V380 Orionis is a binary star system located in the constellation of Orion. It is approximately 1,500 light-years away from Earth and consists of two stars that orbit each other. The system is known for its variability, as the brightness of the stars changes over time. The primary star in V380 Orionis is a massive, hot star, while the secondary star is less massive and cooler. This binary system is also surrounded by a disk of gas and dust, which contributes to its complex behavior and makes it an interesting subject for astronomers studying stellar evolution and interactions.