Newly Forming Stars Don’t Blast Away Material as Previously Believed. So Why Do They Stop Growing?

We thought we understood how stars are formed. It turns out, we don’t. Not completely, anyway. A new study, recently conducted using data from the Hubble Space Telescope, is sending astronomers back to the drawing board to rewrite the accepted model of stellar formation.

What we do know about star formation is that they are born from enormous clouds of hydrogen gas. The gas gets clumped together and compressed by gravity, increasing in pressure and temperature until the mass grows large enough to set off nuclear fusion. But stars don’t seem to absorb all of the gas in their surroundings. Something stops them from reaching enormous sizes.

Until now, the accepted model assumed that the excess gas gets blown away from the star in extremely powerful solar winds, shaped and directed by magnetic fields shooting out from the poles of the star. “There are remarkable ‘U’- or ‘V’- shaped structures extending to the north and south of a protostar,” explains Nolan Habel, one of the researchers from the University of Toledo. “They are actually hollowed-out cavities carved into the surrounding gas by hurricane-like winds or jets of material expelled from the poles of the protostar.”

Protostars being born in the Orion Nebula, as seen by the Hubble Space Telescope. Image Credit: NASA, ESA, STScI, N. Habel and S. T. Megeath (University of Toledo).

These powerful jets were thought to eventually clear out all the excess gas, leaving stars to only absorb about 30% of the material in their surroundings. But the new study turns this theory on its head. The cavities created by the jets do not seem to grow steadily over time, meaning that they alone cannot possibly explain why stars stop growing. There must be some other mechanism that helps clear out the remaining gas surrounding a protostar.

The team made this discovery by studying a sample of 304 protostars at various stages of formation in the Orion Nebula (the closest region of star formation to Earth). The astronomers sorted the stars by age, and then used Hubble imagery to measure the shape and volume of the cavities created by jets. They were expecting to see the cavities grow over time, as the model suggests should happen. But, they didn’t.

“We find that at the end of the protostellar phase, where most of the gas has fallen from the surrounding cloud onto the star, a number of young stars still have fairly narrow cavities,” said Tom Megeath, another researcher on the team. This goes against all common theories of star formation, and is going to require further research to figure out what is happening. Why do stars stop growing, if not because of their polar jets?

A wide view of the Orion Nebula, taken by the Hubble Space Telescope. Image Credit: NASA, ESA, M. Robberto (Space Telescope Science Institute/ESA) and the Hubble Space Telescope Orion Treasury Project Team.

The team has brainstormed a few possible alternatives. The gas clouds in which stars form are not uniformly dense. They have ‘filaments’ of higher density where protostars tend to form, and oscillations in these filaments might fling the protostars away. We also know that stars don’t always form alone: about half of all sun-like stars have a binary partner. It is conceivable that two or more protostars forming close to one another might gravitationally disturb each other, pushing them away from their source material.

For now, these are just theories. It will probably take bigger and better instruments to find a concrete answer. The James Webb Space Telescope, set to launch later this year, might provide astronomers with the clues they need to solve the mystery. In the meantime, there’s a whole lot of astrophysics textbooks out there that are going to need a revised edition.

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Scott Alan Johnston

Scott Alan Johnston is a science writer/editor at the Perimeter Institute for Theoretical Physics, a contributor at Universe Today, and a historian of science. He is the author of "The Clocks are Telling Lies," which tells the story of the early days of global timekeeping, when 19th-century astronomers and engineers struggled to organize time in a newly interconnected world. You can follow Scott on Twitter @ScottyJ_PhD

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