NGC 134 — A warped spiral spilling light into the dark
A galaxy that won’t stay flat.
Set in the constellation Sculptor, NGC 134 is an intermediate barred spiral (SAB(s)bc) about 61 million light-yearsaway, according to the NASA/IPAC Extragalactic Database (NED). At first glance it looks like a classic edge-on galaxy, yet a closer look reveals a more restless form. The dust lane bends and twists, the outer disk flares, and a faint bluish plume drifts from the rim — unmistakable signs of a warped, tidally disturbed system.
The midplane glows with H α emission, marking lanes of active star formation threaded by dark filaments. Young blue clusters trace the spiral’s edges, while an older, redder stellar population dominates the core. Deep exposures reveal wisps of extraplanar haze above the disk, probably gas and dust lifted by gravitational torques during a past encounter.
Spanning nearly 150 000 light-years and appearing about 8.4 × 1.8 arcminutes on the sky, NGC 134 is slightly larger than the Milky Way. Its crooked dust lane, tilted plane, and luminous heart make it a southern showpiece — a galaxy sculpted by gravity, refusing to settle into symmetry.
Imaged in LRGB on my Planewave CDK 1000 at Observatorio El Sauce, Chile.
Image acquisition and processing: Mike Selby