HAT-P-32b




IMAGE DETAILS

Object ............................................ HAT-P-32b
Constellation ..............................  And
V. Magnitude /Depth ..................11.29 / 0.0244
Period (days) ................................2.150008

RA / DEC ..................................... 02h:04m.10sec / +46 41m.16.8ec
Eclipse duration ..........................186.5 minutes
Distance ........................................ 1044
 10
Ly
Spectral type ................................ F/G
Comparison star .........................  Tycho 3281:114
Check star ....................................  Tycho 3280:490

Date + Time ................................  01/08/2016  - 19:30UTC / 01:40 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.........................    Red: 280 X 60  Sec
Mount .......................................   Paramount ME
Guiding ....................................   Unguided
Processing Details ..................   Maxim ,The Sky X , Ccdautopilot 5
More Details ...........................    Environment Temperature : 25 oC Camera Temperature -30 οC
Sky temperature .....................   -14. οC
Notes ........................................   Weather: Clear  Transparence:
Medium  Humidity : 70-75 %
Moon Illumination ...............    1%

Amateur astronomers on duty : Nikolaos I. Paschalis
Analysing data & analysing software :  Ang
elos Tsiaras - Natasa Kokori

HAT-P-32b
is a planet in the orbit of the G-type or F-type star HAT-P-32, which is approximately 1,044 light years away from Earth. HAT-P-32b was first recognized as a possible planet by the planet-searching HATNet Project in 2004, although difficulties in measuring its radial velocity prevented astronomers from verifying the planet until after three years of observation. The Blendanal program helped to rule out most of the alternatives that could explain what HAT-P-32b was, leading astronomers to determine that HAT-P-32b was most likely a planet. The discovery of HAT-P-32b and of HAT-P-33b was submitted to a journal on June 6, 2011.

The planet is considered a Hot Jupiter, and although it is slightly less massive than Jupiter, it is bloated to nearly twice Jupiter's size. At the time of its discovery, HAT-P-32b had one of the largest radii known amongst extrasolar planets. This phenomenon, which has also been observed in planets like WASP-17b and HAT-P-33b, has shown that something more than temperature is influencing why these planets become so large.
 

Nikos Paschalis