Tuesday, November 30, 2021

3360 - PHYSICS - mysteries yet to be solved?

  -  3360   -  PHYSICS  -   mysteries yet to be solved?  Today, no physicist would dare assert that our physical knowledge of the universe is near completion. To the contrary, each new discovery seems to unlock a Pandora's box of even bigger, even deeper physics questions. 


---------------------  3360  -    PHYSICS  -   mysteries yet to be solved?

-  In 1900, the British physicist Lord Kelvin pronounced: "There is nothing new to be discovered in physics now. All that remains is more and more precise measurement." 

Within three decades, quantum mechanics and Einstein's theory of relativity had revolutionized the field. 

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-  No matter how astrophysicists crunch the numbers, the universe simply doesn't add up. Even though gravity is pulling inward on space-time, the "fabric" of the universe, it keeps expanding outward faster and faster.  The Universe expansion is accelerating!

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-   To explain this astrophysicists have proposed an invisible agent that counteracts gravity by pushing space-time apart. They call it “dark energy“. In the most widely accepted model of dark energy, it is a "cosmological constant" which is an inherent property of space itself that has "negative pressure" driving space apart. 

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-  As space expands, more space is created, and with it, more dark energy. Based on the observed rate of expansion, scientists know that the sum of all the dark energy must make up more than 70 percent of the total  mass-energy contents of the universe.

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-  About 84 percent of the matter in the universe does not absorb or emit light. "Dark matter,"  cannot be seen directly, and it hasn't yet been detected by indirect means, either. Instead, dark matter's existence and properties are inferred from its gravitational effects on visible matter, radiation and the structure of the universe. 

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-  This shadowy dark matter substance is thought to pervade the outskirts of galaxies, and may be composed of "weakly interacting massive particles," or WIMPs. Worldwide, there are several detectors on the lookout for WIMPs, but so far, not one has been found. 

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-   Dark mater might form long, fine-grained streams throughout the universe, and that such streams might radiate out from Earth like hairs. 

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-  Entropy is the arrow of time?  The fact that you can't un-break an egg is a common example of the law of increasing entropy.  Time moves forward because a property of the universe called "entropy," roughly defined as the level of “disorder“, that only increases, and so there is no way to reverse a rise in entropy after it has occurred.  You can’t unbreak an egg!

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-   The fact that entropy increases is a matter of logic: There are more disordered arrangements of particles than there are ordered arrangements, and so as things change, they tend to fall into disarray. But the underlying question here is, why was entropy so low in the past?   Why was the universe so ordered at its beginning, when a huge amount of energy was crammed together in a small amount of space?

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-  Space-time might be "flat," rather than curved, and thus that it goes on forever. If so, then the region we can see (which we think of as "the universe") is just one patch in an infinitely large "quilted multiverse."

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-   At the same time, the laws of quantum mechanics dictate that there are only a finite number of possible particle configurations within each cosmic patch (10^10^122 distinct possibilities). 

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-   With an infinite number of cosmic patches, the particle arrangements within them are forced to repeat, infinitely many times over.  This means there are infinitely many parallel universes: cosmic patches exactly the same as ours as well as patches that differ by just one particle's position, patches that differ by two particles' positions, and so on down to patches that are totally different from ours.

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-  Is there something wrong with this logic, or is its bizarre outcome true? And if it is true, how might we ever detect the presence of parallel universes? Why is there more matter than antimatter?

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-  The question of why there is so much more matter than its oppositely-charged and oppositely-spinning twin, antimatter, is actually a question of why anything exists at all. One assumes the universe would treat matter and antimatter symmetrically, and thus that, at the moment of the Big Bang, equal amounts of matter and antimatter should have been produced.

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-   But if that had happened, there would have been a total annihilation of both: Protons would have canceled with antiprotons, electrons with anti-electrons (positrons), neutrons with antineutrons, and so on, leaving behind a sea of photons in a matterless expanse.

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-   For some reason, there was excess matter that didn't get annihilated, and here we are.  We exist as leftover matter!   For this, there is no accepted explanation. The most detailed test to date of the differences between matter and antimatter, announced in 2015, confirm they are mirror images of each other, providing exactly zero new paths toward understanding the mystery of why matter is far more common.

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-  The fate of the universe strongly depends on a factor of unknown value: “Ω ,  a measure of the density of matter and energy throughout the cosmos. If density Ω is greater than 1, then space-time would be "closed" like the surface of an enormous sphere.

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-   If there is no dark energy, such a universe would eventually stop expanding and would instead start contracting, eventually collapsing in on itself in an event dubbed the "Big Crunch." 

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-  If the universe is closed but there is dark energy, the spherical universe would expand forever.

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-  Alternatively, if Ω is less than 1, then the geometry of space would be "open" like the surface of a saddle. In this case, its ultimate fate is the "Big Freeze" followed by the "Big Rip": first, the universe's outward acceleration would tear galaxies and stars apart, leaving all matter frigid and alone. Next, the acceleration would grow so strong that it would overwhelm the effects of the forces that hold atoms together, and everything would be wrenched apart.

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-  If Ω = 1, the universe would be flat, extending like an infinite plane in all directions. If there is no dark energy, such a planar universe would expand forever but at a continually decelerating rate, approaching a standstill. 

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-  If there is dark energy, the flat universe ultimately would experience runaway expansion leading to the Big Rip. 

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-   In the strange realm of electrons, photons and the other fundamental particles, quantum mechanics is law. Particles don't behave like tiny balls, but rather like waves that are spread over a large area. 

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- Each particle is described by a "wavefunction," or “probability distribution“, which tells what its location, velocity, and other properties are more likely to be, but not what those properties are. 

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-  The particle actually has a range of values for all the properties, until you experimentally measure one of them, its location,  at which point the particle's wavefunction "collapses" and it adopts just one location. 

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-  But how and why does measuring a particle make its wavefunction collapse, producing the concrete reality that we perceive to exist? The issue, known as the measurement problem, may seem esoteric, but our understanding of what reality is, or if it exists at all, hinges upon the answer. 

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-  When physicists assume all the elementary particles are actually one-dimensional loops, or "strings," each of which vibrates at a different frequency, physics gets much easier. String theory allows physicists to reconcile the laws governing particles, called “quantum mechanics“, with the laws governing space-time, called “general relativity“, and to unify the four fundamental forces of nature into a single framework. 

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-  But the problem is, string theory can only work in a universe with 10 or 11 dimensions: three large spatial ones, six or seven compacted spatial ones, and a time dimension. The compacted spatial dimensions, as well as the vibrating strings themselves, are about a billionth of a trillionth of the size of an atomic nucleus. 

