NGC 1579 is a compact reflection nebula embedded within the Perseus molecular cloud. Located about 2,000 light-years away, it glows with light scattered by dust grains rather than ionized gas emission. Dense lanes of obscuring dust carve intricate shapes, hinting at ongoing star formation hidden within. The region hosts clusters of newborn stars, making it a laboratory for early stellar evolution. (AI description)
Acquisition Details
LUM = 65x10min
RGB = 36x10min each
Total = 28hrs 50min
