NGC 2238 Rosette Nebula

NGC 2238 Rosette Nebula
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NGC 2238 Rosette Nebula

The cluster and nebula lie at a distance of 5,000 light-years from Earth[5] and measure roughly 130 light years in diameter. The radiation from the young stars excites the atoms in the nebula, causing them to emit radiation themselves producing the emission nebula we see. The mass of the nebula is estimated to be around 10,000 solar masses.
SPECIFICATIONS
Telescope ..........................................................................................................................................................................................................................
Telescope
William Optics 71
Camera ..........................................................................................................................................................................................................................
Camera
ZWO ASI533 MM
Location ..........................................................................................................................................................................................................................
Location
Mill Park VIC
Date of observation ..........................................................................................................................................................................................................................
Date of observation
Sep 18, 24
Filters ..........................................................................................................................................................................................................................
Filters
Antlia 4.5nm Narrowband H-Alpha (Ha) EDGE , Oxygen III (OIII) EDGE, Sulfur II (SII) EDGE.
Processing ..........................................................................................................................................................................................................................
Processing
Adobe Photoshop, Pixinsight
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