Young Stars May Feast Frantically, Grow Chaotically, New Study Shows

Materials Falling onto a Baby Star
Computer simulations show the possible motion of materials falling onto a baby star (left). The infalling matter could be producing bright bursts of light. The middle and right images show what the light patterns would look like, seen from two different angles. (Image credit: Science Advances, H. B. Liu.)

Infant stars may release bursts of light when they collide with and devour dense clumps of matter that otherwise might have gone on to form planets, new research suggests.

The new finding has larger implications for understanding how stars grow and evolve early in their lives — specifically, that stars may grow through chaotic series of violent events, instead of steadily getting larger, as previously thought, the authors of the new work noted.

The new images of the flaring newborn stars "were surprising and fascinating, and nothing like anything previously observed around young stars," representativesofthe National Institutes of Natural Sciences (NINS) in Japan said in a statement. (NINS is one of the managing institutions of the National Astronomical Observatory of Japan, where some of the paper's authors are based.)

The researchers discovered "tails" projecting from the protoplanetary material around the young stars, as well as spikes of gas and dust.

"We suggest a previously unrecognized evolutionary stage in the formation of stars and protoplanetary disks," study lead author Hauyu Baobab Liu, an astronomer at the Academia Sinica Institute of Astronomy and Astrophysics in Taipei, Taiwan, told Space.com.

Observations of baby stars and the gas and dust that surround them. These observations may reveal that clumps of gas and dust fall into the stars (helping them grow) in a more chaotic fashion than once thought. (Image credit: Science Advances, H. B. Liu)

This unstable phase of a protostar's life might last several hundred thousand years, the scientists added.

"Although more simulations are required to match the simulations to the observed images, these images show that this is a promising explanation for the nature of FU Ori[onis]outbursts," NINS representatives said in the statement.

The scientists detailed their findings online Feb. 5 in the journal Science Advances.

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Charles Q. Choi
Contributing Writer

Charles Q. Choi is a contributing writer for Space.com and Live Science. He covers all things human origins and astronomy as well as physics, animals and general science topics. Charles has a Master of Arts degree from the University of Missouri-Columbia, School of Journalism and a Bachelor of Arts degree from the University of South Florida. Charles has visited every continent on Earth, drinking rancid yak butter tea in Lhasa, snorkeling with sea lions in the Galapagos and even climbing an iceberg in Antarctica. Visit him at http://www.sciwriter.us