Sunday, June 30, 2024

4516 - EARTH'S MAGNETIC FIELD?

 

-    4516  -  EARTH'S  MAGNETIC  FIELD?  -   When I got my first boy scout compass I became aware that Earth's magnetic field pointed towards the North Pole.  However, today the needle is changing.  The Earth's changing, irregular magnetic field is causing headaches for polar navigation.


------------------------------------  4516  -  EARTH'S  MAGNETIC  FIELD?

-    Changes in the Earth's global magnetic field over six months in 2014 as measured by the European Space Agency's three-satellite Swarm constellation.   The Earth's liquid molten outer core, composed mostly of iron and nickel, exerts an electromagnetic field extending from the north and south pole that protects the planet from harmful solar particle radiation.

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-   Fluctuations in the strength of Earth's magnetic field is caused by daily changes in solar wind structure and intermittent solar storms.  This can impact the use of geomagnetic field models which are essential for navigation in satellites, planes, ships, cars, and my boy scout compass..

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-    Magnetic field models differ based on the location of data collection, either on or near the Earth's surface or low Earth orbiting satellites. Past research has attributed model differences to space weather activity levels, but a recent analysis of six years of Earth and satellite magnetic field models found model discrepancies are also driven by modeling errors rather than geophysical phenomena alone.

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-    The research team assessed differences between observations from the Swarm mission's low-Earth orbit satellites and a Earth magnetic field model, the thirteenth generation of the International Geomagnetic Reference Field or “IGRF-13”. They focused on differences during low to moderate geomagnetic conditions which encompasses 98.1% of the time between the years 2014 and 2020.

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-   Satellite observations collected at different locations above Earth are sensitive to magnetic field fluctuations, whereas Earth magnetic field models use observations to estimate the Earth's internal magnetic field without accounting for the influence of solar storms. Internal magnetic field models like IGRF-13 are used to track changes in the Earth's magnetic poles, like the North pole's shift of about 45 kilometers north-northwest each year.

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-    Understanding these large differences are important for satellite operation when using IGRF-13 as a reference and for research on the physics of the Earth's magnetosphere, ionosphere and thermosphere.

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-    Model uncertainty was highest in the north and south polar regions, and a statistical analysis revealed that the asymmetry between the north and south polar regions was a major factor driving model differences.

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-   We often assume a nearly symmetrical magnetic field between the northern and southern polar regions, but they are actually very different.  The two geographic poles map to different geomagnetic coordinates. The North pole maps to around 84° Magnetic Latitude (MLAT) and 169° Magnetic Longitude (MLON) and the South pole maps to around −74° MLAT and 19° MLON.

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-    The Swarm satellites' polar orbit track creates a sampling bias with a high concentration of measurements around the geographic poles, which exacerbates the model differences.  Understanding that what has been attributed to geophysical disturbances is really due to the asymmetry of the Earth's magnetic field will help us better create geomagnetic field models as well as help with satellite and aviation navigation.

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-    Another issue that is causing the navigation community concern, is that the polar magnetic field has been changing rapidly over the past decade or so.  This adds further complexity to creating accurate magnetic field models and my boy scout compass.

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June 30, 2024         EARTH'S  MAGNETIC  FIELD?                   4516

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4516 - THE OLDEST STARS - are circling our galaxy?

 

-    4516  -   THE  OLDEST  STARS  -  are circling our galaxy?  -    The oldest stars in the universe found hiding near the Milky Way's edge,    Astronomers reanalyzed the chemical composition of three stars in the Milky Way's halo and found that they are between 12 and 13 billion years old. They may have also been stolen from other galaxies.


-----------------------------  4516  -  THE  OLDEST  STARS  -  are circling our galaxy?

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-    Three alien stars circling the Milky Way could be some of the oldest ever found in the universe. The ancient celestial objects may have been among the first to form after the Big Bang and were likely stolen by our galaxy during gravitational tugs-of-war billions of years ago.

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-    Researchers reanalyzed three previously observed stars each located around 30,000 light-years from Earth in the Milky Way's halo, a massive cloud of stars that orbit beyond our galaxy's main galactic disk. The basic chemical composition of these stars suggests they are all between 12 and 13 billion years old, making them almost as old as the universe itself, which formed around 13.8 billion years ago.

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-   The trio's respective trajectories through the Milky Way also hint that these stars did not originate in our galaxy but were instead stolen from the periphery of some of the universe's oldest galaxies as the Milky Way brushed past them billions of years ago.

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-     The ancient balls of gas, which researchers have dubbed “Small Accreted Stellar System” (SASS) stars, are part of our cosmic family tree.

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-   Normally, stars this old can only be studied by spying on galaxies from the other side of the known universe or by reverse-engineering ancient stars from their descendants. However, the discovery of ancient stars on our cosmic doorstep gives scientists a rare opportunity to study them directly and researchers are now confident there are more stars like these toward our galaxy's edge.

