NASA's Webb Peers Deeper into Mysterious Flame Nebula

Summary
New population census answers the question: How small can you go when forming stars and brown dwarfs?
The Flame Nebula, a star-forming region in the Orion Molecular Cloud Complex, has a long history of observation from telescopes such as NASA’s Hubble Space Telescope. However, the smallest stars within its dark and dusty heart have largely been hidden from view. The infrared vision from NASA’s James Webb Space Telescope has taken a first-time look, counting the smallest and faintest objects to determine the lowest mass required to form brown dwarfs.
Full Article
The Flame Nebula, located about 1,400 light-years away from Earth, is a hotbed of star formation less than 1 million years old. Within the Flame Nebula, there are objects so small that their cores will never be able to fuse hydrogen like full-fledged stars — brown dwarfs. Brown dwarfs, often called “failed stars,” over time become very dim and much cooler than stars. These factors make observing brown dwarfs with most telescopes difficult, if not impossible, even at cosmically short distances from the Sun. When they are very young, however, they are still relatively warmer ...Visit NASA Science to view the full news release including article text and associated Webb imagery, graphics, scientific visualizations, videos, captions, text descriptions, and other information.
News releases highlighting the discoveries of NASA’s James Webb Space Telescope are produced for NASA by the Space Telescope Science Institute (STScI) in Baltimore, Maryland, under NASA Contract NAS5-03127. News release content is developed by the News Team in STScI’s Office of Public Outreach.
News Center Prefooter
Inbox Astronomy
Sign up to receive the latest news, images, and discoveries about the universe:
Contact our News Team
Ask the News Team
Contact our Outreach Office
Ask the Outreach Office
