Astronomers¹ find cosmic dust annoying when it blocks their view of the heavens, but without it the universe would be devoid² of（缺乏） stars. Cosmic dust is the indispensable（不可缺少的） ingredient for making stars and for understanding how primordial³（原始的，根本的） diffuse⁴（弥漫的，散开的） gas clouds assemble themselves into full-blown galaxies⁵. "Formation of galaxies is one of the biggest remaining questions in astrophysics（天体物理学） ," said Andrey Kravtsov, associate professor in astronomy & astrophysics at the University of Chicago.

Astrophysicists are moving closer to answering that question, thanks to a combination of new observations and supercomputer simulations, including those conducted by Kravtsov and Nick Gnedin, a physicist⁶ at Fermi National Accelerator Laboratory.

Gnedin and Kravtsov published new results based on their simulations in the May 1, 2010 issue of The Astrophysical Journal, explaining why stars formed more slowly in the early history of the universe than they did much later. The paper quickly came to the attention of Robert C. Kennicutt Jr., director of the University of Cambridge's Institute of Astronomy and co-discoverer of one of the key observational findings about star formation in galaxies, known as the Kennicutt-Schmidt relation.

In the June 3, 2010 issue of Nature, Kennicutt noted⁷ that the recent spate⁸ of observations and theoretical simulations bodes⁹ well（主吉） for the future of astrophysics. In their Astrophysical Journal paper, Kennicutt wrote, "Gnedin and Kravtsov take a significant step in unifying¹⁰ these observations and simulations, and provide a prime illustration of the recent progress in the subject as a whole."

Star-formation law

Kennicutt's star-formation law relates the amount of gas in galaxies in a given area to the rate at which it turns into stars over the same area. The relation has been quite useful when applied¹¹ to galaxies observed late in the history of the universe, but recent observations by Arthur Wolfe of the University of Californa, San Diego, and Hsiao-Wen Chen, assistant professor in astronomy and astrophysics at UChicago, indicate that the relation fails for galaxies observed during the first two billion years following the big bang.

Gnedin and Kravtsov's work successfully explains why. "What it shows is that at early stages of evolution, galaxies were much less efficient in converting their gas into stars," Kravtsov said.

Stellar evolution leads to increasing abundance of dust, as stars produce elements heavier than helium（氦） , including carbon, oxygen, and iron, which are key elements in dust particles. "Early on, galaxies didn't have enough time to produce a lot of dust, and without dust it's very difficult to form these stellar nurseries," Kravtsov said. "They don't convert the gas as efficiently¹² as galaxies today, which are already quite dusty."

The star-formation process begins when interstellar gas（星际气体） clouds become increasingly dense¹³. At some point the hydrogen and helium atoms start combining to form molecules¹⁵ in certain cold regions of these clouds. A hydrogen molecule¹⁴ forms when two hydrogen atoms join. They do so inefficiently¹⁶ in empty space, but find each other more readily on the surface of a cosmic dust particle.

"The biggest particles of cosmic dust are like the smallest particles of sand on good beaches in Hawaii," Gnedin said.

These hydrogen molecules are fragile and easily destroyed by the intense ultraviolet light emitted from massive young stars. But in some galactic（银河的，乳汁的） regions dark clouds, so-called because of the dust they contain, form a protective layer that protects the hydrogen molecules from the destructive light of other stars.