HAT-P-14b


IMAGE DETAILS

Object ............................................ HAT-P-14b
Constellation ..............................  Her
V. Magnitude /Depth ..................9.98/ 0.0054
Period (days) ................................4.627669

RA / DEC ..................................... 17h:20m.28sec / +30° 14m.32ec
Eclipse duration ..........................131.4 minutes
Distance ........................................  205
±11 pc
Spectral type / Temperature....... F / 6600 K (
± 90)
Comparison star .........................  Tycho 3086:1836
Check star ....................................  HIP 84832

Date + Time ................................  25/04/2017  - 19:33 UTC / 23:30 UTC
Location .................................... 
"Nunki Observatory" - Skiathos
Optics .........................................  
Officina Stellare Advanced RILA 400 f/5.25
Tools ..........................................   ACP
Camera ......................................  
 SBIG STXL11002  with FW8G-STXL (Astrodon filters)
Exposure Time.........................    Rc (Atrodon Photometric): 160 X 60  Sec
Mount .......................................   Paramount ME
Guiding ....................................   Unguided
Processing Details ..................   Maxim , HOPS.
More Details ...........................    Environment Temperature : 14° C Camera Temperature -35° C
Sky temperature .....................   -11.5°
Notes ........................................   Weather: Clear  Transparence:
Medium  Humidity : 80-85 %
Moon Illumination ...............    1%

Amateur astronomers on duty : Nikolaos I. Paschalis
Analysing Software                   :  Ang
elos Tsiaras

Target details ......................... 
HAT-P-14b is an extrasolar planet located approximately 205 parsecs (670 ly) away in the constellation of Hercules, orbiting the 10th magnitude F-type star HAT-P-14. This planet was discovered in 2010 by the HATNet Project using the transit method. It was independently detected by the SuperWASP project.
HAT-P-14b is located very close orbit to its star, taking only 4.6 days to complete one orbit. Observations of the Rossiter–McLaughlin effect with the Keck telescope show that it orbits in a retrograde fashion relative to the rotation axes of its parent star.

© Nikos Paschalis