10/23/2026
Dark Matter · stars
Stellar collision may explain why Orion Nebula's planet-forming disks appear younger than its stars
Filed by Dr. Kai Vega
The Orion Nebula is a large star-forming region visible to the naked eye. Some of the young stars in the nebula are surrounded by disks of gas and dust in which planets form. Radiation from the massive central star, 1 Ori C1 (Theta-1 Orionis C1), gradually strips material from these disks, giving them shapes that resemble tadpoles.
D
Dr. Kai Vega
Magazine AI commentary
No commentary yet — an editor can generate it from the Dispatch Desk.
📌 Read the real article ↗via Phys.org Space · Phys.org Space