(PhysOrg.com) -- Five billion years from now, our Milky Way Galaxy will collide with the Andromeda Galaxy. This will mark a moment of both destruction and creation. The galaxies will lose their separate identities as they merge into one. At the same time, cosmic clouds of gas and dust will smash together, triggering the birth of new stars.
To understand our past and imagine our future, we must understand what happens when galaxies collide. But since galaxy collisions take place over millions to billions of years, we cant watch a single collision from start to finish. Instead, we must study a variety of colliding galaxies at different stages. By combining recent data from two space
telescopes, astronomers are gaining fresh insights into the collision process.
Weve assembled an atlas of galactic train wrecks from start to finish. This atlas is the first step in reading the story of how galaxies form, grow, and evolve, said lead author Lauranne Lanz of the Harvard-Smithsonian Center for Astrophysics (CfA).
Lanz presented her findings today in a press conference at the 218th meeting of the American Astronomical Society.
The new images combine observations from NASAs Spitzer Space Telescope, which observes infrared light, and Galaxy Evolution Explorer (GALEX) spacecraft, which observes ultraviolet light. By analyzing information from different parts of the light spectrum, scientists can learn much more than from a single wavelength alone, because they observe different components of a galaxy.
GALEXs ultraviolet data captures the emission from hot young stars. Spitzer sees the infrared emission from warm dust heated by those stars, as well as from stellar surfaces. Therefore, GALEXs ultraviolet data and Spitzers infrared data highlight areas where stars are forming most rapidly, and together permit a more complete census of the new stars.
In general, galaxy collisions spark star formation. However, some interacting galaxies show fewer new stars than others. Lanz and her colleagues want to figure out what differences in physical processes cause these different outcomes. Their findings will also help guide computer simulations of galaxy collisions.
Were working with the theorists to give our understanding a reality check, said Lanz. Our understanding will really be tested in five billion years, when the Milky Way experiences its own collision.
Lanzs co-authors are Nicola Brassington (Univ. of Hertfordshire, UK); Andreas Zezas (Univ. of Crete, Greece); Howard Smith and Matt Ashby (CfA); Christopher Klein (UC Berkeley); and Patrik Jonsson, Lars Hernquist, and Giovanni Fazio (CfA).
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