Hemisphere:  Northern  ·  Constellation: Triangulum (Tri)  ·  Contains:  M 33  ·  NGC 598  ·  Triangulum galaxy
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Triangulum Galaxy, 



    
        

            José J. Chambó
Triangulum Galaxy
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Technical card

Imaging telescopes or lenses: Meade ETX-70

Imaging cameras: Canon EOS 350D / Digital Rebel XT

Mounts: LXD75

Software: DeepSkyStacker  ·  PixInsight LE


Dates:Nov. 12, 2010

Frames: 26x90" (39') ISO1600

Integration: 39'

Darks: ~10

Flats: ~12

Bias: ~13

Avg. Moon age: 6.31 days

Avg. Moon phase: 38.67%

Bortle Dark-Sky Scale: 3.00

Mean SQM: 20.60

Mean FWHM: 4.26


Basic astrometry details

Astrometry.net job: 114205

RA center: 1h 33' 49"

DEC center: +30° 39' 39"

Pixel scale: 5.335 arcsec/pixel

Orientation: -86.206 degrees

Field radius: 0.972 degrees


Resolution: 620x496

Locations: Hoya Redonda - Valencia (Spain), Enguera, Valencia, Spain

Description

The Triangulum Galaxy is a spiral galaxy located in the Triangulum constellation to a distance of 2,8 million light-years, member of Local Group of galaxies with our Milky Way and the nearby Andromeda Galaxy to wich is conected. Discovered by Giovanni Odierna from Sicily before 1654 and by Messier on 1764 and in wich Herschel has cataloged some H II regions of nursery stars, one of these is NGC 604 is one of the greatest known (40 times the Orion Nebula). M 33 can be observed at naked eye in exceptional conditions of visibility, being so the most away object at naked eye, because its great angular size (two moons) and its fuzzy brightness, the best instrument for observe it are a binoculars or a short focal telescope at very low power.

More info into the Blog  C O M E T O G R A F I A(in Spanish)

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Triangulum Galaxy, 



    
        

            José J. Chambó