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About this Object
Discovered by John Russell Hind in 1852, Hinds varialble nebula is just to the west of the variable star T-Tauri. T Tauri shines at magnitude 9-13 and is a fairly young star formed out of the cloud of dust which surrounds this area. The dust is faintly visible in the image just to the north of T-Tauri and extending south to the edge of the field. NGC 1555 is generally thought to be a reflection nebula which relects the color of the star T-Tauri. The dust in this area is slowly being eaten away by radiation from the star. A dark hole appears surriounding the star which seems to indicate the continuation of this process.

Image Details

Optics : Stellarvue SV 105 Triplet Refracter
Mount: Mountain Instruments MI-250
Camera: Starlight Xpress SXV-H9 w/True Tech Supra Slim filter wheel
Filters: Astronomik Type 2C LRGB filter set
Exposure: 380:90:90:80
Camera/Mount Control: Maxim DL 4.56, CCD Commander
Location: Stark Bayou Observatory, Ocean Springs, MS
Date: Feb 09