Celestial hemisphere:  Northern  ·  Constellation: Ursa Major (UMa)  ·  Contains:  M 101  ·  NGC 5451  ·  NGC 5455  ·  NGC 5457  ·  NGC 5461  ·  NGC 5471
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Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf, Tim Hawkes
Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf
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Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf

Getting plate-solving status, please wait...
Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf, Tim Hawkes
Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf
Powered byPixInsight

Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf

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Description

Combined image from 2 Newtonian telescopes.  2.5h  OSC camera RGB image of M101 at F5.0 and f 1000mm  combined with 40 min of an F4.0 , f = 1200 mm image with part of a 1h HA mono camera image added back into the red channel to emphasise HA regions.

103 of the 251 frames were taken at a darker (Bortle 4) site than the rest (Bortle 6) - moonless on both occasions.  The frames from the darker site were weighted considerably more highly in the overall integration according to their  SNR .

The luminance of the above was replaced with that from 193 x 40s AS1294MM exposures at high resolution (0.405 arcsec/ pixel) to show the May 2023 supernova.

M101 is visible as a large face on spiral galaxy.  It is about 21M ly distant and  comprises about a trillion stars.   Somewhat similar to the Andromeda galaxy It has a disk mass on the order of 100 billion solar masses, along with a small central bulge of about 3 billion solar masses.M101 has a high population  - more than  1200_ of HII regions many of which are very large and bright, three bright enough to be separately classified as NGC 5461, NGC 5462, and NGC 5471.M101 is asymmetrical due to the tidal forces from interactions with its companion galaxies which also triggers star formation in the spiral arms_ and for the largest of these sometimes triggers Type II core collapse supernovae.   

The most recent of these supernovae - first recorded on 19 May 2023 - is shown in this image - at an estimated (approximate by me) visible magnitude of ~ 11.75 on 26 May 2023. It is located near  NGC 5461, a prominent HII region in an outer spiral arm of the bright galaxy.  Accounting for the 21 M ly distance the visible light output can be estimated as ~ 800 million x solar.

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  • Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf, Tim Hawkes
    Original
  • Final
    Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf, Tim Hawkes
    C

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Newtonian RGBHa image of M101 - modified with 26 May 2023 luminance to show SN2023ixf, Tim Hawkes