Saturday, January 6, 2024

4306 - THE FIRST STARS?

 

    4306  - THE  FIRST  STARS?   -   The James Webb Space Telescope (JWST) has glimpsed light from ionized helium in a distant galaxy, which could indicate the presence of the universe’s very first generation of stars.


------------------------------  4306 -  THE  FIRST  STARS?

-    These long-sought,  “Population III” stars, would have been huge balls of hydrogen and helium sculpted from the universe’s primordial gas. Theorists started imagining these first fireballs in the 1970s, hypothesizing that, after short lifetimes, they exploded as supernovas, forging heavier elements and spewing them into the universe.

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-     That star stuff later gave rise to Population II stars more abundant in heavy elements, then even richer Population I stars like our sun, as well as planets, asteroids, comets and eventually life itself.

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-    JWST is transforming vast swaths of astronomy being capable of peering far enough away in space and time to see them. Already, the gigantic floating telescope has detected distant galaxies whose unusual brightness suggests they may contain Population III stars.

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-    About 400,000 years after the Big Bang, electrons, protons and neutrons settled down enough to combine into hydrogen and helium atoms. As the temperature kept dropping, dark matter gradually clumped up, pulling the atoms with it. Inside the clumps, hydrogen and helium were squashed by gravity, condensing into enormous balls of gas until, once the balls were dense enough, nuclear fusion suddenly ignited in their centers. The first stars were born.

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-    The German astronomer Walter Baade categorized the stars in our galaxy into types I and II in 1944. The former includes our sun and other metal-rich stars; the latter contains older stars made of lighter elements.

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-    The idea of Population III stars entered the literature decades later. In a 1984 paper the British astrophysicist Bernard Carr described the vital role this original breed of star may have played in the early universe. Their heat or explosions could have reionized the universe and their heavy-element yield could have produced a burst of pregalactic enrichment, giving rise to later stars richer in heavier elements.

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-    The stars could have grown to immense sizes, measuring anywhere between a few hundred and 100,000 times more massive than our sun, because of the large volume of hydrogen and helium gas available in the early universe.

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-    Those at the heavier end of the range, supermassive stars, would have been relatively cool, red and bloated, with sizes that could encompass almost our entire solar system. Denser, more modestly sized variants of Population III stars would have shone blue hot, with surface temperatures of some 50,000 degrees Celsius, compared to just 5,500 degrees for our sun.

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-     In the present universe, clouds of gas fragment into lots of small stars. But the simulations showed that gas clouds in the early universe, being much hotter than modern clouds, couldn’t as easily condense and were therefore less efficient at star formation. Instead, entire clouds would collapse into a single, giant star.

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-   Their immense proportions meant the stars were short-lived, lasting a few million years at most. (More massive stars burn through their available fuel more quickly.)   Population III stars wouldn’t have lasted long in the history of the universe, perhaps a few hundred million years as the last pockets of primordial gas dissipated.

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-     In 1999, astronomers at the University of Colorado predicted that the stars should produce a telltale signature: specific frequencies of light emitted by helium II, or helium atoms that are missing an electron, when each atom’s remaining electron moves between energy levels.  The helium emission is not actually originating from within the stars themselves, rather, it was created when energetic photons from the stars’ hot surfaces plowed into gas surrounding the star.

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-    In 2015 astronomers detected a possible hint of a helium II signature in a distant, primitive galaxy that might have been linked to a group of Population III stars. Seen as it appeared 800 million years after the Big Bang, the galaxy looked as if it might contain the first evidence of the first stars in the universe.

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-     JWST,  launched in December 2021, with its enormous mirror and unprecedented sensitivity to infrared light, can peer more easily into the early universe than any telescope before it. (Because light takes time to travel here, the telescope sees faint, faraway objects as they appeared long ago.) The telescope can also do spectroscopy, breaking up light into its component wavelengths, which allows it to look for the helium II hallmark of Population III stars.

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-    Analyzed spectroscopy data for more than 2,000 of  JWST’s targets in a distant galaxy seen as it appeared just 620 million years after the Big Bang.   The galaxy is split into two pieces.   Analysis showed that one half seems to have the key signature of helium II mixed with light from other elements, potentially pointing to a hybrid population of thousands of Population III and other stars. Spectroscopy of the second half of the galaxy has yet to be done, but its brightness hints at a more Population III-rich environment.