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-   There's no conceivable way to detect anything that small, and so there's no known way to experimentally validate or invalidate “string theory“.

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-  The equations that describe weather and water, among other things, have not been solved.  Physicists can't exactly solve the set of equations that describes the behavior of fluids, from water to air to all other liquids and gases.

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-   In fact, it isn't known whether a general solution of the so-called “Navier-Stokes equations” even exists, or, if there is a solution, whether it describes fluids everywhere, or contains inherently unknowable points called “singularities“.

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-   As a consequence, the nature of “chaos” is not well understood. Physicists and mathematicians wonder, is the weather merely difficult to predict, or inherently unpredictable? Does turbulence transcend mathematical description, or does it all make sense when you tackle it with the right math?

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-   Do the universe's forces merge into one?    The universe experiences four fundamental forces: electromagnetism, the strong nuclear force, the weak nuclear force  and gravity. To date, physicists know that if you turn up the energy enough three of those forces "unify" and become a single force. 

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-   Physicists have run particle accelerators and unified the electromagnetic force and weak force interactions, and at higher energies, the same thing should happen with the strong nuclear force and, eventually, with gravity.

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-  But even though theories say that should happen, nature doesn't always oblige. So far, no particle accelerator has reached energies high enough to unify the strong force with electromagnetism and the weak interaction. Including gravity would mean yet more energy.

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-   It isn't clear whether scientists could even build one that powerful; the Large Hadron Collider (LHC), near Geneva, can send particles crashing into each other with energies in the trillions of electron volts ( 14 tera-electron volts, or TeV). To reach grand unification energies, particles would need at least a trillion times as much, so physicists are left to hunt for “indirect evidence” of such theories. 

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-  This Grand Unified Theories (GUTs) still have some problems because they predict other observations that so far haven't been seen. There are several GUTs that say protons, over immense spans of time (on the order of 10^36 years), should turn into other particles. 

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-  This has never been observed, so either protons last much longer than anyone thought or they really are stable forever. Another prediction of some types of GUT is the existence of magnetic monopoles, isolated "north" and "south" poles of a magnet, and nobody has seen one of those, either. It's possible we just don't have a powerful enough particle accelerator. Or, physicists could be wrong about how the universe works. 

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-  According to the current theories, if you were to drop a cube of iron into a blackhole, there would be no way to retrieve any of that information. That's because a blackhole's gravity is so strong that its escape velocity is faster than light and light is the fastest thing there is.

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-   However, quantum mechanics says that quantum information can't be destroyed.   “Quantum information” is a bit different from the information we store as “1s’ and “0s” on a computer, or the stuff in our brains. 

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-  That's because quantum theories don't provide exact information about where an object will be, like calculating the trajectory of a baseball in mechanics. Instead, such theories reveal the most likely location or the most likely result of some action. 

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-  As a consequence, all of the probabilities of various events should add up to 1, or 100 percent.   When you roll a six-sided die, the chances of a given face coming up is one-sixth, so the probabilities of all the faces add up to 1, and you can't be more than 100 percent certain something will happen. Quantum theory is, therefore, called “unitary“. If you know how a system ends, you can calculate how it began.

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-  To describe a blackhole, all you need is mass, angular momentum (if it's spinning) and charge. Nothing comes out of a blackhole except a slow trickle of thermal radiation called “Hawking radiation“. 

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-  As far as anyone knows, there's no way to do that reverse calculation to figure out what the blackhole actually gobbled up. The information is destroyed. However, quantum theory says that information can't be completely out of reach. Therein lies the "information paradox."

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-  Rather than information being stored within the deep clutches of a blackhole, the information remains on its boundary, called the “event horizon“.  Do naked singularities exist?

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-  A singularity occurs when some property of a "thing" is infinite, and so the laws of physics as we know them break down. At the center of blackholes lies a point that is infinitely small and dense, packed with a finite amount of matter, a point called a “singularity“. 

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-  In mathematics, singularities come up all the time, dividing by zero is one instance, and a vertical line on a coordinate plane has an "infinite" slope. In fact, the slope of a vertical line is just undefined. 

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-  What would a singularity look like? And how would it interact with the rest of the universe? What does it mean to say that something has no real surface and is infinitely small?

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-  A "naked" singularity is one that can interact with the rest of the universe. Blackholes have event horizons,  spherical regions from which nothing, not even light, can escape. At first glance, you might think the problem of naked singularities is partly solved for black holes at least, since nothing can get out of the event horizon and the singularity can't affect the rest of the universe. It is "clothed,"  while a naked singularity is a blackhole without an event horizon.

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-   Whether singularities can form without an event horizon is still an open question. And if they can exist, then Albert Einstein's theory of general relativity will need a revision, because it breaks down when systems are too close to a singularity.

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-   Naked singularities might also function as wormholes, which would also be time machines ,though there's no evidence for this in nature.

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-  If you swap a particle with its antimatter sibling, the laws of physics should remain the same. So the positively charged proton should look the same as a negatively charged antiproton. That's the principle of “charge symmetry“. 

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-  If you swap left and right, again, the laws of physics should look the same. That's parity symmetry. Together, the two are called “CP symmetry“. Most of the time, this physics rule is not violated. However, certain exotic particles violate this symmetry.   There shouldn't be any violations of CP in quantum mechanics.  We don't know why that is.

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-  Though particle-physics questions account for many unsolved problems, some mysteries can be observed on a bench-top lab setup. “Sonoluminescence” is one of those. If you take some water and hit it with sound waves, bubbles will form.

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-   Those bubbles are low-pressure regions surrounded by high pressure; the outer pressure pushes in on the lower-pressure air, and the bubbles quickly collapse. When those bubbles collapse, they emit light, in flashes that last trillionths of a second.

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-  The problem is, it's far from clear what the source of the light is. Theories range from tiny nuclear fusion reactions to some type of electrical discharge, or even compression heating of the gases inside the bubbles. 

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-  Physicists have measured high temperatures inside these bubbles, on the order of tens of thousands of degrees Fahrenheit, and taken numerous pictures of the light they produce. But there's no good explanation of how sound waves create these lights in a bubble.

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-   The Standard Model is one of the most successful physical theories ever devised. It's been standing up to experiments to test it for four decades, and new experiments keep showing that it is correct. 

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-  The Standard Model describes the behavior of the particles that make up everything around us, as well as explaining why, for example, particles have mass. In fact, the discovery of the Higgs boson, a particle that gives matter its mass, in 2012 was a historic milestone because it confirmed the long-standing prediction of its existence. 

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-  But the Standard Model doesn't explain everything. The Standard Model has made many successful predictions, the Higgs boson, the W and Z boson (which mediate the weak interactions that govern radioactivity), and quarks among them, so it is difficult to see where physics might go beyond it.