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-    This revealed the stellar trio, which each had an unusually low abundance of heavy metals such as iron, strontium and barium in its atmosphere.    One of the stars had around 10,000 times less iron than the sun.

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-    These heavy metals are forged over eons in the heart of stars, and are also found in the exteriors of younger stars, which suck up ingredients that were dispersed by exploding dead stars. The fact that this trio has few heavy metals, means they were formed before most other stars had exploded.

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-    The stars' compositions hinted that they did not originate in the Milky Way. But to confirm this, they traced the orbital trajectories of the three stars and found that they all had a retrograde motion, meaning they are circling our galaxy's supermassive black hole in the opposite direction from a majority of the other stars.

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-    The only way you can have stars going the wrong way from the rest is if you threw them in the wrong way, meaning that these stars were likely ripped from other galaxies by the Milky Way.

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-   Astronomers have identified another 65 retrograde stars with similarly simple compositions. These stars will be studied further to determine if they are also SASS stars.

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-

June 26, 2024         THE  OLDEST  STARS  -  are circling our galaxy                   4515

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---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Sunday, June 30, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Saturday, June 29, 2024

 

-    4514  -   DARK  ENERGY  -  what is expanding the Universe?    Some 13.8 billion years ago, the universe began with a rapid expansion we call the “big bang”. After this initial expansion, which lasted a fraction of a second, gravity started to slow the universe down.  Nine billion years after the universe began, its expansion started to speed up, driven by an unknown force that scientists have named “dark energy”.  But what exactly is dark energy?



---------------  4514  -   DARK  ENERGY  -  what is expanding the Universe?

-     We don't know. But we do know that it exists, it’s making the universe expand at an accelerating rate, and approximately 68.3 to 70% of the universe is this “dark energy”, whatever it is?.

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-   Dark energy wasn't discovered until the late 1990s. But its origin in scientific study stretches all the way back to 1912 when American astronomer Henrietta Swan Leavitt made an important discovery using Cepheid variables, a class of stars whose brightness fluctuates with a regularity that depends on the star's brightness.

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-    All Cepheid stars with a certain period (a Cepheid’s period is the time it takes to go from bright, to dim, and bright again) have the same absolute magnitude, or luminosity, the amount of light they put out. Leavitt measured these stars and proved that there is a relationship between their regular period of brightness and luminosity.

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-     Leavitt’s findings made it possible for astronomers to use a star’s period and luminosity to measure the distances between us and Cepheid stars in far-off galaxies and our own Milky Way.

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-    Around this same time in history, astronomer Vesto Slipher observed spiral galaxies using his telescope’s spectrograph, a device that splits light into the colors that make it up, much like the way a prism splits light into a rainbow. He used the spectrograph to see the different wavelengths of light coming from the galaxies in different spectral lines.

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-    With his observations, Silpher was the first astronomer to observe how quickly the galaxy was moving away from us, called “redshift”, in distant galaxies. These observations would prove to be critical for many future scientific breakthroughs, including the discovery of dark energy.

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-    Redshift is a term used when astronomical objects are moving away from us and the light coming from those objects stretches out. Light behaves like a wave, and red light has the longest wavelength. So, the light coming from objects moving away from us has a longer wavelength, stretching to the “red end” of the electromagnetic.

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-    The discovery of galactic redshift, the period-luminosity relation of Cepheid variables, and a newfound ability to gauge a star or galaxy’s distance eventually played a role in astronomers observing that galaxies were getting farther away from us over time, which showed how the universe was expanding.

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-    In 1922, Russian scientist and mathematician Alexander Friedmann published a paper detailing multiple possibilities for the history of the universe. The paper, which was based on Albert Einstein’s theory of general relativity published in 1917, included the possibility that the universe is expanding.

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-    In 1927, Belgian astronomer Georges Lemaître published a paper also factoring in Einstein’s theory of general relativity. And, while Einstein stated in his theory that the universe was static, Lemaître showed how the equations in Einstein’s theory actually support the idea that the universe is not static but, in fact, is actually expanding.

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-    Astronomer Edwin Hubble confirmed that the universe was expanding in 1929 using observations made by his associate, astronomer Milton Humason. Humason measured the redshift of spiral galaxies. Hubble and Humason then studied Cepheid stars in those galaxies, using the stars to determine the distance of their galaxies (or nebulae, as they called them). -

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-     They compared the distances of these galaxies to their redshift and tracked how the farther away an object is, the bigger its redshift and the faster it is moving away from us. The pair found that objects like galaxies are moving away from Earth faster the farther away they are, at upwards of hundreds of thousands of miles per second,  This observation is now known as Hubble’s Law, or the Hubble-Lemaître law. The universe, they confirmed, is really expanding.

