Thursday, October 5, 2023

4178 - EARLIEST GALAXIES - why are they so bright?

 

-    4178  -   EARLIEST  GALAXIES  -  why are they so bright?     When scientists viewed the James Webb Space Telescope’s (JWST) first images of the universe’s earliest galaxies, they were shocked. The young galaxies appeared too bright, too massive and too mature to have formed so soon after the Big Bang. It would be like an infant growing into an adult within just a couple years.


---------------  4178   -   EARLIEST  GALAXIES  -  why are they so bright?

-    The startling discovery even caused some physicists to question the standard model of cosmology, wondering whether or not it should be upended.  Using new simulations, a Northwestern University-led team of astrophysicists now has discovered that these galaxies likely are not so massive after all. Although a galaxy’s brightness is typically determined by its mass, the new findings suggest that less massive galaxies can glow just as brightly from irregular, brilliant bursts of star formation.

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-    Not only does this finding explain why young galaxies appear deceptively massive, it also fits within the standard model of cosmology.  The discovery of these galaxies was a big surprise because they were substantially brighter than anticipated.

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-   Typically, a galaxy is bright because it’s big. But because these galaxies formed at cosmic dawn, not enough time has passed since the Big Bang. How could these massive galaxies assemble so quickly?   Simulations show that galaxies have no problem forming this brightness by cosmic dawn.

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-    A period that lasted from roughly 100 million years to 1 billion years after the Big Bang, cosmic dawn is marked by the formation of the universe’s first stars and galaxies. Before the JWST launched into space, astronomers knew very little about this ancient time period.

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-   Prior to JWST, most of our knowledge about the early universe was speculation based on data from very few sources. With the huge increase in observing power, we can see physical details about the galaxies and use that solid observational evidence to study the physics to understand what’s happening.

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-    Advanced computer  simulations produced cosmic dawn galaxies that were just as bright as those observed by the JWST. The simulations are part of the Feedback of Relativistic Environments(FIRE) project.   The new study includes collaborators from the Flatiron Institute’s Center for Computational Astrophysics, Massachusetts Institute of Technology and University of California, Davis.

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-    The FIRE simulations combine astrophysical theory and advanced algorithms to model galaxy formation. The models enable researchers to probe how galaxies form, grow and change shape, while accounting for energy, mass, momentum and chemical elements returned from stars.

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-    In massive galaxies like the Milky Way, stars form at a steady rate, with the numbers of stars gradually increasing over time. But so-called bursty star formation occurs when stars form in an alternating pattern, many stars at once, followed by millions of years of very few new stars and then many stars again.

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-   “Bursty star formation” is especially common in low-mass galaxies.  The details of why this happens are still the subject of ongoing research.  A burst of stars form, then a few million years later, those stars explode as supernovae. The gas gets kicked out and then falls back in to form new stars, driving the cycle of star formation. But when galaxies get massive enough, they have much stronger gravity. When supernovae explode, they are not strong enough to eject gas from the system. The gravity holds the galaxy together and brings it into a steady state.

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-    Most of the light in a galaxy comes from the most massive stars.  Because more massive stars burn at a higher speed, they are shorter lived. They rapidly use up their fuel in nuclear reactions. So, the brightness of a galaxy is more directly related to how many stars it has formed in the last few million years than the mass of the galaxy as a whole.

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October 5,  2023       EARLIEST  GALAXIES  -  why are they so bright?      4178

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