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-   Most physicists agree that the Standard Model is not complete. There are several contenders for new, more complete models ,string theory is one such model, but so far, none of these have been conclusively verified by experiments. 

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-  Dimensionless constants are numbers that don't have units attached to them. The speed of light, for example, is a fundamental constant measured in units of meters per second (or 186,282 miles per second). Unlike the speed of light, dimensionless constants have no units and they can be measured, but they can't be derived from theories, whereas constants like the speed of light can be.

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-  Certain "dimensionless constants" are considered fundamental to physics. In fact, there are many more than six; about 25 exist in the Standard Model.   For example, the “fine structure constant“, usually written as alpha, governs the strength of magnetic interactions. 

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-  It is about 0.007297. What makes this number odd is that if it were any different, stable matter wouldn't exist. Another is the ratio of the masses of many fundamental particles, such as electrons and quarks, to the Planck mass, which is 1.22 ´1019 GeV/c2. 

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-  Physicists would love to figure out why those particular numbers have the values they do, because if they were very different, the universe's physical laws wouldn't allow for humans to be here. And yet there's still no compelling theoretical explanation for why they have those values. That is just what God decided.

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-  What is gravity? Other forces are mediated by particles. Electromagnetism is the exchange of photons. The weak nuclear force is carried by W and Z bosons, and gluons carry the strong nuclear force that holds atomic nuclei together.

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-   All of the other forces can be quantized, meaning they could be expressed as individual particles and have non-continuous values.  Gravity doesn't seem to be like that. Most physical theories say it should be carried by a hypothetical massless particle called a “graviton“. 

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-  The problem is, nobody has found gravitons yet, and it's not clear that any particle detector that could be built could see them, because if gravitons interact with matter, they do it very, very rarely.  So seldom that they'd be invisible against the background noise.

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-   It isn't even clear that gravitons are massless, though if they have a mass at all, it's very, very small, smaller than that of neutrinos, which are among the lightest particles known. 

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-  String theory posits that gravitons (and other particles) are closed loops of energy, but the mathematical work hasn't yielded much insight so far.  Because gravitons haven't been observed yet, gravity has resisted attempts to understand it in the way we understand other forces, as an exchange of particles. 

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-   Gravity may be operating as a particle in extra dimensions beyond the three of space (length, width, and height) and one of time (duration)we are familiar with, but whether that is true is still unknown. 

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-  The universe seems relatively stable. It has been around for about 13.8 billion years. But what if the whole thing were a massive accident?  It all starts with the Higgs Boson and the universe's vacuum.

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-   Vacuum, or empty space, should be the lowest possible energy state, because there's nothing in it. Meanwhile, the Higgs boson, via the so-called Higgs field, gives everything its mass. 

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-  The energy state of the vacuum can be calculated from the potential energy of the Higgs field and the masses of the Higgs and top quark.  So far, those calculations appear to show that the universe's vacuum might not be in the lowest possible energy state. 

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-  That would mean it's a “false vacuum“. If that's true, our universe might not be stable, because a false vacuum can be knocked into a lower energy state by a sufficiently violent and high-energy event.

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-   If that were to happen, there would be a phenomenon called “bubble nucleation“. A sphere of lower-energy vacuum would start growing at the speed of light. Nothing, not even matter itself, would survive. Effectively, we'd be replacing the universe with another one, which might have very different physical laws. We May Live in a Multiverse.

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-  The idea of a false vacuum means that our universe might have popped into existence in just that way, when a previous universe's false vacuum was knocked into a lower energy state. Perhaps we were the result of an accident with a particle accelerator.

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-  Those guys better e careful with throwing the wrong switch on that particle accelerator.  We may get swallowed up by another universe.   Then what would we do?

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November 28, 2021      PHYSICS  -   mysteries yet to be solved?               3360                                                                                                                                                  

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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”  -----------

--------------------- ---  Tuesday, November 30, 2021  ---------------------------






3363 - GALAXIES - beyond were light can see?

  -  3363   -  GALAXIES  -  beyond were light can see?  The present “reachability limit” has a boundary 18 billion light-years away.  The limit of the visible universe is 46.1 billion light-years, as that’s the limit of how far away an object that emitted light that would just be reaching us today would be after expanding away from us for 13.8 billion years.  


---------------------  3363  -   GALAXIES  -  beyond were light can see?  

-  Our universe, everywhere and in all directions, is filled with stars and galaxies.   Beyond our Milky Way galaxy are trillions of others galaxies, nearly all of which are expanding away from us. 

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-  From our vantage point, we observe up to 46,100,000,000 light-years away.  As long as the light from any galaxy that was emitted at the start of the hot Big Bang 13.8 billion years ago would have reached us by today, that object is within our presently observable universe. However, not every observable object is reachable. 

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-  Our visible universe contains an estimated 2 trillion galaxies.  The “Hubble eXtreme Deep Field” (XDF) survey may have observed a region of sky just 1/32,000,000th of the total, but was able to uncover 5,500 galaxies within it.  This is an estimated 10% of the total number of galaxies actually contained in this pencil-beam-style slice. 

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-  The remaining 90% of galaxies are either too faint or too red or too obscured for Hubble to reveal.  Most of them are already permanently unreachable by us.

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-  Although there are magnified, ultra-distant, very red and even infrared galaxies in the extreme Deep Field, there are galaxies that are even more distant out there than what we’ve discovered in our deepest-to-date views.   These galaxies will always remain visible to us, but we will never see them as they are today, 13.8 billion years after the Big Bang. 

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-  As the universe expands, the space between all unbound objects increases over time.

Light redshifts and distances between unbound objects change over time in the expanding universe.  The objects start off closer than the amount of time it takes light to travel between them, the light redshifts due to the expansion of space, and the two galaxies wind up much farther apart than the light-travel path taken by the photon exchanged between them.

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-  Beyond distances of 14.5 billion light-years, space’s expansion pushes galaxies away faster than light can travel.  

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-  Over time, the expansion rate still drops, but remains positive and large because of “dark energy“.  The expected fates of the universe  all correspond to a universe where the matter and energy combined fight against the initial expansion rate. In our observed universe, a cosmic acceleration is caused by some type of unexplained dark energy. 

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-  All of these universes are governed by the Friedmann equations, which relate the expansion of the universe to the various types of matter and energy present within it. 

Dark energy, inherent to space itself, never decreases, even as the universe expands.

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-     Radiation , and a cosmological constant  all evolve with time in an expanding universe. As the universe expands, the “matter density dilutes“, but the “radiation” also becomes cooler as its wavelengths get stretched to longer, less energetic states. Dark energy’s density will truly remain constant as a form of energy intrinsic to space itself.