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-    The Webb Space telescope will rewrite cosmic history if It works.   Astronomers propose to use the gravity of giant clusters of galaxies to see individual stars in the early universe. Using a massive object like a cluster to warp light and magnify more distant objects (a technique known as gravitational lensing) is a common way astronomers obtain views of distant galaxies.

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-      And there remains the tantalizing possibility that some of the unexpectedly bright galaxies already seen by JWST in the early universe could owe their brightness to massive Population III stars.

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-     Webb Space Telescope's discovery of the universe's oldest black holes is also giving astronomers some vital clues for how they came to be.   JWST has spotted the oldest black hole ever seen, an ancient monster with the mass of 1.6 million suns lurking 13 billion years in the universe's past.   Looking back in time to our universe's beginnings, the supermassive black hole at the center of the infant galaxy GN-z11 was spotted just 440 million years after the universe began.

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-     Closer to the present-day,  black holes are born from the collapse of giant stars. They grow by ceaselessly gorging on gas, dust, stars and other black holes. As they feast, friction causes the material spiraling into the black holes' to heat up, and they emit light that can be detected by telescopes, turning them into “active galactic nuclei” (AGN).

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-    The most extreme AGN are quasars, supermassive black holes that are billions of times heavier than the sun and shed their gaseous cocoons with light blasts trillions of times more luminous than the brightest stars.

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-     Because light travels at a fixed speed through the vacuum of space, the deeper that scientists look into the universe, the more remote light they intercept and the further back in time they see. To spot the black hole the astronomers scanned the sky with two infrared cameras the JWST's Mid-Infrared Instrument (MIRI) and Near Infrared Camera and used the cameras' built-in spectrographs to break down the light into its component frequencies.

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-    By deconstructing these faint glimmers from the universe's earliest years, they found an unexpected spike among the frequencies contained within the light, a key sign that the hot material around a black hole was beaming out faint traces of light across the universe.

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-   The  Webb Space Telescope also spotted six gigantic galaxies, each roughly the size of our own Milky Way, that formed at a bafflingly fast pace, taking shape just 500 million years after the Big Bang.

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-  This group of galaxies from the dawn of the universe  are so massive they shouldn't exist.  The six gargantuan galaxies, which contain almost as many stars as the Milky Way despite forming only 500 to 700 million years after the Big Bang, have been dubbed "universe breakers".   If they're real, the discovery calls our entire understanding of galaxy formation into question.

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-     Scientists don't know exactly when the first clumps of stars began to merge into the beginnings of the galaxies we see today, but cosmologists previously estimated that the process began slowly taking shape within the first few hundred million years after the Big Bang. Currently accepted theories suggest that 1 to 2 billion years into the universe's life, these early protogalaxies reached adolescence forming into dwarf galaxies that began devouring each other to grow into ones like our own.

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-   Because light travels at a fixed speed through the vacuum of space, the deeper we look into the universe, the more remote light we intercept and the further back in time we see.   JWST  is peering roughly 13.5 billion years into the past, the astronomers found that enormous galaxies had already burst into life very quickly after the Big Bang, when the universe was just 3% of its current age.

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-   The galaxies are so massive, they are in tension with 99 percent of the models for cosmology.  This means that either the models need to be altered, or scientific understanding of galaxy formation requires a fundamental rethink.

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-    Right now, all evidence points to these celestial objects being galaxies, but the astronomers haven't ruled out that some of them could be enormous quasars or supermassive black holes.

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-   Previous imaging of the early universe by the Hubble Space Telescope didn't detect the giant galaxies, but JWST is about 100 times more powerful than Hubble.

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-  The $10 billion JWST launched to a gravitationally stable location beyond the moon's orbit, a Lagrange point, in December 2021. The space observatory was designed to read the earliest chapters of the universe's history in its faintest glimmers of light, which have been stretched to infrared frequencies from billions of years of travel across the expanding fabric of space-time.

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-    The next step will be to take a spectrum image of the giant galaxies, providing them with accurate distances and a better idea of the chemical makeup of  the beginning of the universe.

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January 5, 2023                  THE  FIRST  STARS?                        4306

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