Celestial 'Snow Angel' Dazzles in Hubble Telescope Photo
Get the world’s most fascinating discoveries delivered straight to your inbox.
You are now subscribed
Your newsletter sign-up was successful
Want to add more newsletters?
Delivered Daily
Daily Newsletter
Sign up for the latest discoveries, groundbreaking research and fascinating breakthroughs that impact you and the wider world direct to your inbox.
Once a week
Life's Little Mysteries
Feed your curiosity with an exclusive mystery every week, solved with science and delivered direct to your inbox before it's seen anywhere else.
Once a week
How It Works
Sign up to our free science & technology newsletter for your weekly fix of fascinating articles, quick quizzes, amazing images, and more
Delivered daily
Space.com Newsletter
Breaking space news, the latest updates on rocket launches, skywatching events and more!
Once a month
Watch This Space
Sign up to our monthly entertainment newsletter to keep up with all our coverage of the latest sci-fi and space movies, tv shows, games and books.
Once a week
Night Sky This Week
Discover this week's must-see night sky events, moon phases, and stunning astrophotos. Sign up for our skywatching newsletter and explore the universe with us!
Join the club
Get full access to premium articles, exclusive features and a growing list of member rewards.
Just in time for the holidays, the Hubble Space Telescope has snapped a spectacular view of a star-forming region in our Milky Way galaxy that looks like a snow angel in deep space.
This region, called Sharples 2-106 (or S106 for short) is located nearly 2,000 light-years away in the direction of the constellation of Cygnus (The Swan). The nebula is found in a relatively isolated part of the Milky Way, researchers said.
The S106 nebula measures several light-years across, and contains vast clouds of gas that resemble outstretched wings amidst an hourglass shape. The light from the glowing gas is colored blue in this image. A video and photo of the "snow angel" based on Hubble's observations reveals a spectacular view of the cosmic sight.
Hubble's view captures furious activity in the nebula, with ridges and ripples of super-hot gas mixing with the cooler interstellar medium. A massive young star, called Infrared Source 4 or IRS 4, is responsible for this turbulence, scientists said.
Radiation from IRS 4 makes the lobes of gas glow bright blue in the image, as they stretch outward from the central star. Luminous red veins also appear throughout the nebula creating intricate patterns.
A ring of dust and gas around the star squeezes the expanding nebula into its apparent hourglass shape. Faint light from the central star reflects off tiny dust particles, making the surrounding environment glow, and revealing darker filaments of dust beneath the blue dust clouds, the researchers said.
Astronomers have studied S106 and found several hundred brown dwarfs, which are cool, failed stars. When the nebula is viewed in infrared wavelengths, more than 600 of these misfit stars appear, scientists said.
Get the world’s most fascinating discoveries delivered straight to your inbox.
Brown dwarfs weigh less than a tenth of our sun, and because of this low mass, they are unable to trigger enough energy through nuclear fusion. These cosmic objects encompass the S106 nebula in a small cluster, the researchers said.
S106 was the 106th object to be catalogued by astronomer Stewart Sharpless in the 1950s, the researchers said.
The newly released image was taken by Hubble in February. The composite picture was created by stitching together two images taken in infrared light.
This story was provided by SPACE.com, a sister site to LiveScience. Follow SPACE.com for the latest in space science and exploration news on Twitter @Spacedotcom and on Facebook.