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-  All galaxies beyond a certain distance always remain unreachable, even at the speed of light.  Our deepest galaxy surveys can reveal objects tens of billions of light years away, but there are more galaxies within the observable universe we still have yet to reveal. 

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-  There are parts of the universe that are not yet visible today that will someday become observable to us, and there are parts that are visible to us that are no longer reachable by us, even if we traveled at the speed of light. 

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-  The present “reachability limit” has a boundary 18 billion light-years away.  The limit of the visible universe is 46.1 billion light-years, as that’s the limit of how far away an object that emitted light that would just be reaching us today would be after expanding away from us for 13.8 billion years. 

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-  However, beyond about 18 billion light-years, we can never access a galaxy even if we traveled towards it at the speed of light.   All galaxies closer than that could be reached if we left today; all galaxies beyond that are unreachable.

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-  Given enough time, light that was emitted by a distant object will arrive at our eyes, even in an expanding universe. However, if a distant galaxy’s recession speed reaches and remains above the speed of light, we can never reach it, even if we can receive light from its distant past. 


-  Only 6% of presently observable galaxies remain reachable; 94% already lie beyond our reach.  

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-  The “GOODS-North survey“,  contains some of the most distant galaxies ever observed, a great many of which are already unreachable by us. As time marches forward, more and more galaxies suffer this same fate, disconnecting from us.   Each year, another 160 billion stars, enough to compose one major galaxy, become newly unreachable.

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-  The stars, in the M81 group, will become unreachable after another 100 billion years.  Located a mere 3.6 Megaparsecs away from our Local Group, the M81 group is the nearest substantial group of galaxies to our own Local Group, but will remain gravitationally unbound. 

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-  After 100 billion years, even these galaxies will become unreachable to us, even if we were to leave at the speed of light. After that, only our “Local Group of Galaxies” will remain within reach.

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- The Local Group of galaxies is dominated by Andromeda and the Milky Way, and additionally consists of about 60 other, smaller galaxies. All are located within 5 million light-years of one another, with the nearest galactic groups beyond our own remaining gravitationally unbound from ourselves for all-time. 

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-  Our understanding of blackholes is now central to our understanding of the cosmos. The next generation “Very Large Array” (ngVLA) will help astronomers study these mysterious objects.

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-  Astronomers have long known that Einstein's theory of gravity allowed for an object to be so massive that light itself could not escape, but they initially doubted that blackholes existed in the Universe.

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-  Today blackholes are recognized as a standard result of the death of very massive stars. 

A century ago, astronomers thought that the Universe consisted mostly of stars. They shine with the colors of light that our human eyes can see, and to most of us, the picture of an astronomer includes a telescope turned to the heavens. 

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-  Today, we now recognize that a variety of objects shine at wavelengths that our eyes cannot see, from long wavelength radio waves to extremely high-energy gamma rays.  We now know that there are a variety of other messengers carrying to us information about the Universe.

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-   Cosmic rays are energetic sub-atomic particles, with energies well above those that particle accelerators such as the Large Hadron Collider can produce. In the most extreme cases, a sub-atomic particle can hit the Earth's atmosphere with as much energy as a fast-pitch baseball. 

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-  Billions of neutrinos rain upon us every second. They are born from nuclear fusion in the Sun, from distant exploding stars, and from the regions near supermassive blackholes. And gravitational waves constantly wash over the Earth and the Solar System. These distortions of spacetime itself are generated by colliding blackholes, and potentially by the expansion of the Universe.

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-  Within our own Milky Way, the “ngVLA” will greatly expand our ability to detect blackholes in binary systems, enabling probes of supernova explosions and blackhole formation. It will also enable the detection of less massive blackholes that dwell in the centers of dwarf galaxies throughout the local cluster.

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-  The detection of gravitational waves, along with their direct link to merging compact objects, marks one of the major breakthroughs in astrophysics over the past 10 years. The ngVLA will be able to resolve and observe the motion of mergers of supermassive black holes and neutron stars, both sources of gravitational waves. 

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-  New facilities can detect these merging stellar remnants in galaxies up to 600 million light-years away through the gravitational wave and neutrino events they produce, and the ngVLA will be able to detect the radio emission to the same distance, permitting us to determine the physical conditions at the location of neutrino production.

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-  Even the most supermassive of the supermassive blackholes aren’t very large, making it extremely difficult to measure their sizes. However, astronomers have recently developed a new technique that can estimate the mass of a blackhole based on the movement of hot gas around them even when the blackhole itself it smaller than a single pixel.

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-  Supermassive blackholes are surrounded by tons of superheated plasma. That plasma swirls around the backhole, forming a torus and an accretion disk that continually feeds material into the blackhole. Because of the extreme gravity, that gas moves incredibly quickly and shines fiercely. It’s that light that we identify as a “quasar‘, which can be seen from across the universe.

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-  While the quasars are relatively easy to spot, it’s much more challenging to quantify the properties of the central blackhole. Now, for the first time, in 2021,  Astronomers are demonstrating the feasibility of directly determining the mass of a quasar using a technique called spectroastrometry.

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-  “Spectroastrometry’ relies on observing the area around the blackhole. As the gas swirls around it, some of it will be moving in our direction and some if it will be moving away. The portion of the gas moving towards us will be blue-shifted, and the portion moving away will shift more red.

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-   Even if the central blackhole and accretion disk are too small to resolve, this technique can still be applied to regions further away, and through modeling the researchers can estimate a mass.

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-  By separating spectral and spatial information in the collected light, as well as by statistically modeling the measured data, astronomers can derive distances of much less than one image pixel from the center of the accretion disk.

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-  This technique was applied to “J2123-0050“, a quasar active when the universe was just 2.9 billion years old. They found that the central black hole weighed 1.8 billion solar masses.

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-  With the significantly increased sensitivity of the James Webb Space Telescope (JWST) and the Extremely Large Telescope (ELT), with a primary mirror diameter of 39 meters, currently under construction, we will soon be able to determine quasar masses at the highest redshifts

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November 29, 2021    GALAXIES  -  beyond were light can see?       3363                                                                                                                                                  

----------------------------------------------------------------------------------------

-----  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”  -----------

--------------------- ---  Tuesday, November 30, 2021  ---------------------------






3362 - EARTH’S - magnetic core is moving?

  -  3362   - EARTH’S  -  magnetic core is moving?  Though the Earth’s magnetic field is very similar to that of a bar magnet, with a north and south pole, it is not as stable because it is generated by complex processes inside the Earth. These cause the magnetic poles to wander.


---------------------  3362  -  EARTH’S  -  magnetic core is moving?

