The Elephant's Trunk Nebula is a concentration of interstellar gas and dust within the much larger ionized gas region catalogued as IC 1396; it is located in the constellation Cepheus about 2,400 light years away from Earth. It is thought to be a site of star formation, containing several very young (less than 100,000 yr) stars that were discovered in infrared images in 2003. Two older (but still young, a couple of million years, by the standards of stars, which live for billions of years) stars are present in a small, circular cavity in the head of the globule. Winds from these young stars may have emptied the cavity.

The combined action of the light from the massive star ionizing and compressing the rim of the cloud, and the wind from the young stars shifting gas from the center outward lead to very high compression in the Elephant's Trunk Nebula. This pressure has triggered the current generation of protostars.

This target is beyond the effective abilities of my small telescope.The trunk feature itself cannot really be made out at all.