Scientists have released a vibrant new composite image of the Tarantula Nebula, also known as 30 Doradus. NASA described the colorful observation as resembling “a collage made of layered sheets of colored cellophane,” offering new details about the extensive star formation region.
The Tarantula Nebula is located in the Large Magellanic Cloud, a galaxy situated approximately 160,000 light-years from Earth. Within this nebula, thousands of young stars are embedded in a complex, honeycomb-like structure of gas and dust.
This latest image integrates data from several NASA observatories. X-rays from the Chandra X-ray Observatory, which has observed the Tarantula Nebula multiple times, are included. Infrared data from the James Webb Space Telescope highlights thousands of young stars and vast clouds of cool dust, which are the raw materials for future star and planet formation.
The composite image incorporates full views from the Hubble and Webb telescopes, along with a significant portion of the Chandra data. These findings were recently published in a research paper in The Astrophysical Journal. Data from NASA’s retired Spitzer Space Telescope was also utilized in the study.
Researchers analyzing the combined data have concluded that the Tarantula Nebula may be losing energy through several processes. Observations indicate that up to half of its hot gas is escaping, turbulent mixing is cooling the remaining gas, and thermal conduction is transferring heat to cooler shell material without further mixing.