-   Magnetic fields are generated by electric charges in motion. In a bar magnet, the moving charges are electrons orbiting in atoms. In the Earth, they are electrons in circulating currents of molten iron.

-

-   Hot material in Earth’s outer liquid iron core expands, becoming less dense than its surroundings, and therefore rises. Cooling and becoming less dense, it should sink back down again. But, the Earth’s rotation prevents this.

-

-  Consequently, liquid circulates around the core, and friction between its different layers charges them up just like a plastic comb rubbing against a nylon sweater. It’s these moving charges that generate the Earth’s magnetic field.

-

-  The two requirements for planetary magnetism are therefore a liquid core and rotation. We know this because Venus, though roughly Earth’s size, has essentially no magnetic field. The planet has a liquid core but rotates slowly, only once every 243 Earth days.

-

-  Why do Earth’s magnetic poles move?  Though the Earth’s magnetic field is very similar to that of a bar magnet, with a north and south pole, it is not as stable because it is generated by complex processes inside the Earth. These cause the magnetic poles to wander.

-

-  Historically, the North Pole has moved at about 15 kilometers per year. But since the 1990s it has sped up, and now is moving at about 55 kilometers per year towards Siberia. It is speculation, but this might foreshadow a ‘magnetic reversal’ in which the magnetic north and south poles change locations. This has happened 171 times in the past 71 million years, and, we are overdue for a flip.

-

-  Models of the Earth’s magnetic field based on satellite observations have shown that the present wandering is the result of a battle between ‘blobs’ of unusually intense magnetic fields deep inside the planet.

-

-  What would happen if the magnetic field disappeared?  Scientists discovered magnetic reversals by measuring the magnetic field on either side of mid-Atlantic ridges from which molten rock is extruded like toothpaste from a tube. As it solidifies, its crystals align along the direction of the Earth’s magnetic field at the time, leaving a ‘tape recording’ of reversals.

-

-  Reversals are believed to take place over 1,000 to 10,000 years, during which time the field shrinks to zero before growing again with the opposite polarity. There were therefore times, maybe even centuries, when the Earth had essentially no magnetic field.

-

-  This is dangerous for life since the planet’s magnetic field extends far into space and creates a protective bubble around Earth, shielding the planet’s surface from the hurricane of particles of the Sun’s ‘solar wind’ and higher energy ‘cosmic ray’ particles from deep space.

-

-  Normally, these particles are safely funneled down at the poles, creating the “auroras“ (Northern Lights ). Without a protective field, such deadly radiation would increase the mutation rate of living cells, leading to cancers in animals. Nevertheless, life has weathered large numbers of such events before without being wiped out.

-

-  How stable is Earth’s magnetic field?  The fact that the Earth’s magnetic field depends on electric currents carried by molten material circulating in the planet’s turbulent interior means it is inherently variable, as demonstrated by the present wandering of the magnetic north pole (the magnetic south pole is, surprisingly, not wandering as fast).

-

-  What is remarkable is that the magnetic field generated by such violent internal convulsions is relatively stable 99.9 per cent of the time. It is the stability of the Earth’s magnetic field, and the reliability of the protection it has provided, that has enabled life on Earth to persist for almost at least 3.8 billion years.

-

-  How do animals use the magnetic field to navigate?  Many creatures demonstrate remarkable feats of navigation. The suspicion has therefore arisen that they have some kind of magnetic sense, enabling them to detect the magnetic field lines between the poles. Pinpointing the mechanism, however, has proved difficult. But progress has been made in 2021 by Japanese scientists investigating a process discovered many years ago.

-

-  In the 1970s scientists observed single-celled organisms streaming in a fixed direction in a muddy pond and showed they were responding to a magnetic field. Biologists later discovered that such single-celled organisms contain tiny bags of magnetic iron oxide or iron sulphide.

-

-  They have shown that a magnetic field causes chemical changes that can affect cellular behavior. They achieved this with the aid of a cellular chemical that fluoresces depending on the external magnetic field. When they waved a magnet near cells, the chemical dimmed by up to 3.5 per cent.

-

-   From the study of seismology which is the measurements of sound waves traveling through Earth  we can tell that the core is molten. Plus, from our knowledge of the abundance of elements in the Universe and how they behave, we think it’s made mainly of iron under huge amounts of pressure.

-

-  All this indicates its temperature is about 6,000°C, similar to the temperature of the Sun’s surface. And Earth’s core is only 3,000 kilometers from its surface.  So why doesn’t Earth’s core fry us all?   Because the core is surrounded by a mostly solid mantle of rock.

-

-  The crust we live on floats on that mantle, giving us more protection. But the most important reason we don’t all melt is the difference between heat and temperature. Roughly speaking, heat is energy and temperature is density of energy, basically how much energy is crammed into a given size.

-

-  A spark from a sparkler can have a temperature of 1,500°C, but won’t really hurt you. On the other hand, a bath of boiling water at only 100°C would kill you. That’s because the bath contains much more heat energy.

-

-  To melt the whole Earth, you would need much more energy than the heat in its core. The Sun is huge and could easily do that,  but,  luckily it’s 150,000,000 kilometers away.

-

-  The Earth’s axis isn’t perfectly upright relative to its orbit, but instead is tilted at an angle of around 23.5°. This so-called obliquity has long been known to change slightly over thousands of years as a result of the gravitational influence of the Sun, the Moon and the other planets. 

-

-  But evidence is also emerging for effects resulting from climate change.  In 2013, researchers reported that satellite measurements had revealed that the Earth’s tilt is being affected by the shift in mass caused by the melting of ice covering Greenland.

-

-   The team found that around 15 years ago the Earth’s axis began to move east and then south. Earlier this year, researchers confirmed the effect, and added another cause: changes in the amount of water stored in the Earth’s continents. Lower rainfall over Europe and Asia in recent years seems to be adding to the axial drift.

-

-  So is man-made global warming to blame for these changes?  It’s probably just part of the Earth’s natural climatic rhythms. Either way, the effect isn’t anything to lose sleep over: the recent shift amounts to less than one-millionth of the Earth’s total tilt angle.

-

-  You probably would not notice this tilt or axial drift.   You would get more of this effect drinking too much alcohol.

-

November 29, 2021    EARTH’S  -  magnetic core is moving?        3362                                                                                                                                                  

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--------------------- ---  Tuesday, November 30, 2021  ---------------------------






3361 - MILKY WAY GALAXY

  -  3361  -   MILKY WAY  GALAXY    -   Our galaxy is an awe-inspiring place full of stars, supernovas, nebulas, energy and dark matter, but many aspects of it remain mysterious, even to scientists.  Before the advent of electric lights, everybody on Earth had an unobstructed view of the night sky. The enormous milky band of stars crossing it was impossible to miss.  It was our Milky Way Galaxy.


