Just like fog curling around a street lamp, reflection nebulae like NGC 1999 only shine because of the light from an embedded source. In the case of NGC 1999, this source is the aforementioned newborn star which is visible at the center of this image. Named V380 Orionis, this star is thought to be somewhere between 1 and 3 million years old. The most notable aspect of NGC 1999’s appearance, however, is the conspicuous hole in its center, which resembles an inky-black keyhole of cosmic proportions.
Just like fog curling around a street lamp, reflection nebulae like NGC 1999 only shine because of the light from an embedded source. In the case of NGC 1999, this source is the aforementioned newborn star which is visible at the center of this image. Named V380 Orionis, this star is thought to be somewhere between 1 and 3 million years old. The most notable aspect of NGC 1999’s appearance, however, is the conspicuous hole in its center, which resembles an inky-black keyhole of cosmic proportions.
This image was created from archival Wide Field Planetary Camera 2 (WFC2) observations that date from shortly after Servicing Mission 3A in 1999. At the time, astronomers believed that the dark patch in NGC 1999 was something called a Bok globule — a dense, cold cloud of gas, molecules, and cosmic dust that blots out background light. However, follow-up observations using a collection of telescopes including ESA’s Herschel Space Observatory revealed that the dark patch is actually an empty region of space. The origin of this unexplained rift in the heart of NGC 1999 remains unknown.
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