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-    Scientists previously thought that the universe's expansion would likely be slowed down by gravity over time, an expectation backed by Einstein's theory of general relativity. But in 1998, everything changed when two different teams of astronomers observing far-off supernovae noticed that (at a certain redshift) the stellar explosions were dimmer than expected.

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-    While dim supernovae might not seem like a major find, these astronomers were looking at “Type 1a supernovae”, which are known to have a certain level of luminosity. So they knew that there must be another factor making these objects appear dimmer. Scientists can determine distance (and speed) using an objects' brightness, and dimmer objects are typically farther away (though surrounding dust and other factors can cause an object to dim).

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-    This led the scientists to conclude that these supernovae were just much farther away than they expected by looking at their redshifts.  And using the spectrum, they were able to figure out the objects’ redshift and, therefore, how fast they were moving away from us. They found that the supernovae were not as close as expected, meaning they had traveled farther away from us faster than ancitipated. These observations led scientists to ultimately conclude that the universe itself must be expanding faster over time.

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-    While other possible explanations for these observations have been explored, astronomers studying even more distant supernovae or other cosmic phenomena in more recent years continued to gather evidence and build support for the idea that the universe is expanding faster over time, a phenomenon now called “cosmic acceleration”.   What could be driving the universe to stretch out faster over time?

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-    Right now, “dark energy” is just the name that astronomers gave to the mysterious "something" that is causing the universe to expand at an accelerated rate.   Dark energy has been described by some as having the effect of a negative pressure that is pushing space outward. However, we don't know if dark energy has the effect of any type of force at all. There are many ideas floating around about what dark energy could possibly be.

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-   Some scientists think that dark energy is a fundamental, ever-present background energy in space known as “vacuum energy”, which could be equal to the cosmological constant, a mathematical term in the equations of Einstein's theory of general relativity. Originally, the constant existed to counterbalance gravity, resulting in a static universe. But when Hubble confirmed that the universe was actually expanding, Einstein removed the constant, calling it “my biggest blunder” .

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-   But when it was later discovered that the universe’s expansion was actually accelerating, some scientists suggested that there might actually be a non-zero value to the previously-discredited cosmological constant. They suggested that this additional force would be necessary to accelerate the expansion of the universe. This theorized that this mystery component could be attributed to something called “vacuum energy,” which is a theoretical background energy permeating all of space.

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-   Space is never exactly empty. According to quantum field theory, there are virtual particles, or pairs of particles and antiparticles. It's thought that these virtual particles cancel each other out almost as soon as they crop up in the universe, and that this act of popping in and out of existence could be made possible by “vacuum energy” that fills the cosmos and pushes space outward.

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-    While this theory has been a popular topic of discussion, scientists investigating this option have calculated how much vacuum energy there should theoretically be in space. They showed that there should either be so much vacuum energy that, at the very beginning, the universe would have expanded outwards so quickly and with so much force that no stars or galaxies could have formed, or… there should be absolutely none.

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-    This means that the amount of vacuum energy in the cosmos must be much smaller than it is in these predictions. However, this discrepancy has yet to be solved and has even earned the moniker "the cosmological constant problem."

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-    Some scientists think that dark energy could be a type of energy fluid or field that fills space, behaves in an opposite way to normal matter, and can vary in its amount and distribution throughout both time and space. This hypothesized version of dark energy has been nicknamed “quintessence” after the theoretical fifth element discussed by ancient Greek philosophers.

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-   It's even been suggested by some scientists that quintessence could be some combination of dark energy and dark matter, though the two are currently considered completely separate from one another. While the two are both major mysteries to scientists, dark matter is thought to make up about 85% of all matter in the universe.

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-   Some scientists think that dark energy could be a sort of defect in the fabric of the universe itself; defects like cosmic strings, which are hypothetical one-dimensional "wrinkles" thought to have formed in the early universe.

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-    Some scientists think that dark energy isn't something physical that we can discover. Rather, they think there could be an issue with general relativity and Einstein's theory of gravity and how it works on the scale of the observable universe. Within this explanation, scientists think that it's possible to modify our understanding of gravity in a way that explains observations of the universe made without the need for dark energy.

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- Einstein actually proposed such an idea in 1919 called unimodular gravity, a modified version of general relativity that scientists today think wouldn't require dark energy to make sense of the universe.

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-    Dark energy is one of the great mysteries of the universe. For decades, scientists have theorized about our expanding universe.

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-    NASA plays a critical role in the ESA (European Space Agency) mission Euclid (launched in 2023), which will make a 3D map of the universe to see how matter has been pulled apart by dark energy over time. This map will include observations of billions of galaxies found up to 10 billion light-years from Earth.