---------------------  3361  -   MILKY WAY  GALAXY  

-   Ancient peoples gave different names to the cloud-like structure of our galaxy, but our modern version derives from the Greeks, who had a myth about the infant Hercules being brought to the goddess Hera, who nursed him while she was asleep. When she awoke and pulled away, her breast milk spilled across the heavens. 

-

-  The source of the Greek name itself has been lost to the ages.  We're not sure exactly how many stars are in the Milky Way.  Counting stars is a tedious business. Even astronomers argue over the best way to do it. 

-

-  Their telescopes see only the brightest stars in our galaxy, and many are hidden by obscuring gas and dust. One technique to estimate the stellar population of the Milky Way is to look at how fast stars are orbiting within it, which gives an indication of the gravitational tug, and therefore the mass, of the galaxy.

-

-  Divide the galactic mass by the average size of a star and you should have your answer.  Stars vary widely in size, and many assumptions go into estimating the number of stars residing in the Milky Way. 

-

-  The European Space Agency's Gaia satellite has mapped the location of 1,000,000,000 stars in our galaxy, and its scientists believe this represents 1 percent of the total, so perhaps the Milky Way contains about 100 billion stars. 

-

-  Astronomers are also unsure exactly how much our galaxy weighs, with estimates ranging from 700 billion to 2 trillion times the mass of our sun. Most of the Milky Way's mass, perhaps 85 percent, is in the form of “dark matter“, which gives off no light and so is impossible to directly observe.

-

-   A 2020 study looked at how strongly our galaxy's humongous mass gravitationally tugs on smaller galaxies orbiting it and updated the estimate of the Milky Way's mass to 960,000,000,000 times the mass of the sun.

-

-  Several studies have indicated that the Milky Way and its neighbors are living out in a big empty spot in the universe.. From afar, the large-scale structure of the universe looks like a colossal cosmic web, with string-like filaments connecting dense regions separated by enormous, mostly empty voids. 

-

- Our galaxy seems to be an inhabitant of the Keenan, Barger and Cowie (KBC) Void, named after three astronomers who identified it in a 2013. Last year, 2020, a separate team looked at the motion of galaxies in the cosmic web to provide additional confirmation that we're floating in one of the big, empty areas.

-

-  Lurking in the heart of our galaxy is a hungry behemoth, a gigantic blackhole with the weight of 4,000,000 suns. Scientists know that it's there because they can trace the paths of stars in the Milky Way's center and see that they seem to orbit a supermassive object that can't be seen.

-

-   Astronomers have been combining observations from multiple radio telescopes to try and get a glimpse of the environment surrounding the blackhole, which is packed with gas and dust spinning around the blackhole's maw. The project, called the Event Horizon Telescope, expects to have preliminary images of the blackhole's edge.

-

-   When Portuguese explorer Ferdinand Magellan sailed through the Southern Hemisphere in the 16th century, he and his crew were among the first Europeans to report on circular clusters of stars in the night sky, according to the European Southern Observatory. 

-

-  These clusters are actually small galaxies that orbit our Milky Way like planets around a star, and they have been named the Small and Large Magellanic clouds. Many such dwarf galaxies orbit ours and sometimes they get eaten by our massive Milky Way. 

-

-  Earlier this year, astronomers used new data from the Gaia satellite that showed millions of stars in our galaxy moving in similar narrow, "needle-like" orbits, suggesting they all originated from an earlier dwarf galaxy dubbed "the Gaia Sausage".

-

-  Swirling through the mostly empty space between stars in our galaxy is a bunch of dirty grease. Oily organic molecules known as ‘aliphatic carbon compounds” are produced in certain types of stars and then are leaked out into interstellar space. 

-

-  These grease-like substances could account for between a quarter and one-half of the Milky Way's interstellar carbon .   Carbon is an essential building block of living things, finding it in abundance throughout the galaxy could suggest that other star systems harbor life.

-

-   The Milky Way is going to crash with its neighbor in 4 billion years.  Our galaxy isn't going to be here forever. Astronomers know that we are currently speeding toward our neighbor, the Andromeda galaxy, at around 250,000 mph . 

-

-  When the crash comes, in about 4 billion years, most research has suggested that the more massive Andromeda galaxy would swallow up our own and survive. But in a recent study, astronomers reweighed Andromeda and found that it was roughly equivalent to 800 billion suns, or about on par with the Milky Way's mass. That means that exactly which galaxy will emerge less scathed from the future galactic crash remains an open question.

-

-  Stars from our galactic neighbors are racing toward the Milky Way.  Researchers were recently searching for hypervelocity stars, which get thrown at mind-bending speeds from the Milky Way after interacting with the giant blackhole in its center.

-

-   What they found was even stranger.  Rather than flying away from our galaxy, most of the fast stars they spotted were barreling toward us.  These could be stars from another galaxy, zooming right through the Milky Way.  

-

-   These odd stars could have originated in the Large Magellanic Cloud or some other galaxy farther away. They may constitute the tip of the iceberg of a large population of similar stars.

-

-  Scientists in 2010 uncovered gigantic, never-before-seen structures stretching for 25,000 light-years above and below the galaxy. Named 'Fermi bubbles' after the telescope that found them, these gamma-ray-emitting objects have defied astronomers' explanations ever since.

-

-   In 2020 a team gathered evidence suggesting that the bubbles are the aftermath of an energetic event 6 million to 9 million years ago, when the supermassive blackhole in the galactic center swallowed a huge clump of gas and dust and burped out the giant, glowing clouds.

-

-  Over the last decade, astronomers keep detecting odd flashes of light coming at them from the distant cosmos. Known as “fast radio bursts” (FRBs), these mysterious signals have no agreed-upon explanation. 

-

-  Despite knowing about them for more than 10 years, researchers had until recently captured only 30 or so examples of these FRBs. But in a recent study, Australian scientists managed to find 20 more FRBs, nearly doubling the number of known objects.

-

-   While they still don't know the odd flashes' origin, the team was able to determine that the light had traveled through several billion light-years of gas and dust, which imparted telltale signs on the signal, suggesting that the FRBs were coming from quite a long way off.

-

-    Astronomers have found that a white dwarf is pummeling a companion object, either a lightweight star or a planet, with incessant blasts of heat and radiation plus a relentless gravitational pull tearing it apart.

-

-  Most stars, including the Sun, will become "white dwarfs" after they begin to run out of fuel, expand and cool into a red giant, and then lose their outer layers. This evolution leaves behind a stellar nub that slowly fades for billions of years.

