Celestial hemisphere:  Northern  ·  Constellation: Canes Venatici (CVn)  ·  Contains:  M 94  ·  NGC 4736
Spiral Galaxy Messier 94 (M94), Tom Wildoner
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Spiral Galaxy Messier 94 (M94)

Spiral Galaxy Messier 94 (M94), Tom Wildoner
Powered byPixInsight

Spiral Galaxy Messier 94 (M94)

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Description

This is the spiral galaxy named Messier 94 (M94 or NGC 4736) found in the constellation Canes Venatici. It has an apparent magnitude of 8.99 and is about 16 million light-years away from Earth.

From NASA - New stars are forming at a high rate within the bright ring. This region is known as a starburst ring. The cause of this peculiarly shaped star-forming region is likely a pressure wave traveling outward from the galactic center, compressing the gas and dust in the outer regions. The compression of material means the gas starts to collapse into denser clouds. Inside these dense clouds, gravity pulls the gas and dust together until the temperature and pressure are high enough for stars to be born.

Observation data (Epoch J2000)
Constellation: Canes Venatici
Right ascension: 12h 50m 53.1s
Declination: +41° 07′ 14″
Apparent dimension (V): 11.2’ × 9.1’
Apparent magnitude (V): 8.99

Tech Specs: Orion 8" f/8 Ritchey-Chretien Astrograph Telescope, Celestron CGEM-DX pier mounted, ZWO ASI290MC and ASI071MC-Pro, ZWO AAPlus, ZWO EAF, 66 x 60 seconds at -10C plus darks and flats, processed using PixInsight and DSS. Image Date: January 26, 2022. Location: The Dark Side Observatory, Weatherly, PA, USA (Bortle Class 4).

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Spiral Galaxy Messier 94 (M94), Tom Wildoner