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Andromeda Star Birth Is Slowing Down

A study using NASA's Hubble Space Telescope shows star formation in the nearby Andromeda galaxy has declined for 500 million years, with a steep drop in the last 40 million years.

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A Detailed View of Our Neighbor

Located 2.5 million light-years away, Andromeda is a spiral galaxy comparable to the Milky Way. Its proximity allows astronomers to examine individual stars to understand past stellar growth.

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Surveying Two-Thirds of the Disk

Researchers combined two Panchromatic Hubble Andromeda Treasury surveys. By measuring about 200 million individual stars across the disk, the team built a comprehensive timeline of Andromeda's past activity.

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Tracking Blue and Red Populations

Younger, massive stars appear bluer, whereas older, lower-mass stars look redder. Scientists divided images into 300-light-year squares to map variations in star-forming activity over time.

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Measuring the Rate of Decay

Star formation dropped from one solar mass per year 500 million years ago to half that 40 million years ago. Today, the rate is just one-fifth of a solar mass annually.

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Activity Ring Drives the Drop

Recent star formation is concentrated in a ring 32,000 light-years from the core. Decreasing activity inside this structural ring accounts for much of Andromeda's overall slowdown.

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Investigating Neighboring M32

Scientists checked if nearby satellite galaxy M32 triggered the reduction. A slowdown near M32 starting 60 million years ago suggests a potential past encounter between the two galaxies.

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Future Observations with Roman

Future wide-field views from NASA’s upcoming Nancy Grace Roman Space Telescope will cover 100 times more area than Hubble, mapping Andromeda’s entire disk and outer halo.

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