Celestial hemisphere:  Northern  ·  Constellation: Ursa Major (UMa)  ·  Contains:  M 101  ·  NGC 5447  ·  NGC 5449  ·  NGC 5450  ·  NGC 5451  ·  NGC 5453  ·  NGC 5455  ·  NGC 5457  ·  NGC 5461  ·  NGC 5462  ·  NGC 5471  ·  NGC 5477  ·  Pinwheel galaxy
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THE SUPERNOVA IN THE PINWHEEL GALAXY - Face-on Spiral Galaxy & Supernova - Deepsky 2541mm LRGBhA - Constellation Ursar Major, Thomas ArtOfPix Großschmidt
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THE SUPERNOVA IN THE PINWHEEL GALAXY - Face-on Spiral Galaxy & Supernova - Deepsky 2541mm LRGBhA - Constellation Ursar Major

Getting plate-solving status, please wait...
THE SUPERNOVA IN THE PINWHEEL GALAXY - Face-on Spiral Galaxy & Supernova - Deepsky 2541mm LRGBhA - Constellation Ursar Major, Thomas ArtOfPix Großschmidt
Powered byPixInsight

THE SUPERNOVA IN THE PINWHEEL GALAXY - Face-on Spiral Galaxy & Supernova - Deepsky 2541mm LRGBhA - Constellation Ursar Major

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Description

THE SUPERNOVA IN THE PINWHEEL GALAXY
- Face-on Spiral Galaxy & Supernova
- Deepsky 2541mm LRGBhA
- Constellation Ursar Major

Messier 101, also known as the Pinwheel Galaxy, is a large spiral galaxy in the constellation Ursa Major. It is around 21 million light years away from Earth and is one of the brightest and most massive spiral galaxies in the Local Galaxy Group.
The Fire Wheel Galaxy has a striking spiral structure characterized by extended spiral arms. They extend far around the bright central region and are filled with numerous young, massive stars, star-forming regions and luminous gas clouds. The galaxy also has a relatively large and bright core.
With a diameter of around 170,000 light years, Messier 101 is one of the largest spiral galaxies we know of. It belongs to the classification of grand design spiral galaxies, as its spiral structure is particularly clear and symmetrical.
The galaxy is also known for its high rate of star formation. There are numerous areas of intense star formation in the spiral arms, where young, massive stars are formed. These stars radiate large amounts of energy and influence the environment by heating and ionizing gas and dust.

M101&SN2023ixf_SupernovaInPinwheelGalaxy_LRGBhA_Remotetelescope_2541mm-Crop1-facebook.jpg

SN 2023ixf is a type II supernova (core collapse) located in the Windmill Galaxy (M101). It was first observed on May 19, 2023 by Koichi Itagaki and immediately classified as a type II supernova. The supernova is about 21 million light years away from Earth and is expected to have left behind either a neutron star or a black hole, based on current models of stellar evolution.

M101&SN2023ixf_SupernovaInPinwheelGalaxy_LRGBhA_Remotetelescope_2541mm-Crop2-facebook.jpg

Telescope: ATFIL-15, PlaneWave CDK 12.5 f/8, 2541mm, Insight Observatory
Camera: ZWO ASI6200MM Pro, Chroma hA3nm, LRGB Astronomik
Mount: Software Bisque Paramount ME II GEM
Lights: 12xLuminance/13xRed/12xGreen/12xBlue each 300s Bin1x1
Lights: 05xhAlpha each 600s Bin1x1
Location: Beryl, Utah USA (Utah Desert Remote Observatories)
Acquired imageset, taken by Craig Stocks, Imageedit - Thomas ArtOfPix Großschmidt

Image processing:
Mainly Pixinsight, Photoshop, Lightroom, GraXpert, BTX Blur Terminator, Noise Terminator, Star X Terminator

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