Messier 36, 37, 38 (M 36, 37, 38)
Introduction | Map | Pseudo
Photo (Starry Night 7) | My Best Own Photos | My
Own Observations | References || Appendix:
My Own Photos
On this page I collect my observations of the open star clusters M 36 (NGC 1960), M
37 (NGC 2099), and M 38 (NGC 1912) in
the constellation Auriga.
Introduction
Auriga (with main star Capella) belonged to the constellations
that were more or less unknown to me at the beginning. At the core the constellation
forms a hexagon if you take it exactly, but it is likely that you will perceive
only a pentagon... This is a very striking pattern, but it is located very
high up sometimes (for example, in February), so you have to look steeply
upwards to see it. Perhaps this is a reason for my ignorance with respect
to it...
In Auriga there are three more striking Messier objects, the open
star clusters M
36, M 37, and M 38. They are located almost on a line, which projects
from the outside into the hexagon. The exact sequence is: M 37 (outside)
- M 36 Inside) - M 38 (further inside) (from East to West).
M 36 (NGC 1960) |
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M 37 (NGC 2099) |
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M 38 (NGC 1912) |
Size: 12' (Stoyan)
Distance: 3,300 light years (Stoyan)
Rating: *** (Stoyan) |
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Size: 16' (Stoyan)
Distance: 4,500 light years (Stoyan)
Rating: *** (Stoyan) |
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Size: 25' (Stoyan) - nearly moon size
Distance: 3,500 light years (Stoyan)
Rating: *** (Stoyan) |
Nearby, there are the nebulae IC 405 and IC 410 (see map below). IC 410 (with embedded open star cluster NGC 1893) can also be photographed together with M 36 (plus NGC 1931, IC 417) in a Vespera mosaic.
Map
M 37, M 36, and M 38 in constellation Auriga (large
overview map) (Image Courtesy
of SkySafari Astronomy, www.simulationcurriculum.com)
Pseudo Photo (Starry Night 7)
Pseudo photo of M 37, M 36, and M 38 created with Starry
Night 7 (large
version, larger
version) (Image Courtesy
of Starry Night Education, www.simulationcurriculum.com)
My Best Own Photos
eVscope
M 36
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M 36 - Nov 17, 2020 |
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M 36 - Nov 17, 2020 |
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M 36 - Nov 17, 2020, photo above processed |
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M 36 - Nov 17, 2020, photo above processed |
M 37
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M 37 - Nov 17, 2020 |
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M 37 - Nov 17, 2020 |
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M 37 - Nov 17, 2020, photo above processed |
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M 37 - Nov 17, 2020, photo above processed |
M 38
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M 38 - Nov 17, 2020 |
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M 38 - Nov 17, 2020 |
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M 38 - Nov 17, 2020, photo above processed |
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M 38 - Nov 17, 2020, photo above processed |
M 36, M 37, M 38 (Comparison)
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M 36 - Nov 17, 2020, processed |
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M 37 - Nov 17, 2020, processed |
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M 38 - Nov 17, 2020, processed |
Vespera
M 36, M 37, M 38
M 36 and M 38 (plus IC 417, NGC 1907, NGC 1931)
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M 36/38, Feb 7, 2023 - original, 4950s, mosaic |
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Ditto, evaluation with astrometry.net |
M 36 and IC 410 (plus NGC 1931, IC 417, NGC 1893)
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M 36 & IC 410, Feb 29, 2024 - original, 6830s, mosaic, CLS Filter |
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M 36 & IC 410, Feb 29, 2024 - large, 6830s, mosaic, CLS Filter, processed (PSE, DN) |
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Evaluation with nova.astrometry.net |
My Own Observations
Observations February 2017
- February 13, 2017 (Mühlhausen/Kraichgau: Heritage
100P, LT binoculars):
Looked for all three star clusters, and found two of them without a doubt,
namely the inner clusters M 36 (which is regarded as the most
beautiful and therefore probably got the lowest number "36")
and M 38. I was able to find M 36 more easily and reproducible,
whereas I had some problems with finding M 38. But despite all my efforts,
I was not able to find M 37.*
- February 14, 2017 (ditto: GSO GSD 680, LT binoculars):
The attempts with my GSD 680 showed another pattern: I did not find M
38, but found M 37 and M 36. M 37 appeared to me more
beautiful this time, and M 36 not quite as beautiful.
