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STELLAR CHEMISTRY
Investigating Star Formation Is UMass Amherst Researcher's Mission
by Staff Writers
Amherst MA (SPX) Feb 28, 2017


Within galaxies, stars are born in cold clouds of gas tens to hundreds of light-years across, which collapse to form groups of stars that can have planets. Factors such as gas density, metal content, outflow feedback and radiation from young stars are believed to play a role in star formation.

University of Massachusetts Amherst astrophysicist Stella Offner, who has received a five-year, $429,000 faculty early career development (CAREER) grant from National Science Foundation (NSF), plans to use it not only to study how stars are born, but also to develop interactive online astronomy "tours" to enhance K-12 science education in local schools.

The CAREER grant is NSF's highest award to junior faculty who exemplify the role of teacher-scholars through outstanding research, excellent education and integrating education and research with their institution's mission.

Offner says she hopes to develop a better understanding of two fundamental questions in star formation, that is, how stars obtain their masses and how stars interact with their birth environments. Her team will perform computer simulations of forming star clusters and test different theories for the origin of star masses.

She says, "This is an important astrophysics problem because a star's mass determines how long it will live, whether it could host planets and how it will eventually die."

Offner will use the simulations to produce models to compare directly to telescope observations of star-forming regions in the Milky Way galaxy.

"From small stars all the way to huge ones that are a hundred times the mass of our Sun, the same physics is at work, but we do not know how it produces such a broad range of different masses," she notes.

"Many astronomers are trying to measure the distribution of stars in distant, old galaxies by looking at their total light, but we can't interpret that until we understand the distribution in the local universe," she adds.

Within galaxies, stars are born in cold clouds of gas tens to hundreds of light-years across, which collapse to form groups of stars that can have planets.

Factors such as gas density, metal content, outflow feedback and radiation from young stars are believed to play a role in star formation.

Offner will perform computer simulations to figure out how a few basic rules of physics interact with these and other variables to form stars of such different sizes and qualities. She works closely with astronomers who observe star-forming regions to design such simulations.

Using new data from this work, Offner plans to have her undergraduate astronomy students create tours about stars and planets using the public software WorldWide Telescope (WWT), which makes actual astronomy data available to any user around the globe.

"Astronomers rely on public support for our research," she says, "so we feel a strong obligation to share our exciting new discoveries with the public."

The WWT program is easy to use and allows astronomy data to be explored by everyone, the astrophysicist says. In addition to planet and star tours, she will create interactive online astronomy labs for girls in the Eureka! program held on the UMass Amherst campus each summer.

"I hope to find local teachers who are interested in using these labs in their classrooms as well," Offner says.

STELLAR CHEMISTRY
Dawn of a New Era for Supernova 1987A
Charlottesville VA (SPX) Feb 27, 2017
Three decades ago, astronomers spotted one of the brightest exploding stars in more than 400 years. The titanic supernova, called Supernova 1987A (SN 1987A), blazed with the power of 100 million suns for several months following its discovery on Feb. 23, 1987. Since that first sighting, SN 1987A has continued to fascinate astronomers with its spectacular light show. Located in the nearby L ... read more

Related Links
WorldWide Telescope
Stellar Chemistry, The Universe And All Within It

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