Along the Taurus Molecular Cloud

Explanation: The cosmic brush of star formation composed this interstellar canvas of emission, dust, and dark nebulae. A 5 degree wide telescopic mosaic, it frames a region found north of bright star Aldebaran on the sky, at an inner wall of the local bubble along the Taurus molecular cloud . At lower left, emission cataloged as Sh2-239 shows signs of embedded young stellar objects. The region's Herbig-Haro objects, nebulosities associated with newly born stars, are marked by tell-tale reddish jets of shocked hydrogen gas. Above and right T Tauri, the prototype of the class of T Tauri variable stars , is next to a yellowish nebula historically known as Hind's Variable Nebula ( NGC 1555 ). T Tauri stars are now generally recognized as young, less than a few million years old, sun-like stars still in the early stages of formation .