Triangulum Galaxy
"They point and marvel, calling me their neighbor. As if they could ever truly cross the distance, bridge the gap between their world and mine."
“An Autumn Evening with the Pinwheel of Triangulum”
On 24 October 2024 a brilliant, 92 % gibbous Moon arched over the northern treetops. Most of the night-sky crowd headed indoors—moon-wash is the sworn enemy of faint galaxies, after all. Yet the CGEM mount whirred into life at 20:30, slewing the 80 mm refractor toward a patch of sky so dim it looked empty. The target sat three million light-years away:
Messier 33, the Triangulum Galaxy—compact, blue-tinged, restless with newborn suns.
I. A Spiral without a Heart
Unlike the Milky Way or Andromeda, M 33 sports no central bulge. Its disc is a playground of loosely wound arms humming with star-forming regions, the most famous of which—NGC 604—is large enough to swallow dozens of Orion Nebulae. Astronomers suspect Triangulum may be gravitationally flirting with Andromeda (and, by extension, us), a slow dance that could someday knit the Local Group’s three big spirals into one.
Angular size: 71 × 42 arc-minutes—stretching wider on the sky than the full Moon.
True span: ~60 000 light-years.
Brightness: Mag 5.7 (bright on paper, but surface-brightness low enough to drown in moonlight).
II. Harvesting Photons under a Moon-Bright Sky
L 90 60 1.5
R 30 60 0.5
G 30 60 0.5
B 30 60 0.5
H-α 20 300 1.7
Total integration ≈ 4.7 h
Guiding: 0.72″ RMS—steady as a metronome in 5 km h⁻¹ breezes.
Camera: ASI294MM Pro at –10 °C.
Filters: Antlia LRGB-V plus 3 nm H-α for the scarlet star-nurseries.
A perfect meridian flip at midnight and frequent autofocus tweaks kept stars needle-sharp despite an 8 °C chill.
III. Digital Alchemy
Calibrate & stack in PixInsight (20 flats, darks, flat-darks per channel).
Process LRGB first—dust off the workflow, stretch the faint outer arms until they glow silver-blue.
Blend H-α using an “L-enhance” trick: sprinkle the 3 nm data into the red channel, then pop the giant nebulae without overwhelming the galaxy’s pastel tones.
Local contrast (using HDRMT) teased out mottled dust lanes; star-size masks kept halos in check.
Final polish: gentle star reduction and a tiny dash of SCNR to tame Moon-induced gradients.
After two attempts the galaxy floated on-screen: spiral arms afire with pink H-II knots, a bluish starlight whirlpool with no bright core—Triangulum wearing its eternal youth like a badge.
IV. What the Session Taught
Moonlight isn’t fatal—short, rapid LRGB subs plus a deep H-α layer can out-smart a 93 % Moon.
Compact gear, big pay-off—an 80 mm scope and 60-second exposures drew out a galaxy 3 million light-years away.
Dynamic galaxies matter—M 33’s bulge-less disc hints we’re watching a spiral still growing, still assembling its identity.
By 03:00 the script parked the scope, and dew sparkled on the equipment.
On the monitor, Triangulum spun in delicate blues and rose-petal reds—a cosmic pinwheel frozen in time, bearing postcards from stellar nurseries that ignited when humanity’s ancestors were still fashioning stone tools.