Celestial hemisphere:  Northern  ·  Constellation: Coma Berenices (Com)  ·  Contains:  M 91  ·  NGC 4548
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M91, 



    
        

            sydney
M91
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M91

Getting plate-solving status, please wait...
M91, 



    
        

            sydney
M91
Powered byPixInsight

M91

Acquisition details

Dates:
April 12, 2020 ·  May 14, 2020
Frames:
Astrodon I-series: 60×480(8h) bin 2×2
Luminance: 46×600(7h 40′) bin 1×1
Integration:
15h 40′
Avg. Moon age:
20.88 days
Avg. Moon phase:
62.94%

Basic astrometry details

Astrometry.net job: 3615882

RA center: 12h35m25s.7

DEC center: +14°2952

Pixel scale: 0.511 arcsec/pixel

Orientation: 127.734 degrees

Field radius: 0.186 degrees

Resolution: 2178x1464

File size: 1.0 MB

Data source: Backyard

Description

M91 (NGC 4548) is a barred spiral galaxy in the constellation Coma Berenices. It is one of the faintest Messier objects at approximately magnitude 11. M91 is about 63 million light-years away and has an apparent size of 5.4 x 4.3 arc minutes. The observation of Cepheid variable stars by the Hubble Space Telescope confirmed that M91 is a member of the Virgo Cluster [https://iopscience.iop.org/article/10.1086/307151/fulltext/39340.text.html]. M91 is classified as “anemic” for its relative lack of star forming regions and gas, possibly resulting from ram pressure stripping as it passes through the dense galaxy cluster [http://adsabs.harvard.edu/full/1999A%26A...349..411V].

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M91, 



    
        

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