- February 15, 2017: (ditto: Heritage
100P on GoTo mount, LT binoculars):
I found all three open star clusters thanks to the GoTo mount. This time
my verdict was: M 36 appeared to me most beautiful, M 38 came
in second, and M 37 was a little fainter than the other two clusters...
- February 26, 2017: (ditto: Heritage
P130 on GoTo mount): I once
again accessed all three open star clusters with the Heritage P130 on
the GoTo mount and found them all. M 36 was the smallest, but
brightest cluster with comparatively few stars, M 37 was relatively
faint and in small magnification almost just a glimmer, whereas M
38 was the largest cluster, but also fainter than M 36 (new moon).
- March 16, 2017: (ditto): M 36, M 37, and M 38 observed
but no details noted
The visibility and rating of the three star clusters thus fluctuated quite
a bit. But at least one can state that all the three star clusters were more
or less well recognizable even when using a 4" telescope.
*) Whether this was due to a wrong alignment of the telescope, I do not
know. In any case, it was very difficult for me to point the LED finder at
these three targets because they were so high up in the sky. I therefore
tried it on "good luck". Here a 90° angle finder would surely
have served me well!
Observations End of March 2017
- 30.3.2017 (Mühlhausen/Kraichgau: Heritage
P130 on GoTo mount):
All three star clusters observed
Observations February to April 2018
- February 12, 2018 (Mühlhausen/Kraichgau: Explorer
150PDS on GoTo mount with Atik
Infinity, StarSense): M
36-38 for the first time photographed
- February 13, 2018 (Mühlhausen/Kraichgau: TS binoculars): M
36-38 seen well with binoculars as a shimmering spots of different
sizes
- March 18-19, 2018 (Kellinghusen and Erkerode, TS binoculars): M
36-38 observed with binoculars, seen nicely (the center cluster was
the smallest and somewhat lower, the right one the largest, the left
one in between).
- April 8, 2018 (Mühlhausen/Kraichgau: Explorer
150PDS on GoTo-Mount with Atik
Infinity, StarSense): M
36-38 photographed, but only M 36 found when looking for M 38...
Observations February 2019 ff
- February 27, 2019 (Mühlhausen/Kraichgau: PS
72/432 on AZ
Pronto Mount, TS binoculars): M
37 was very small with 24 mm, "normal" at higher magnification
(7 mm).
- April 28, 2019 (Mühlhausen/Kraichgau: PS
72/432 on GoTo mount): M
36, M 37, and M 38 were very faint with 10 mm.
- May 1, 2019 (Mühlhausen/Kraichgau: Explorer
150PDS on GoTo mount): M
36, M 37, and M 38 were faint and fine, but
better than in the PS 72/432.
Observations January to May 2020
- January 16, 2020 (Mühlhausen/Kraichgau: C8 on Star
Discovery mount (SynScan WLAN, iPhone)): M 37, M 36, M 38 first
observed with C8R and 24 as well as 32 mm eyepieces (1,25")
- very nice (M 38 showed a "cross", M 36 distributed, M 37 fine,
many stars).
Ditto observed without reducer (2"); very nice again, somewhat larger field
of view, that appeared somewhat nicer.
