NGC300

NGC300
0

NGC300

NGC300 is a spiral galaxy in the constellation Sculptor. It is inclined at an angle of 42 degrees as viewed from the earth and lies approximately 7 million light-years from our Milky Way galaxy.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
Planewave CDK 24
Camera ..........................................................................................................................................................................................................................
Camera
FLI PL9000
Location ..........................................................................................................................................................................................................................
Location
Rio Hurtado, Chile
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Posted 11 March, 2021
Filters ..........................................................................................................................................................................................................................
Filters
L,R,G,B
Processing ..........................................................................................................................................................................................................................
Processing
PixInsight and Photoshop
Credits ..........................................................................................................................................................................................................................
Credits
Data set curated by Nik Szymanek
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