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Stephan's Quintet, attended from my back patio, Sept-Nov, 2024. The quintet is composed of several galaxies, NGC 7317 (upper left), NGC 7318A & NGC 7318B (center-left), NGC 7320 (center-upper-right), and NGC7319 (center-lower-right). Also in the image is NGC 7320C (far lower-right).
One of these galaxies is not like the others. Can you tell which one? It's NGC 7320 (center-upper-right), the one that looks blueish-white. That's because it's much closer to us than the other galaxies. The other gravitationally connected galaxies are about 210-240 million light-years away, while NGC 7320 is only a mere 39 million light-years away. The much smaller NGC 7320 is photobombing the other galaxies.
It's a bit like taking a snapshot of your friends, only to have your pet tarantula, much closer to your camera, jump into the frame in such a way that at a glance it appears human sized. It's sort of like that. Except your friends and tarantula are galaxy sized.
The purplish-red splotches in NGC 7320 are highlighted from data obtained with my Hα (hydrogen-alpha) filter. That's from emission nebulae within the NGC 7320 galaxy itself. After subtracting out the broadband red data, it was the only galaxy (in this particular image) showing such Hα specific emissions. That's not to say that the other galaxies don't have Hα emissions (or nebulae), but if they do, the spectrum is shifted outside the passband of my Hα filter due to cosmological redshift (i.e., the universe's expansion).
So if you've ever wondered what cosmological redshifted galaxies look like compared to a much closer galaxy in the foreground, here you go.
In retrospect, that gives me an idea: My back-of-the-envelope calculations suggest that the cosmological redshift of the other galaxies might serendipitously shift their Hα emissions into the passband of another filter I own (my SII [sulphur-II] filter). It's too late to gather more data now, but perhaps I'll revisit this target in the future with that in mind.
Equipment:
Celestron C14 EdgeHD telescope
SkyWatcher EQ8-R Pro mount
Celestron 0.7x Focal reducer (for C14 EdgeHD)
Off-axis guider (OAG) with guide camera
Baader LRGB filter set
Antlia Hα filter
ZWO ASI6200MM-Pro Main Camera
Software:
N.I.N.A.
PHD2 Guiding
PixInsight with
o RC-Astro Plugins
o SkyPixels "GAME" plugin
Acquisition/Integration:
Location: San Diego, USA
Bortle Class 7 (maybe 8 ) skies
All subframes binned 2×2
Stacked using drizzle algorithm
L: 714×60 sec = 11.90 hrs
R: 378×120 sec = 12.60 hrs
G: 396×120 sec = 13.20 hrs
B: 319×120 sec = 10.63 hrs
Hα: 62×600 sec = 10.33 hrs
Total integration time: 58.67 hours
.
One of these galaxies is not like the others. Can you tell which one? It's NGC 7320 (center-upper-right), the one that looks blueish-white. That's because it's much closer to us than the other galaxies. The other gravitationally connected galaxies are about 210-240 million light-years away, while NGC 7320 is only a mere 39 million light-years away. The much smaller NGC 7320 is photobombing the other galaxies.
It's a bit like taking a snapshot of your friends, only to have your pet tarantula, much closer to your camera, jump into the frame in such a way that at a glance it appears human sized. It's sort of like that. Except your friends and tarantula are galaxy sized.
The purplish-red splotches in NGC 7320 are highlighted from data obtained with my Hα (hydrogen-alpha) filter. That's from emission nebulae within the NGC 7320 galaxy itself. After subtracting out the broadband red data, it was the only galaxy (in this particular image) showing such Hα specific emissions. That's not to say that the other galaxies don't have Hα emissions (or nebulae), but if they do, the spectrum is shifted outside the passband of my Hα filter due to cosmological redshift (i.e., the universe's expansion).
So if you've ever wondered what cosmological redshifted galaxies look like compared to a much closer galaxy in the foreground, here you go.
In retrospect, that gives me an idea: My back-of-the-envelope calculations suggest that the cosmological redshift of the other galaxies might serendipitously shift their Hα emissions into the passband of another filter I own (my SII [sulphur-II] filter). It's too late to gather more data now, but perhaps I'll revisit this target in the future with that in mind.
Equipment:
Celestron C14 EdgeHD telescope
SkyWatcher EQ8-R Pro mount
Celestron 0.7x Focal reducer (for C14 EdgeHD)
Off-axis guider (OAG) with guide camera
Baader LRGB filter set
Antlia Hα filter
ZWO ASI6200MM-Pro Main Camera
Software:
N.I.N.A.
PHD2 Guiding
PixInsight with
o RC-Astro Plugins
o SkyPixels "GAME" plugin
Acquisition/Integration:
Location: San Diego, USA
Bortle Class 7 (maybe 8 ) skies
All subframes binned 2×2
Stacked using drizzle algorithm
L: 714×60 sec = 11.90 hrs
R: 378×120 sec = 12.60 hrs
G: 396×120 sec = 13.20 hrs
B: 319×120 sec = 10.63 hrs
Hα: 62×600 sec = 10.33 hrs
Total integration time: 58.67 hours
.