HAT-P-8b


IMAGE DETAILS

Object ............................................ HAT-P-8b
Constellation ..............................   Peg
V. Magnitude /Depth .................. 10.17 / 0.0076
Period (days) ................................ 3.0763402 days

RA / DEC ..................................... 22h:55m.10.0sec / +35° 26m.50 sec
Eclipse duration ......................... 216 minutes
Distance ........................................  230(±15)  pc

Spectral type / Temperature....... - / 6200(±80)K
Comparison star .........................  GSC 2757:514
Check star ....................................  GSC 2757:820

Date + Time ................................  02/8/2019  - 19:50 UTC / 01:03 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): 200X 60  Sec
Mount .......................................   Paramount ME
Guiding ....................................   Unguided
Processing Details ..................   Maxim ,The Sky X , HOPS.
More Details ...........................    Environment Temperature : 26° C Camera Temperature -25° C
Sky temperature .....................   12° C
Notes ........................................   Weather: Clear  Transparence:
Medium  Humidity : 75-87 %
Moon Illumination ...............    4%

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

Target details ......................... HAT-P-8b is an extrasolar planet located approximately 720 light years away in the constellation of Pegasus, orbiting the 10th magnitude star GSC 02757-01152. This planet was discovered by transit on December 5, 2008. Despite the designation as HAT-P-8b, it is the 11th planet discovered by the HATNet Project. The mass of the planet is 50% more than Jupiter while the radius is also 50% more than Jupiter. The mass of this planet is exact since the inclination of the orbit is known, typical for transiting planets. This is a so-called “hot Jupiter” because this Jupiter-like gas giant planet orbits in a really close torch orbit around the star, making this planet extremely hot (in the order of a thousand kelvins). The distance from the star is roughly 20 times smaller than that of Earth from the Sun, which places the planet roughly 8 times closer to its star than Mercury is from the Sun. The “year” on this planet lasts only 3 days, 1 hour, 49 minutes, and 54 seconds, compared with Earth's 365 days, 6 hours, 9 minutes, and 10 seconds in a sidereal year.

© Nikos Paschalis