The Pinwheel Galaxy, also known as Messier 101, is a grand design spiral galaxy situated in the constellation Ursa Major. Due to its face-on orientation and expansive spiral arms, it offers an ideal subject for deep-sky imaging, particularly for capturing galactic structure in high resolution. From an imaging perspective, the galaxy’s extended disk and subtle features demand long integration times and dark skies to bring out low surface brightness details. Capturing the full breadth of its spiral arms, which are laced with star-forming regions and dust lanes, requires wide-field imaging setups or precision mosaicking for narrower fields of view.
Narrowband imaging is less commonly applied to galaxies like M101 compared to emission nebulae, but H-alpha filters can be particularly useful for isolating ionized hydrogen regions scattered throughout the spiral arms. These regions, rich in star formation, stand out when H-alpha data is layered over broadband LRGB exposures, providing a hybrid approach that enhances both structural and emission-line features. High-sensitivity sensors with low read noise and high quantum efficiency are critical to preserving faint details in the outer spiral arms, which can be easily lost in light pollution or insufficient exposure depths. Accurate color calibration and flat-field correction become essential in post-processing to ensure true representation of the galaxy’s diverse components.
Given M101’s angular size, capturing its intricate core and peripheral arms in high resolution benefits from telescopes with excellent tracking and stable mounts, especially when working at longer focal lengths. Dithering between exposures and using drizzle integration during stacking can help mitigate undersampling and enhance fine detail resolution. Astronomers often complement their optical imaging with ultraviolet or infrared observations to analyze stellar populations and dust content across the galaxy. For both professional and amateur astronomers, imaging the Pinwheel Galaxy represents a technical and aesthetic challenge, rewarding patient acquisition and meticulous processing with a vivid portrait of one of the Local Group’s most photogenic galaxies.
Object | Pinwheel Galaxy (M101) |
Link | https://www.shetzers.com/pinwheel-galaxy-m101-2/ |
Wiki Link | https://en.wikipedia.org/wiki/Pinwheel_Galaxy |
Hemisphere | Northern |
Constellation | Ursa Major |
Other Names contained in image | M101, NGC 5457 |
Imaging telescopes or lenses | Takahashi TOA-130NFB |
Imaging cameras | QHY268M |
Mounts | Astro Physics 1600 |
Focal reducers | None |
Software | N.I.N.A., AP Drivers, PHD Lab PHD2, Viking, PixInsight, Photoshop, Lightroom |
Filters | Astrodon LRGB Gen2 E-Series Tru-Balance 36mm unmounted. Chroma Technology Narrowband 3nm Ha, SII, OIII – 36mm Unmounted |
Accessories | Moonlite NightCrawler 35 focuser, Maxdome II, Digital Loggers Pro Switch, Sky Alert Weather Station, Pegagsus Ultimate Powerbox v2, QHY 7-slot filter wheel. |
Guiding Telescope or Lenses | Orion 60mm Guide Scope |
Guiding Camera | ZWO ASI290MM Mini |
Imaging Dates | 3/1/24, 5/15/24, 5/16/24, 5/17/24, 6/8/24, 6/9/24, 6/12/24, 7/2/24, 7/3/24, 7/4/24, 7/5/24, 7/6/24, 7/7/24, 7/8/24, 7/9/24, 7/31/24 |
Frames | Ha:22×600″ (3.7h) Gain 56, High Gain Mode, Temp -25C, Bin 1×1 Luminance: 62×180″ (3.1h) Gain 26, High Gain Mode, Temp -25C, Bin 1×1 Red: 58×300″ (4.8h) Gain 26, High Gain Mode, Temp -25C, Bin 1×1 Green: 57×300″ (4.8h) Gain 26, High Gain Mode, Temp -25C, Bin 1×1 Blue: 55×300″ (4.6h) Gain 26, High Gain Mode, Temp -25C, Bin 1×1 |
Integration | 21h |
Darks | 50 |
Flats | 20 per Filter |
Flat Darks | 40 |
Bortle Dark-Sky Scale: | 2 |
RA center | 210.8001 |
DEC center | 54.34128 |
Pixel scale | 3.76 |
Resolution | 6280 x 4210 |
Locations | Sirus 3.5m Observatory, Carbondale Colorado |
Data source | Colorado Starry Nights Observatory |
Seeing | Average |
Post Processing Techniques | PixInsight to Photoshop to Lightroom |
Type | LRGB with Ha |