How the First Stars Were Born

How the First Stars Were Born
Projected gas distribution around the protostar. The large-scale gas distribution around the cosmological halo. (Image credit: Yoshida et al/Astrophysical Journal)

Anew supercomputer simulation offers the most detailed view yet of how the firststars evolved after the Big Bang.

Themodel follows the simpler physics that ruled the early universe to see how coldclumps of gas eventually grew into giant star embryos.

"Untilyou put that physics in the code, you can't evaluate how the first protostarsformed," said Lars Hernquist, an astrophysicist at Harvard University whose early-stars model is detailed in this week's issue of the journal Science.His remarks were made Wednesday during a press teleconference.

Mysterious "darkmatter" provided the first gravitational impetus for hydrogen andhelium gas to start clumping together, Hernquist said. The gas began releasingenergy as it condensed, forming molecules from atoms, which further cooled theclump and allowed for even greater condensing.

Unlikeprevious models, the latest simulation takes this cooling process of "complexradiative transfer" into account, said Nagoya University astrophysicist NaokiYoshida, who headed up the modeling project.

"Nosimulation has ever gotten to the point of identifying this important stage inthe birthof a star," Hernquist noted.

Contributing Writer

Jeremy Hsu is science writer based in New York City whose work has appeared in Scientific American, Discovery Magazine, Backchannel, Wired.com and IEEE Spectrum, among others. He joined the Space.com and Live Science teams in 2010 as a Senior Writer and is currently the Editor-in-Chief of Indicate Media.  Jeremy studied history and sociology of science at the University of Pennsylvania, and earned a master's degree in journalism from the NYU Science, Health and Environmental Reporting Program. You can find Jeremy's latest project on Twitter