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The Outskirts of Ancient Galaxies Change Our View of the Universe ✛✦
Original: "Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions"
The Webb telescope revealed that in distant galaxies, the centers are older than the outskirts, meaning their mass is less than previously thought.
For a long time, astronomers looked at distant galaxies as an unfamiliar city, assessing its age only by the central square with ancient cathedrals. The bright core seemed ancient, and the whole galaxy appeared disproportionately massive for the young Universe. But the new James Webbtelescope allowed us to see the outskirts: there the stars are younger and bluer. The age difference between the center and the edge reaches a billion years — as if the heart of the city was built in antiquity, and the suburbs were built yesterday. Previously, with spectroscopy (splitting light), the instrument mainly captured the center, and the mass was overestimated. Analyzing the entire area using photometry (brightness measurement) lowered the estimates, and the galaxies no longer contradicted the Big Bang theory and dark matter — an invisible substance holding stars, which was pointed out by Vera Rubin.
The most astonishing of the galaxies appeared when the Universe was 300 million years old — like seeing a gray-bearded baby.
One of the galaxies formed when the universe was 300 million years old — like a newborn with a gray beard.
\frac{\Delta (U-V)}{\Delta R}
The gradient of the U−V color index as we move from the galaxy center to the edge, measured in magnitudes per kiloparsec. A negative value means the core is redder and likely older than the outskirts.