Stellar nursery sparkles at the edge of our galaxy in gorgeous Hubble Telescope image

A very sparkly region of space with hazy structures ballooning from the right toward the left of the screen. Some areas have a pink glow.
A section of active star formation within the emission nebula Sh2-284, located 15,000 light-years from Earth. (Image credit: NASA, ESA, and M. Andersen (European Southern Observatory - Germany); Processing: Gladys Kober (NASA/Catholic University of America))

A sparkling stellar nursery appears reminiscent of the early universe in new images from the Hubble Space Telescope.

The emission nebula, known as Sh2-284, is an immense region of gas and dust that fuels new star formation. Located 15,000 light-years from Earth, at the end of an outer spiral arm of our Milky Way galaxy, Sh2-284 lacks elements heavier than hydrogen and helium, much like the environment of the early universe, according to a statement from NASA.

"These conditions mimic the early universe, when matter was mostly helium and hydrogen and heavier elements were just beginning to form via nuclear fusion within massive stars," NASA officials said in the statement. This is what is known as a "low-metallicity" region.

The Hubble Space Telescope image offers an up-close view of one section of the nebula, which is largely shaped by a young central star cluster called Dolidze 25, located outside of the image frame. The cluster is home to young stars ranging in age from 1.5 million to 13 million years old (for reference, our sun is 4.6 billion years old).

Emission nebulas are areas of active star formation, where ultraviolet radiation from nearby young, hot stars ionizes the surrounding gas (primarily hydrogen), which then, in turn, emits a bright light. The ionizing winds and radiation from the star cluster pushes gas and dust around in the nebula, creating the intricate features and cloud-like carvings observed in the Hubble image.

The new infrared view from Hubble captures the nebula's dazzling starlight that might otherwise be obscured by dense dust and gas clouds if observed at a visible wavelength. The newborn stars glow bright pink in infrared light and appear exceptionally vibrant against the dark clouds of gas and dust.

The recent observations of Sh2-284, which NASA released online on March 8, can be used to study how low metallicity influences stellar formation, and how that can be applied to our understanding of the early universe.

Join our Space Forums to keep talking space on the latest missions, night sky and more! And if you have a news tip, correction or comment, let us know at: community@space.com.

Samantha Mathewson
Contributing Writer

Samantha Mathewson joined Space.com as an intern in the summer of 2016. She received a B.A. in Journalism and Environmental Science at the University of New Haven, in Connecticut. Previously, her work has been published in Nature World News. When not writing or reading about science, Samantha enjoys traveling to new places and taking photos! You can follow her on Twitter @Sam_Ashley13. 

You must confirm your public display name before commenting

Please logout and then login again, you will then be prompted to enter your display name.