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-    NASA's Nancy Grace Roman Space Telescope, set to launch by May 2027, is designed to investigate dark energy, among many other science topics, and will also create a 3D dark matter map. Roman's resolution will be as sharp as NASA’s Hubble Space Telescope's, but with a field of view 100 times larger, allowing it to capture more expansive images of the universe. This will allow scientists to map how matter is structured and spread across the universe and explore how dark energy behaves and has changed over time. Roman will also conduct an additional survey to detect Type Ia supernovae.

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-    In addition to NASA’s missions and efforts, the Vera C. Rubin Observatory, supported by a large collaboration that includes the U.S. National Science Foundation, which is currently under construction in Chile, is also poised to support our growing understanding of dark energy. The ground-based observatory is expected to be operational in 2025.

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-   The combined efforts of “Euclid, Roman, and Rubin” will usher in a new “golden age” of cosmology, in which scientists will collect more detailed information than ever about the great mysteries of dark energy.

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-   Additionally, NASA's James Webb Space Telescope (launched in 2021), the world’s most powerful and largest space telescope, aims to make contributions to several areas of research, and will contribute to studies of dark energy.

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-   NASA's SPHEREx (the Spectro-Photometer for the History of the Universe, Epoch of Reionization, and Ices Explorer) mission, scheduled to launch no later than April 2025, aims to investigate the origins of the universe. Scientists expect that the data collected with SPHEREx, which will survey the entire sky in near-infrared light, including over 450 million galaxies, could help to further our understanding of dark energy.

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-   NASA also supports a citizen science project called “Dark Energy Explorers”, which enables anyone in the world, even those who have no scientific training, to help in the search for dark energy answers.  Let us know as soon as you figure it out!

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June 29, 2024     DARK  ENERGY  -  what is expanding the Universe?                 4514

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--------  Comments appreciated and Pass it on to whomever is interested. ---

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--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Saturday, June 29, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Thursday, June 27, 2024

4513 - EARLIEST GALAXIES ?

 

-    4513  - EARLIEST  GALAXIES  ?      Using the James Webb Space telescope researchers have become the first to see the formation of three of the earliest galaxies in the universe, more than 13,000,000,000  years ago.



---------------------------------  4513  -   EARLIEST  GALAXIES  ?

-   For the first time in the history of astronomy, researchers have witnessed the birth of three of the universe's earliest galaxies, somewhere between 13.3 and 13.4 billion years ago.

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-    Through the telescope, researchers were able to see signals from large amounts of gas that accumulate and accrete onto a mini-galaxy in the process of being built. While this is how galaxies are formed according to theories and computer simulations, it had never actually been witnessed.

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-    These are the first 'direct' images of galaxy formation that we've ever seen. Whereas the James Webb has previously shown us early galaxies at later stages of evolution, here we witness their very birth, and the construction of the first star systems in the universe.

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-   They estimate the birth of the three galaxies to have occurred roughly 400-600 million years after the Big Bang, the explosion that began it all. While that sounds like a long time, it corresponds to galaxies forming during the first three to four percent of the universe's 13.8-billion-year overall lifetime.

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-   Shortly after the Big Bang, the universe was an enormous opaque gas of hydrogen atoms, unlike today, where the night sky is speckled with a blanket of well-defined stars.   During the few hundred million years after the Big Bang, the first stars formed, before stars and gas began to coalesce into galaxies.

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-   The birth of galaxies took place at a time in the history of the universe known as the “Epoch of Reionization”, when the energy and light of some of the first galaxies broke through the mists of hydrogen gas.

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-   It is these large amounts of hydrogen gas that the researchers captured using the James Webb Space Telescope's infrared vision. This is the most distant measurement of the cold, neutral hydrogen gas, which is the building block of the stars and galaxies.

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-   We are constantly trying to push the limit of how far out into the universe we can see.   One of the most fundamental questions that we humans have always asked is: 'Where do we come from?'. Here, we piece together a bit more of the answer by shedding light on the moment that some of the universe's first structures were created.

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-   Researchers were able to measure the formation of the universe's first galaxies by using sophisticated models of how light from these galaxies was absorbed by the neutral gas located in and around them. This transition is known as the “Lyman-alpha transition”.

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-    By measuring the light, the researchers were able to distinguish gas from the newly formed galaxies from other gas. These measurements were only possible thanks to the James Webb Space Telescope's incredibly sensitive infrared spectrograph capabilities.

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-    The universe began its "life" about 13.8 billion years ago in an enormous explosion, the Big Bang. The event gave rise to an abundance of subatomic particles such as quarks and electrons. These particles aggregated to form protons and neutrons, which later coalesced into atomic nuclei. Roughly 380,000 years after the Big Bang, electrons began to orbit atomic nuclei, and the simplest atoms of the universe gradually formed.

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-    The first stars were formed after a few hundred million years. And within the hearts of these stars, the larger and more complex atoms that we have around us were formed.

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-    Later, stars coalesced into galaxies. The oldest galaxies known to us were formed about

400 million years after the Big Bang. Our own solar system came into being about 4.6 billion years ago, more than 9 billion years after the Big Bang.