-

- Typically, white dwarfs give off low-energy X-rays, which researchers saw in their sample. However, these white dwarfs also had surprisingly bright X-ray emission at higher energies.  See Review 3339 to learn more abut these white dwarf stars.

-

-  Astronomy gives us so much more to learn.  The fact that we know that is even more amazing.

-

November 28, 2021          MILKY WAY  GALAXY               3361                                                                                                                                                  

----------------------------------------------------------------------------------------

-----  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”  -----------

--------------------- ---  Tuesday, November 30, 2021  ---------------------------






3359 - WHITE DWARF - stars with perplexing behavior?

  -  3359   -   WHITE  DWARF  -  stars with perplexing behavior?  A white dwarf star that completes a full rotation once every 25 seconds is the fastest spinning confirmed white dwarf.  It as an extremely rare  “magnetic propeller system”. The white dwarf is pulling gaseous plasma from a nearby companion star and flinging it into space at around 3,000 kilometers per second.

-

---------------  Merging white dwarfs create gravity waves

---------------  3359  -     WHITE  DWARF  -  stars with perplexing behavior?

-  Astronomers have found that a white dwarf is pummeling a companion object, either a lightweight star or a planet, with incessant blasts of heat and radiation plus a relentless gravitational pull tearing it apart.

-

-  Most stars, including our Sun, will become "white dwarfs" after they begin to run out of fuel, expand and cool into a ‘red giant star“, and then lose their outer layers. This evolution leaves behind a stellar nub that slowly fades for billions of years.

-

-  Typically, white dwarfs give off low-energy X-rays. However, these particular white dwarfs had surprisingly bright X-ray emission at higher energies.  The white dwarf “KPD 0005+5106 “ had high-energy X-ray emission that was regularly increasing and decreasing in brightness every 4 hours and 42 minutes. 

-

-  This recurring ebb and flow of X-rays indicates that this star has an object in orbit around it, either a very low-mass star or a planet.

-

-  Material from this low-mass star or planet could be slamming into the north and south poles of the white dwarf, creating a bright spot of high-energy X-ray emission. As the white dwarf and its companion orbit around each other this hot spot would go in and out of view, causing the high-energy X-rays to regularly increase and decrease.

-

-  Looking for this companion with optical light telescopes haven't seen anything, which means it is a very dim star, a brown dwarf, or a planet.

-

-  This star located in our galaxy about 1,300 light-years from Earth, is one of the hottest known white dwarf stars, with a surface temperature of about 360,000 degrees Fahrenheit. By comparison, the surface of the Sun is about 10,000 degrees Fahrenheit.

-

-  The companion object is about 500,000 miles away from the white dwarf, about one thirtieth of the distance from Mercury to the Sun.

-

- The researchers looked at what would happen if this object was a planet with the mass about equal to Jupiter, a possibility that agrees with the data more readily than a dim star or a brown dwarf.

-

-   In these models, the white dwarf would pull material from the planet onto the white dwarf, a process that the planet could only survive for a few hundred million years before eventually being destroyed. This stolen material swirls around the white dwarf, which glows in X-rays that Chandra can detect.   This object that is basically being ripped apart by constant gravitational forces.

-

-  The two other white dwarfs were also thought to be solitary objects, but they show similar energetic X-ray emission to KPD 0005+5106. By analogy, this suggests they may also have faint companions, possibly planets.

-

-  A white dwarf star that completes a full rotation once every 25 seconds is the fastest spinning confirmed white dwarf.  It as an extremely rare  “magnetic propeller system”. The white dwarf is pulling gaseous plasma from a nearby companion star and flinging it into space at around 3,000 kilometers per second.

-

-  It is only the second magnetic propeller white dwarf to have been identified in over 70 years.  A white dwarf is a star that has burnt up all of its fuel and shed its outer layers, now undergoing a process of shrinking and cooling over millions of years.

-

-   The star is the size of the Earth but is thought to be at least 200,000 times more massive. It is part of a binary star system and its immense gravity is pulling material from its larger companion star in the form of plasma.

-

-   This plasma was falling onto the white dwarf's equator at high speed, providing the energy that has given it this fast spin. One rotation of the planet Earth takes 24 hours, while the equivalent on J0240+1952 is a mere 25 seconds. That's almost 20 percent faster than the confirmed white dwarf with the most comparable spin rate, which completes a rotation in just over 29 seconds.

-

-   At some point in its evolutionary history this star developed a strong magnetic field. The magnetic field acts as a protective barrier, causing most of the falling plasma to be propelled away from the white dwarf. 

-

-  The remainder will flow towards the star's magnetic poles. It gathers in bright spots on the surface of the star and as these rotate in and out of view they cause pulsations in the light that the astronomers observe from Earth, which they then used to measure the rotation of the entire star.

-

-  It is pulling material from its companion star due to its gravitational effect, but as that gets closer to the white dwarf the magnetic field starts to dominate. This type of gas is highly conducting and picks up a lot of speed from this process, which propels it away from the star and out into space.

-

-   Astronomers have found that a white dwarf is pummeling a companion object, either a lightweight star or a planet, with incessant blasts of heat and radiation plus a relentless gravitational pull tearing it apart.

-

-  Most stars, including the Sun, will become "white dwarfs" after they begin to run out of fuel, expand and cool into a red giant, and then lose their outer layers. This evolution leaves behind a stellar core that slowly fades for billions of years.

-

-   The white dwarf “KPD 0005+5106” had high-energy X-ray emission that was regularly increasing and decreasing in brightness every 4.7 hours. This recurring ebb and flow of X-rays indicates that the star has an object in orbit around it, either a very low-mass star or a planet.

-

-  Material from the low-mass star or planet could be slamming into the north and south poles of the white dwarf, creating a bright spot of high-energy X-ray emission. As the white dwarf and its companion orbit around each other this hot spot would go in and out of view, causing the high-energy X-rays to regularly increase and decrease.

-

-  This star is located in our galaxy about 1,300 light-years from Earth.  It is one of the hottest known white dwarf stars, with a surface temperature of about 360,000 degrees Fahrenheit. By comparison, the surface of the Sun is about 10,000 degrees Fahrenheit.

-

-  This companion object is about 500,000 miles away from the white dwarf, only about one thirtieth of the distance from Mercury to the Sun.

-

-  The researchers looked at what would happen if this object was a planet with the mass about that of Jupiter, a possibility that agrees with the data more readily than a dim star or a brown dwarf. In their models, the white dwarf would pull material from the planet onto the white dwarf, a process that the planet could only survive for a few hundred million years before eventually being destroyed. This stolen material swirls around the white dwarf, which glows in X-rays that Chandra can detect.