- February 5, 2020 (Mühlhausen/Kraichgau: eVscope): M
36 and M 38 photographed
- February 15-16, 2020 (Mühlhausen/Kraichgau: eVscope): M
36-M 38 photographed
- March 13 and 18, 2020 (Mühlhausen/Kraichgau: eVscope): M
36-M 38 photographed
- May 10, 2020 (Mühlhausen/Kraichgau: eVscope): M
37 photographed; very hard to observe and photograph (Unistellar
task; moon too bright, M 37 too low)
Observations November 2020
- November 17, 2020 (Mühlhausen/Kraichgau: eVscope): M
36, 37, 38 photographed in the new rectangular format without overlay
Observations January to February 2021
Observations March to April 2022
- March 20, 2022 (Mühlhausen/Kraichgau: eVscope 2): M 36, M 37, M 38 photographed (app version 1.5)
- April 9, 2022 (Mühlhausen/Kraichgau: eVscope 2): M 38 photographed (app version 1.5)
Observations February 2023
- February 7, 2023 (Mühlhausen/Kraichgau: Vespera): M 36 and M 38 photographed together (mosaic)
- February 13, 2023 (Mühlhausen/Kraichgau: Vespera): M 36, M 37, and M 38 photographed alone
Observations March 2024
- March 29, 2024 (Mühlhausen/Kraichgau: Vespera): M 36 and IC 410 photographed together (mosaic); plus NGC 1931, IC 417, NGC 1893 (embedded in IC 410)
References
On this Site
Appendix: My Own Photos
Atik Infinity & Explorer 150PDS (February 12, 2018)
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M 36 (Auriga), unprocessed |
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Ditto, post-processed and sharpened |
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Ditto, post-processed more aggressively and sharpened |
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M 37 (Auriga), unprocessed |
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Ditto, post-processed and sharpened |
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Ditto, post-processed more aggressively and sharpened |
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M 38 (Auriga), unprocessed |
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Ditto, post-processed and sharpened |
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Ditto, post-processed more aggressively and sharpened |
Photos taken with Sky-Watcher Explorer 150PDS (February 12, 2018), 600 x
600 section with 1:1 pixels in the large version
Atik Infinity & Explorer 150PDS (April 8, 2018)
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M 36 (Auriga), unprocessed |
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Ditto, post-processed |
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Ditto, post-processed and sharpened |
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M 36 (Auriga), unprocessed |
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Ditto, post-processed |
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Ditto, post-processed and sharpened |
Photos taken with Sky-Watcher Explorer 150PDS (April 8, 2018), originals
reduced to 600 x 450 pixels; found M 36 when looking for M 38...
eVscope
M 36
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M 36 - Feb 15, 2020 |
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M 36 - Feb 16, 2020 |
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M 36 - Mar 13, 2020 |
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M 36 - Mar 13, 2020 |
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M 36 - Mar 18, 2020 |
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M 36 - Mar 18, 2020, photo left processed |
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M 36 - Nov 17, 2020 |
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M 36 - Nov 17, 2020 |
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M 36 - Nov 17, 2020, photo above processed |
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M 36 - Nov 17, 2020, photo above processed |
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M 37
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M 37 - Feb 15, 2020 |
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M 37 - Feb 16, 2020 |
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M 37 - Mar 13, 2020 |
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M 37 - Mar 18, 2020 |
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M 37 - Mar 18, 2020, processed |
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M 37 - May 10, 2020, processed (Live View) |
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M 37 - Nov 17, 2020 |
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M 37 - Nov 17, 2020 |
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M 37 - Nov 17, 2020, photo above processed |
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M 37 - Nov 17, 2020, photo above processed |
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M 38
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M 38 - Feb 15, 2020, manual exposure |
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M 38 - Feb 15, 2020 |
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M 38 - Feb 16, 2020 |
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M 38 - Mar 13, 2020 |
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M 38 - Mar 18, 2020 |
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M 38 - Mar 18, 2020, processed |
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M 38 - Nov 17, 2020 |
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M 38 - Nov 17, 2020 |
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M 38 - Nov 17, 2020, photo above processed |
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M 38 - Nov 17, 2020, photo above processed |
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eVscope 2
M 36
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M 36 - Mar 20, 2022 |
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M 36 - Mar 20, 2022, photo left processed |
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M 37
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M 37 - Mar 20, 2022 |
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M 37 - Mar 20, 2022, photo left processed |
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M 38
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M 36 - Mar 20, 2022 |
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M 36 - Mar 20, 2022, photo left processed |
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M 38 - Apr 9, 2022 |
Vespera
M 36, M 37, M 38
M 36 and IC 410 (plus IC 417, NGC 1907, NGC 1931)
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M 36/38, Feb 7, 2023 - original, 4950s, mosaic |
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Ditto, evaluation with astrometry.net |
M 36 and IC 410 (plus NGC 1931, IC 417, NGC 1893)
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M 36 & IC 410, Feb 29, 2024 - original, 6830s, mosaic, CLS Filter |
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M 36 & IC 410, Feb 29, 2024 - large, 6830s, mosaic, CLS Filter, processed (PSE, DN) |
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Evaluation with nova.astrometry.net |