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June 27, 2024                EARLIEST  GALAXIES  ?                     4513

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---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Thursday, June 27, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Monday, June 24, 2024

4512 - ASTEROIDS - protecting the Earth?

 

-    4512  - ASTEROIDS  -  protecting the Earth?  -    The key to protecting Earth from being hit by asteroids is knowing where all these are.  More than 27,000 asteroids in our solar system had been overlooked in existing telescope images. Thanks to a new AI-powered algorithm, we now have a catalog of them.

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--------------------------  4512  -   ASTEROIDS  -  protecting the Earth?

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-    The scientists behind the discovery say the tool makes it easier to find and track millions of asteroids, including potentially dangerous ones that might strike Earth someday. It is for those threatening space rocks that the world would need years of advance warning before trying to deflect them away from our planet.

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-    Most of the newfound asteroids hover in the asteroid belt between Mars and Jupiter, where scientists have already cataloged over 1.3 million such rocky shards over the past 200 years. The latest bounty includes about 150 space rocks whose paths glide them within Earth's orbit; to be clear, however, none of these "near-Earth asteroids" seem to be on a collision path with our planet.

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-    Others are Trojans that follow Jupiter in its orbit around the sun. Observations of these asteroids are yet to be submitted to the official body responsible for asteroid discoveries.

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-    Astronomers conventionally find new asteroids by studying pockets of our sky over and over again, through telescope images gathered multiple times each night — usually every few hours. While planets, stars and galaxies in the background remain unchanged from one image to the next, asteroids are spotted as specks of light that move noticeably, which are then flagged and verified. From there, orbits of these asteroids are determined and monitored.

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-    This is really a job for AI.   AI tools designed for asteroid searches are already approaching levels attainable by humans.   The algorithm known as “Tracklet-less Heliocentric Orbit Recovery”, or THOR, analyzed over 400,000 archival images of the sky maintained by the National Optical-Infrared Astronomy Research Laboratory, or NOIRLab.

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-    As long as there are about five observations in 30 days associated with the same pocket of the sky, the algorithm can get to work. It's trained on a large dataset that makes it capable of analyzing as many as 1.7 billion light dots in just a single telescope image.

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-    It is designed to scope out and connect a point of light from one image of the sky to another one in a different image, and determine whether both specks represent the same object.   More often than not, that indicates an asteroid moving through space.

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-    The scientists scaled their algorithm using Google Cloud, whose computational heft and data storage services made it easier for the scientists to test out thousands of orbits of asteroid candidates.

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-    In 2022,  scientists used THOR to discover 100 asteroids that had been undetected in existing telescope images. Other teams of astronomers have also leveraged AI to find new asteroids.   Citizen scientists spearheaded training of an algorithm that led to the discovery of 1,000 new asteroids in archival images clicked by the Hubble Space Telescope.

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-   Last July, a software named “HelioLinc3D” designed to hunt for near-Earth asteroids found a 600-foot-wide space rock expected to approach within 140,000 miles of Earth. That's closer than the average distance between our planet and the moon.

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-   Scientists have so far spotted over 2,000 such "potentially hazardous asteroids" and estimate about 2,000 more are yet to be discovered. Detecting these space rocks in an effort to aid planetary defense is one of the tasks of the upcoming Vera C. Rubin Observatory in Chile, for which the asteroid-hunting HelioLinc3D software was developed.

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-    The 8.4-meter telescope, which is scheduled to start operations in 2025, will take images of the southern sky every night for at least a decade, each image covering 40-full-moons of area. Scientists say this cadence, supported by AI-based software like THOR and HelioLinc3D, could help the observatory find as many as 2.4 million asteroids, double than those now cataloged, in its first six months of operations.

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June 13, 2024            ASTEROIDS  -  prortecting the Earth?                    4512

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---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, June 24, 2024  ---------------------------------

 

 

 

 

 

           

 

 

4511 - ASTEROIDS - close to Earth?

-    4511  -   ASTEROIDS  -   close to Earth?      This asteroid will get closer to Earth than any in human history.   On Friday, April 13, 2029 a massive asteroid passes safely past Earth.   Asteroid “Apophis” is 1,230 feet  across, larger than 90% of space rocks.

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-------------------------------  4511  - ASTEROIDS  -   close to Earth?

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-    Asteroid “Apophis” will pass just 19,635 miles from Earth’s surface, the closest approach of an asteroid of this size that humankind has ever experienced. It will pass between Earth’s geostationary satellites and the Atlantic Ocean, just a tenth of the distance between Earth and the moon.

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-    “Apophis” will be visible to the naked eye. As it crosses the Atlantic, a few billion people in Europe, Africa and Asia can see it for a few hours in the night sky if skies are clear.

