Introduction | Map | Find/Identify | Sketch | My Best Own Photos | My Own Observations | References || Appendix: My Own Photos
On this page I collect my observations of the galactic emission nebula (supernova remnant) M 1 (Crab Nebula; NGC 1952) in the constellation Taurus / Bull.
Taurus / Bull is another constellation that I only knew by its name. Thanks to the Hyades (Mel 25), it has now become more familiar to me - at least its star Aldebaran, which glares conspicuously yellow (or golden). While the Hyades are at the center of Taurus, the galactic emission nebula M 1 (NGC 1952), also known as Crab Nebula, is located at its left end and slightly above the end star zeta Tauri. It is famous for being a supernova remnant from 1054.
M 1 (NGC 1952):
Size: 5 'x 4' / 6' (Stoyan / Karkoschka)
Distance: 6,200 light years (Stoyan)
Rating: *** (Stoyan)
Note: NGC 6960/6992/5 (Cirrus or Veil Nebula), M 1 (Crab Nebula), and IC 443 (Jellyfish Nebula) are the only supernova remnants that I have observed so far.
M 1 (Crab Nebula) between Gemini / Twins and Taurus / Bull and below Elnath in Auriga (Image Courtesy of SkySafari Astronomy, www.simulationcurriculum.com)
Find: While the Hyades are at the center of Taurus, the galactic emission nebula M 1 (NGC 1952), also known as Crab Nebula, is located at its left end and slightly above the end star zeta Tauri (and nearly on the connecting line between zeta Tauri and Elnath). Whenever you see a faint glow in the eyepiece, you found M 1!
Identify: If the galactic emission nebula M 1 in the constellation Taurus was found in the way described above, it is also identified. (Image Courtesy of SkySafari Astronomy, www.simulationcurriculum.com)
The sketch by Michael Vlasov (DeepSkyWatch.com) provides a rough impression of what I observed (my impression was much fainter than the sketch):
Sketch of the Crab Nebula by Michael Vlasov (Copyright © Michael Vlasov 2016)
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M 1 (Taurus), post-processed and noise removed |
Ditto,post-processed and noise removed |
Ditto, post-processed and noise removed |
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M 1 - Jan 28, 2020, processed |
M 1 - Jan 28, 2020, processed |
M 1 - Mar 22, 2020, processed |
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M 1 - Mar 6, 2021, processed |
M 1 - Mar 6, 2021, processed |
M 1 - Mar 6, 2021, processed |
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M 1 - Feb 7, 2023, 784 s |
M 1 - Feb 7, 2023 - photo left processed |
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M 1, Jan 9, 2024 - original (179 frames = 1790 s) |
M 1, Jan 9, 2024 - large (179 frames = 1790 s), photo left processed |
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M 1, Jan 26, 2024 - original (149 frames = 1490 s), CLS Filter |
M 1, Jan 26, 2024 - large (149 frames = 1490 s), CLS Filter, photo left processed |
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M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section |
M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section, photo left processed |
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M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section, processed and denoised (DN) |
M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section, processed and denoised (DN) |
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M 1, Feb 18, 2025 - 1800 (180 frames = 30 min), section |
M 1, Feb 18, 2025 - 1800 (180 frames = 30 min), section, photo left processed |
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M 1, Feb 18, 2025 - 1800 (180 frames = 30 min), section, processed and denoised (PAI) |
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M 1, Feb 7, 2023 - original (181 frames = 1810 s) |
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M 1, Jan 9, 2024 - original (179 frames = 1790 s) |
M 1, Jan 9, 2024 - large (179 frames = 1790 s), photo left processed |
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M 1, Jan 26, 2024 - original (149 frames = 1490 s), CLS Filter |
M 1, Jan 26, 2024 - large (149 frames = 1490 s), CLS Filter, photo left processed |
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M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section |
M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section, photo left processed |
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M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section, processed and denoised (DN) |
M 1, Nov 4, 2024 - 1800 (180 frames = 30 min), section, processed and denoised (DN) |
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M 1, Feb 18, 2025 - 1800 (180 frames = 30 min), section |
M 1, Feb 18, 2025 -1800 (180 frames = 30 min), section, photo left processed |
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M 1, Feb 18, 2025 - 1800 (180 frames = 30 min), section, processed and denoised (PAI) |
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