Messier 97 in Ursa Major, the Owl Nebula
Messier 97, M97 or the Owl Nebula, is a planetary nebula
formed by the death of a star similar to our own sun.
The central star has ~60% solar mass but has 100
times the luminosity of our sun. M97 has
a radius of ~0.1 ly, and is 2.0 kly from us.
Hover over the image for an annotated view.
Date: 8 March 2026
FOV: cropped to 15' × 10'; M97 is about 3.3'
Rotation: −90.256°
Telescope: Celestron C14 SCT (3910mm, f/11)
Starizona SCT Coma Corrector/Reducer (2652.5mm, f/7.5)
Guiding: ZWO183 MM
Computer: ASIair plus 256GB
Mount: iOptron CEM120
Camera: ZWO ASI2600MC Pro Cooled (0°C) Color CMOS with gain 100
Pixel size: 3.76 μm
Resolution: 0.292 arcsec/pixel
Filter: Optolong UV/IR
Stacking: thirty-eight 300 second frames using PixInsight
Calibration frames: 20 dark, 20 flat, 20 dark flat
Total Time: 3 hours 10 minutes
Processing: Pixinsight – SPCC, DBE, SPCC, BlurXT, NoiseXT → Linear
HTS, GHS, MStr, PixelMath MStr + GHS + HST → Stars,
Linear, StarXT, HTS, GHS, MStr,
PixelMath MStr + GHS + HST → Starless
HDRMST_6_PhLm,
PixelMath ~(~Starless*~Stars) → Blend
Location: Darling Hill Observatory in Vesper, NY