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-   “Asteroid 99942”,  “Apophis” was discovered on June 19, 2004, by astronomers at Kitt Peak National Observatory, who revealed that this stony, S-type asteroid orbits the sun every 324 days and comes close to Earth every decade or so. It is calculated that it could strike Earth in 2029, 2036 or 2068. It was, therefore, named after Apophis, the Egyptian demon of chaos and destruction.

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-    Even though there was only a 2.7% chance of a direct hit by Apophis, the devastation caused by it striking Earth led astronomers to try to understand its orbit in more detail.

 An asteroid’s orbit can only be calculated so far into the future. Although the following time it comes close to Earth, in 2044, it will be at a greater distance, astronomers can only rule out an impact for the next 100 years.

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-   The calculations are difficult because a close flyby, such as the one in 2029, will alter Apophis’ orbit so that it could strike Earth in a future orbit. However, astronomers have reduced the uncertainty in Apophis’ orbit from hundreds to just a few miles.

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-   The close pass in 2029 of Apophis is a rare opportunity to visit, so NASA already has a spacecraft in hot pursuit. This close pass is seen as the perfect opportunity to learn more about planetary defense and how an asteroid reacts to passing so close to a body with such enormous gravity. It’s thought that Apophis will be squeezed so much that asteroid quakes and landslides could result.

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-    Watching closely will be NASA’s OSIRIS-Apophis Explorer (OSIRIS-APEX) spacecraft. It’s the identical spacecraft that 2020 visited Asteroid Bennu. Then called OSIRIS-REx, NASA’s first asteroid sample-return mission, it returned a package of samples to Utah in September 2023 before re-directing towards Apophis in a mission extension costing NASA $200 million. OSIRIS-APEX will orbit Apophis for 18 months as it passes Earth in 2029.

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-   The European Space Agency is also considering a mission to Apophis, the Rapid Apophis Mission for SEcurity and Safety (RAMSES) mission, to launch in 2027.  What scientists learn from sending spacecraft to study Apophis in 2029 will be about how a relic of the early solar system reacts to gravity. The findings could be crucial for future Earthlings in hundreds of years when the massive asteroid poses a bigger threat.

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-    The key to protecting Earth from being hit by asteroids is knowing where all these are. More than 27,000 asteroids in our solar system had been overlooked in existing telescope images.   But,  thanks to a new AI-powered algorithm, we now have a catalog of them. The scientists behind the discovery say the tool makes it easier to find and track millions of asteroids, including potentially dangerous ones that might strike Earth someday.

-

-    It is for those threatening space rocks that the world would need years of advance warning before trying to deflect them away from our planet.    Most of the newfound asteroids hover in the asteroid belt between Mars and Jupiter, where scientists have already cataloged over 1.3 million such rocky shards over the past 200 years.

-

-    The latest bounty includes about 150 space rocks whose paths glide them within Earth's orbit;  however, none of these "near-Earth asteroids" seem to be on a collision path with our planet. Others are “Trojans” that follow Jupiter in its orbit around the sun.

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-    Astronomers conventionally find new asteroids by studying pockets of our sky over and over again, through telescope images gathered multiple times each night, usually every few hours. While planets, stars and galaxies in the background remain unchanged from one image to the next, asteroids are spotted as specks of light that move noticeably, which are then flagged and verified. From there, orbits of these asteroids are determined and monitored.

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-    This is really a job for AI.  In fact, AI tools designed for asteroid searches are already approaching levels attainable by humans.   The algorithm is known as “Tracklet-less Heliocentric Orbit Recovery”, or THOR, analyzed over 400,000 archival images of the sky maintained by the National Optical-Infrared Astronomy Research Laboratory, or NOIRLab.

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-    As long as there are about five observations in 30 days associated with the same pocket of the sky, the algorithm can get to work. It's trained on a large dataset that makes it capable of analyzing as many as 1.7 billion light dots in just a single telescope image. It is designed to scope out and connect a point of light from one image of the sky to another one in a different image, and determine whether both specks represent the same object.  More often than not, that indicates an asteroid moving through space.

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-    The scientists scaled their algorithm using Google Cloud, whose computational heft and data storage services made it easier for the scientists to test out thousands of orbits of asteroid candidates. 

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-    In 2022, the same team of scientists used THOR to discover 100 asteroids that had been undetected in existing telescope images. Other teams of astronomers have also leveraged AI to find new asteroids.

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-   Citizen scientists spearheaded training of an algorithm that led to the discovery of 1,000 new asteroids in archival images clicked by the Hubble Space Telescope. Last July, a software named “HelioLinc3D” designed to hunt for near-Earth asteroids found a 600-foot-wide space rock expected to approach within 140,000 miles of Earth. That's closer than the average distance between our planet and the moon.

