NASA James Webb Space Telescope (JWST)

N79 is a massive star-forming region located in the Large Magellanic Cloud (LMC), a satellite galaxy of our Milky Way. 

• The N79 complex spans approximately 1,630 light-years and is considered a younger version of the Tarantula Nebula (30 Doradus). 

• The image, specifically focusing on the N79 South (S1) region, was taken using JWST's Mid-InfraRed Instrument (MIRI). 

• Astronomers have identified 97 new young stellar objects (YSOs) within N79, highlighting its high efficiency in forming stars. 

• The vibrant colors represent the glow of ionized hydrogen gas and other interstellar material. 

• The distinct "starburst" pattern around the bright central object is a result of the telescope's diffraction spikes. 

Discovered within the constellation Dorado, this stellar nursery is a cosmic laboratory for studying detailed views of star formation, raw material, and ultimately early galaxy formation. There is no mythology associated with Dorado. It is one of 12 constellations named by the Dutch astronomer Petrus Plancius based on observations by Dutch navigators. The name means “the dolphinfish” in Latin. It first appeared on a celestial globe published by Plancius in 1597. It was later included in Johann Bayer’s star atlas in 1603. The constellation is usually represented as a dolphinfish such as the Mahi-mahi. It is not in any way related to the marine mammal known as the dolphin. This constellation has also been represented as a goldfish and a swordfish, but the dolphinfish is the correct representation based on the name Dorado.