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The green and red splotch in this image is the most active star-making
galaxy in the very distant universe. Nicknamed "Baby Boom," the galaxy is
churning out an average of up to 4,000 stars per year, more than 100 times
the number produced in our own Milky Way galaxy. It was spotted 12.3
billion light-years away by a suite of telescopes, including NASA's
Spitzer Space Telescope.
Baby Boom is a type of galaxy called a starburst. Like some other
starbursts, it is thought to be a collection of colliding galaxies. As the
galaxies smash together, gas becomes compressed, triggering the birth of
stars. In this multi-wavelength portrait, the color red shows where loads
of new stars are forming in Baby Boom, and where warm dust heated by the
stars is giving off infrared light.
Green (visible-light wavelengths) denotes gas in the Baby Boom galaxy,
while blue (also visible light) shows galaxies in the foreground that are
not producing nearly as many stars. Yellow/orange (near-infrared light)
indicates starlight from the outer portion of Baby Boom. The red blob to
the left is another foreground galaxy that is not producing a lot of
stars.
This composite contains data from NASA's Hubble Space Telescope,
Spitzer and Japan's Subaru Telescope
in Hawaii.