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-    Scientists have so far spotted over 2,000 such "potentially hazardous asteroids" and estimate about 2,000 more are yet to be discovered. Detecting these space rocks in an effort to aid planetary defense is one of the tasks of the upcoming Vera C. Rubin Observatory in Chile, for which the asteroid-hunting HelioLinc3D software was developed.

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-    The 8.4-meter telescope, which is scheduled to start operations in 2025, will take images of the southern sky every night for at least a decade, each image covering 40-full-moons of area. Scientists say this cadence, supported by AI-based software like THOR and HelioLinc3D, could help the observatory find as many as 2.4 million asteroids,  double than those now cataloged in its first six months of operations.

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June 23, 2024           ASTEROIDS  -   close to Earth?                    4511

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--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Monday, June 24, 2024  ---------------------------------

 

 

 

 

 

           

 

  

Sunday, June 23, 2024

 

-    4510  -  WEBB  TELESCOPE'S    -  new discoveries?   When the James Webb Space Telescope was launched at the end of 2021, we expected stunning images and illuminating scientific results. So far, the powerful space telescope has lived up to our expectations. The JWST has shown us things about the early universe we never anticipated.

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-------------------------------  4510  -  WEBB  TELESCOPE'S    -  new discoveries? 

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-     The early universe is one of the JWST's primary scientific targets. Its infrared capabilities allow it to see the light from ancient galaxies with greater acuity than any other telescope. The telescope was designed to directly address confounding questions about the high-redshift universe.

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-    The early universe and its transformations are fundamental to our understanding of the universe around us today. Galaxies were in their infancy, stars were forming, and black holes were forming and becoming more massive.

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-   The Hubble Space Telescope was limited to observations at about z=11. The JWST  current high-redshift observations have reached z=14.32. Astronomers think that the JWST will eventually observe galaxies at z=20.

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-   The first few hundred million years after the Big Bang is called the “Cosmic Dawn”. JWST showed us that ancient galaxies during the Cosmic Dawn were much more luminous and, therefore, larger than we expected. The galaxy the telescope found at z=14.32, called JADES-GS-z14-0, has several hundred million solar masses.

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-     How can nature make such a bright, massive, and large galaxy in less than 300 million years?"   They were differently shaped, that they contained more dust than expected, and that oxygen was present. The presence of oxygen indicates that generations of stars had already lived and died.   The presence of oxygen so early in the life of this galaxy is a surprise and suggests that multiple generations of very massive stars had already lived their lives before we observed the galaxy.

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-    JADES-GS-z14-0 is not like the types of galaxies that have been predicted by theoretical models and computer simulations to exist in the very early universe.  Active galactic nuclei (AGN) are supermassive black holes (SMBHs) that are actively accreting material and emitting jets and winds.

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-   Quasars are a sub-type of AGN that are extremely luminous and distant, and quasar observations show that SMBHs were present in the centers of galaxies as early as 700 million years after the Big Bang. But their origins were a mystery.

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-   Astrophysicists think that these early SMBHs were created from black hole "seeds" that were either "light" or "heavy." Light seeds had about 10 to 100 solar masses and were stellar remnants. Heavy seeds had 10 to 105 solar masses and came from the direct collapse of gas clouds.

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-    The JWST's ability to effectively look back in time has allowed it to spot an ancient black hole at about z=10.3 that contains between 107 to 108 solar masses. The Hubble Space Telescope didn't allow astronomers to measure the stellar mass of entire galaxies the way that the JWST does.

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-    Astronomers know that the black hole at z=10.3 has about the same mass as the stellar mass of its entire galaxy. This is in stark contrast to modern galaxies, where the mass of the black hole is only about 0.1% of the entire stellar mass.

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-   Such a massive black hole existing only about 500 million years after the Big Bang is proof that early black holes originated from heavy seeds. This is actually in line with theoretical predictions.

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-    We know that in the early universe, hydrogen became ionized during the Epoch of Reionization (EoR). Light from the first stars, accreting black holes, and galaxies heated and reionized the hydrogen gas in the intergalactic medium (IGM), removing the dense, hot, primordial fog that suffused the early universe.

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-    Young stars were the primary light source for the reionization. They created expanding bubblesof ionized hydrogen that overlapped one another. Eventually, the bubbles expanded until the entire universe was ionized.

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-   This was a critical phase in the development of the universe. It allowed future galaxies, especially dwarf galaxies, to cool their gas and form stars. But scientists aren't certain how black holes, stars, and galaxies contributed to the reionization or the exact time frame in which it took place.

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-    We know that hydrogen reionization happened, but exactly when and how it happened has been a major missing piece in our understanding of the first billion years.  Astronomers knew that reionization ended about 1 billion years after the Big Bang, at about redshift z=5-6. But before the JWST, it was difficult to measure the properties of the UV light that caused it. With the JWST's advanced spectroscopic capabilities, astronomers have narrowed down the parameters of reionization.

