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Contains:  M 78, NGC 2064, NGC 2067, NGC 2068, NGC 2071
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M78, 



    
        

            AlBroxton
M78
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M78

Technical card

Imaging telescopes or lenses:Celestron C11 Celestron

Imaging cameras:40D Canon

Mounts:CGEM Celestron

Guiding telescopes or lenses:80mm EON Orion

Guiding cameras:Orion Star Shooter

Focal reducers:6.3 reducer Celestron

Software:photoshop5.00 Images Plus


Dates:Jan. 31, 2011

Frames: 32x120" bin 0x0

Integration: 1.1 hours

Avg. Moon age: 27.10 days

Avg. Moon phase: 6.55%


Basic astrometry details

Astrometry.net job: 3443343

RA center: 5h 46' 48"

DEC center: +0° 6' 50"

Pixel scale: 3.570 arcsec/pixel

Orientation: 7.062 degrees

Field radius: 0.546 degrees


Resolution: 906x626

Locations: Leesburg home, Leesburg , Florida, United States

Description

The nebula Messier 78 (also known as M78 or NGC 2068) is a reflection nebula in the constellation Orion. It was discovered by Pierre Méchain in 1780 and included by Charles Messier in his catalog of comet-like objects that same year. M78 is the brightest diffuse reflection nebula of a group of nebulae that include NGC 2064, NGC 2067 and NGC 2071. This group belongs to the Orion Molecular Cloud Complex and is about 1,600 light years distant from Earth. M78 is easily found in small telescopes as a hazy patch and involves two stars of 10th magnitude. These two stars, HD 38563A and HD 38563B, are responsible for making the cloud of dust in M78 visible by reflecting their light.

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Author

AlBroxton
AlBroxton
License: None (All rights reserved)
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            AlBroxton
    Original
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            AlBroxton
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M78, 



    
        

            AlBroxton