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NASA selects Gamma-ray Telescope to Chart Milky Way evolution
by Staff Writers
Greenbelt MD (SPX) Oct 19, 2021

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NASA has selected a new space telescope proposal that will study the recent history of star birth, star death, and the formation of chemical elements in the Milky Way. The gamma-ray telescope, called the Compton Spectrometer and Imager (COSI), is expected to launch in 2025 as NASA's latest small astrophysics mission.

NASA's Astrophysics Explorers Program received 18 telescope proposals in 2019 and selected four for mission concept studies. After detailed review of these studies by a panel of scientists and engineers, NASA selected COSI to continue into development.

"For more than 60 years, NASA has provided opportunities for inventive, smaller-scale missions to fill knowledge gaps where we still seek answers," said Thomas Zurbuchen, associate administrator for the agency's Science Mission Directorate in Washington. "COSI will answer questions about the origin of the chemical elements in our own Milky Way galaxy, the very ingredients critical to the formation of Earth itself."

COSI will study gamma rays from radioactive atoms produced when massive stars exploded to map where chemical elements were formed in the Milky Way. The mission will also probe the mysterious origin of our galaxy's positrons, also known as antielectrons - subatomic particles that have the same mass as an electron but a positive charge.

COSI's principal investigator is John Tomsick at the University of California, Berkeley. The mission will cost approximately $145 million, not including launch costs. NASA will select a launch provider later.

The COSI team spent decades developing their technology through flights on scientific balloons. In 2016, they sent a version of the gamma-ray instrument aboard NASA's super pressure balloon, which is designed for long flights and heavy lifts.


Related Links
Explorers Program
Stellar Chemistry, The Universe And All Within It


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STELLAR CHEMISTRY
Researchers reveal a wobbly and flared Milky Way disk based on LAMOST-Gaia data
Beijing, China (SPX) Oct 04, 2021
Astronomers, from National Astronomical Observatories of Chinese Academy of Sciences (NAOC), Shanghai Astronomical Observatory of CAS and Nanjing University, revealed a wobbly and flared Milky Way disk based on LAMOST-Gaia data, which updates our understanding about the disk. The Milky Way is a typical disk galaxy. In the classical view of the Milky Way, the disk is symmetric and flat on the whole, like a pancake. Stars in the disk rotate around the Galactic center, with mean radial and vertical v ... read more

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