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-    We have found spectroscopically confirmed galaxies up to z = 13.2, implying reionization may have started just a few hundred million years after the Big Bang.  JWST results also show that accreting black holes and their AGN likely contributed no more than 25% of the UV light that caused reionization.

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-   There is still significant debate about the primary sources of reionization, in particular, the contribution of faint galaxies. Even though the JWST is extraordinarily powerful, some distant, faint objects are beyond its reach.

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-    The JWST is not even halfway through its mission and has already transformed our understanding of the universe's first one billion years. It was built to address questions around the Epoch of Reionization, the first black holes, and the first galaxies and stars. There's definitely much more to come. Who knows what the sum total of its contributions will be?

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-    Among the most fundamental questions in astronomy is: How did the first stars and galaxies form?    For hundreds of millions of years after the Big Bang, the universe was filled with a gaseous fog that made it opaque to energetic light. By one billion years after the Big Bang, the fog had cleared and the universe became transparent, a process known as “reionization”. Scientists have debated whether active, supermassive black holes or galaxies full of hot, young stars were the primary cause of reionization.

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-   Almost every single galaxy that we are finding shows these unusually strong emission line signatures indicating intense recent star formation. These early galaxies were very good at creating hot, massive stars.

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-    These bright, massive stars pumped out torrents of ultraviolet light, which transformed surrounding gas from opaque to transparent by ionizing the atoms, removing electrons from their nuclei. Since these early galaxies had such a large population of hot, massive stars, they may have been the main driver of the reionization process. The later reuniting of the electrons and nuclei produces the distinctively strong emission lines.

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-   These young galaxies underwent periods of rapid star formation interspersed with quiet periods where fewer stars formed. These fits and starts may have occurred as galaxies captured clumps of the gaseous raw materials needed to form stars. Alternatively, since massive stars quickly explode, they may have injected energy into the surrounding environment periodically, preventing gas from condensing to form new stars.

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-    The light from faraway galaxies is stretched to longer wavelengths and redder colors by the expansion of the universe—a phenomenon called “redshift”. By measuring a galaxy's redshift, astronomers can learn how far away it is, and therefore, when it existed in the early universe. Before Webb, there were only a few dozen galaxies observed above a redshift of 8, when the universe was younger than 650 million years old, but JADES has now uncovered nearly a thousand of these extremely distant galaxies.

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-    Determining redshift involves looking at a galaxy's spectrum, which measures its brightness at myriad closely spaced wavelengths. But a good approximation can be determined by taking photos of a galaxy using filters that each cover a narrow band of colors to get a handful of brightness measurements. In this way, researchers can determine estimates for the distances of many thousands of galaxies at once.

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-   More than 700 candidate galaxies existed when the universe was between 370 million and 650 million years old. The sheer number of these galaxies was far beyond predictions from observations made before Webb's launch. The observatory's exquisite resolution and sensitivity are allowing astronomers to get a better view of these distant galaxies than ever before.

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-    James Webb Space Telescope has discovered the four most distant galaxies ever observed, one of which formed just 320 million years after the Big Bang when the universe was still in its infancy.

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-    By the time light from the most distant galaxies reaches Earth, it has been stretched by the expansion of the universe and shifted to the infrared region of the light spectrum.  The Webb telescope's NIRCam instrument has an unprecedented ability to detect this infrared light, allowing it to quickly spot a range of never-before-seen galaxies..

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-    The galaxies date from 300 to 500 million years after the Big Bang more than 13 billion years ago, when the universe was just two percent of its current age.  That means the galaxies are from what is called "the epoch of reionisation," a period when the first stars are believed to have emerged. The epoch came directly after the cosmic dark ages brought about by the Big Bang.

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-    The Webb telescope confirmed the existence of JADES-GS-z10-0, which dates from 450 million years after the Big Bang and had previously been spotted by the Hubble Space Telescope.   All four galaxies are "very low in mass," weighing roughly a hundred million solar masses. The Milky Way, in comparison, weighs 1.5 trillion solar masses by some estimations.

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-   The galaxies are very active in star formation in proportion to their mass.   The galaxies were also "very poor in metals.  This is consistent with the standard model of cosmology, science's best understanding of how the universe works, which says that the closer to the Big Bang, the less time there is for such metals to form.

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-    However, the discovery of six massive galaxies from 500-700 million years after the Big Bang led some astronomers to question the standard model.   Those galaxies, also observed by the Webb telescope, were bigger than thought possible so soon after the birth of the universe.

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June 23, 2024                            4511

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--------  Comments appreciated and Pass it on to whomever is interested. ---

---   Some reviews are at:  --------------     http://jdetrick.blogspot.com ----- 

--  email feedback, corrections, request for copies or Index of all reviews

---  to:  ------    jamesdetrick@comcast.net  ------  “Jim Detrick”  -----------

--------------------- ---  Sunday, June 23, 2024  ---------------------------------