-

-  The two other white dwarfs were also thought to be solitary objects, but they show similar energetic X-ray emission. This suggests they may also have faint companions, possibly planets.

-

-  Microlensing  involves looking for the magnification and bending of light from distant sources around intervening objects. Microlensing has shown that a planet can survive the evolution of a white dwarf through its red giant phase.

-

-  Scientists will need to do more theoretical modeling of the evolution of double stars to understand how the planet or low-mass star might end up so close to the white dwarf.

-

-  Another white dwarf star completes a full rotation once every 25 seconds is the fastest spinning confirmed white dwarf.  The spin period of the star confirms it as an extremely rare example of a magnetic propeller system: the white dwarf is pulling gaseous plasma from a nearby companion star and flinging it into space at around 3,000 kilometers per second ( 2,237 miles per our).   It is only the second magnetic propeller white dwarf to have been identified in over 70 years.

-

-  A white dwarf is a star that has burnt up all of its fuel and shed its outer layers, now undergoing a process of shrinking and cooling over millions of years. Another one is the size of the Earth but is thought to be at least 200,000 times more massive. It is part of a binary star system and its immense gravity is pulling material from its larger companion star in the form of plasma.

-

-   This plasma was falling onto the white dwarf's equator at high speed, providing the energy that has given it this fast spin. One rotation of the planet Earth takes 24 hours, while the equivalent on  “J0240+1952” is a 25 seconds. 

-

-  That's almost 20 percent faster than the confirmed white dwarf with the most comparable spin rate, which completes a rotation in just over 29 seconds.

-

-   At some point in its evolutionary history J0240+1952 developed a strong magnetic field. The magnetic field acts as a protective barrier, causing most of the falling plasma to be propelled away from the white dwarf. 

-

-  The remainder will flow towards the star's magnetic poles. It gathers in bright spots on the surface of the star and as these rotate in and out of view they cause pulsations in the light that the astronomers observe from Earth, which they then used to measure the rotation of the entire star.

-

-   The rotation is so fast that the white dwarf must have an above average mass just to stay together and not be torn apart.  It is pulling material from its companion star due to its gravitational effect, but as that gets closer to the white dwarf the magnetic field starts to dominate. 

-

-  This type of gas is highly conducting and picks up a lot of speed from this process, which propels it away from the star and out into space.  This is one of only two stars with this magnetic propeller system discovered in the past 70 years. 

-

-  Although material being flung out of the star was first observed in 2020, astronomers had not been able to confirm the rapid spin that is a main ingredient of a magnetic propeller, as the pulses are too fast and dim for other telescopes to observe.

-

November 28, 2021    WHITE  DWARF  -  stars with perplexing behavior?    3356                                                                                                                                                  

----------------------------------------------------------------------------------------

-----  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”  -----------

--------------------- ---  Tuesday, November 30, 2021  ---------------------------






Sunday, November 28, 2021

3358 - PHOTONS - have a lot of explaining to do?

  -  3358   -  PHOTONS  -  have a lot of explaining to do?  -  A photon is an elementary particle in physics.  It is the quantum of the electromagnetic field.   And, it is the basic "unit" of light and all other forms of electromagnetic radiation. It is the force carrier for the electromagnetic force. 

-


---------------------  3358  -   PHOTONS  -  have a lot of explaining to do?

-  The effects photon and the electromagnetic force are easily observable at both the microscopic and macroscopic level.   Because the photon has “no rest mass“; this also allows for interactions at long distances. 

-

-  Like all elementary particles, photons are governed by quantum mechanics and will exhibit wave-particle duality.  They exhibit properties of both waves and particles.  A single photon may be refracted by a lens or exhibit wave interference, but also act as a particle giving a definite result when its location is measured.

-

-  The modern concept of the photon was developed gradually by Albert Einstein to explain experimental observations that did not fit the classical wave model of light. The photon model accounted for the frequency dependence of light's energy, and explained the ability of matter and radiation to be in thermal equilibrium. 

-

-  It also accounted for anomalous observations, including the properties of blackbody radiation, that other physicists, most notably Max Planck, had sought to explain using semiclassical models, in which light is still described by Maxwell's equations, but the material objects that emit and absorb light are quantized. 

-

-  Although these semiclassical models contributed to the development of quantum mechanics, further experiments proved Einstein's hypothesis that light itself is quantized; those quanta of light are photons.

-

-  In the modern Standard Model of particle physics, photons are described as a necessary consequence of physical laws having a certain symmetry at every point in spacetime. The intrinsic properties of photons, such as charge, mass and spin, are determined by the properties of this “gauge symmetry“.

-

-  The photon concept has led to momentous advances in experimental and theoretical physics, such as lasers, Bose–Einstein condensation, quantum field theory, and the probabilistic interpretation of quantum mechanics. It has been applied to photochemistry, high-resolution microscopy, and measurements of molecular distances. 

-

-  Recently, photons have been studied as elements of quantum computers and for sophisticated applications in optical communication such as quantum cryptography.

The invention of lasers have greatly advanced our understanding of photons.  Physicists have even used laser photons to deep-freeze antimatter.

-

-  In this antimatter experiment, an ultraviolet laser quelled the thermal jitters of antihydrogen atoms, chilling the antiatoms to just above absolute zero. This technique for slowing down antimatter could help scientists build the first antimatter molecules. 

-

-  Taming unruly antimatter with laser light may also allow physicists to measure the properties of antiatoms much more precisely.  Comparing antiatoms with normal atoms could test some fundamental symmetries of the universe.

-

-  Laser photons can cool atoms by dampening the atoms’ motion with a barrage of light particles, i.e. photons.   To create antihydrogen atoms researchers mixed antiprotons with positrons, the antiparticles of electrons, at the CERN particle physics lab near Geneva.

-

-   Over several hours, a laser beam tuned to a specific frequency of UV light slowed the antihydrogen atoms from whizzing around at up to 90 meters per second to about 10 meters per second.

-

-  Future observations of supercooled antihydrogen could test an idea called “charge-parity-time“, or CPT, symmetry. This physics principle says that normal atoms should absorb and emit photons with the exact same energies as their antimatter look-alikes. 

-

-  Even the tiniest differences between hydrogen and antihydrogen could undermine modern theories of physics.

-

-  Einstein’s theory of gravity predicts that matter and antimatter should fall to Earth at the same rate. Lab experiments dropping laser-cooled antiatoms, instead of warm, jittery ones into free fall could provide a clearer view of gravity’s effects.

-

November 26, 2021   PHOTONS  -  have a lot of explaining to do?     3358                                                                                                                                                  

----------------------------------------------------------------------------------------

-----  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, November 28, 2021  ---------------------------