
02/09/2017 - 22:00 UTC
Location
“Nunki Observatory” - Skiathos
Optics
Officina Stellare Advanced RILA 400 f/5.25
Tools
THE SKY X
Camera
SBIG STXL11002 with FW8G-STXL (Astrodon filters)
Exposure Time
Rc: 3.9 Hours
Mount
Paramount ME
Guiding
Unguided
Processing Details
ACP, Muniwin
More Details
Environment Temperature: 22 °C Camera Temperature -25 °C
Sky temperature
-12.4. οC
Notes
Weather: Clear Transparence: Medium Humidity: 75-85%
Moon Illumination
Moon phase on the night of the observation88%