Saturday, June 8, 2024

4494 - SOLAR STORMS - heading our way?

 

-    4494  -      SOLAR  STORMS  -  heading our way?  -     More solar storms could be heading our way, June 6, 2024.   Auroras may be pretty, but the solar storms that cause them can cause serious havoc on Earth.



-------------------------------------  4494    -    SOLAR  STORMS  -  heading our way?

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-    Tourists normally have to pay big money and brave cold climates for a chance to see an aurora, but on May 10, 2024, many people around the world simply had to look up to see these colorful displays dance across the sky.

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-   Usually banished to the poles of Earth, the auroras strayed as far as Mexico, southern Europe and South Africa on the evening of May 10, delighting skygazers and filling social media with images of exuberant pinks, greens and purples.

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-   But for those charged with protecting Earth from powerful solar storms such as the one that caused the auroras, a threat lurks beneath the stunning colors.  We need to understand that behind this beauty, there is danger.

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-    Potential impacts of solar storms are the taking out power grids and satellites, or exposing astronauts to dangerous levels of radiation.

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-   The latest auroras were caused by the most powerful geomagnetic storm since the "Halloween Storms" of October 2003, which sparked blackouts in Sweden and damaged power infrastructure in South Africa.

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-    There were reports that some self-driving farm tractors in the United States stopped in their tracks when their GPS guidance systems went out due to the storm.

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-    Massive explosions on the surface of the Sun shoot out plasma, radiation and even magnetic fields at incredibly fast speeds born on the solar wind.  These strange effects are caused by massive explosions on the surface of the sun that shoot out plasma, radiation and even magnetic fields at incredibly fast speeds born on the solar wind.

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-   The recent activity has come from a sunspot cluster 17 times the size of Earth which has continued raging over the week.   It blasted out the strongest solar flare seen in years.

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-   The sunspot has been turning towards the edge of the sun's disk, so activity is expected to die down in the short term as its outbursts aim away from our planet.  But in roughly two weeks the sunspot will swing back around, again turning its gaze towards Earth.

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-   It is difficult to predict how violent these sunspots could be, or whether they could spark further auroras.  But solar activity is only just approaching the peak of its roughly 11-year cycle, so the odds of another major storm are highest "between now and the end of next year".

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-    Geomagnetic storms such as the recent one create a magnetic charge of voltage and current, "essentially overloading" things like satellites and power grids.   The most famous example came in 1859 during the worst solar storm in recorded history, called the “Carrington Event”.

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-   As well as stunning auroras, the storm caused sparks to fly off of telegraph stations. The charge that originated from the sun was so strong that some telegraphs worked without being plugged into a power source.

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-   So what would happen if such a powerful geomagnetic storm struck Earth again?    Most countries have improved their power grids, which should prevent prolonged outages like those that hit Sweden in 2003 or Canada in 1989.

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-  Still suggested is that people have an emergency kit in case electricity is knocked out for a day or two. Fresh water might also help in case filtration plants go offline.

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-   Astronauts are particularly at risk from radiation during extreme solar activity. Those on the International Space Station usually take the best shelter they can when a bad storm is expected.

 

Bettwy said a massive solar storm could expose astronauts to an "unhealthy dose" of radiation, but he did not think it would be lethal.  Emphasizing radiation can also potentially "get through the fuselage" of planes flying near the north pole.

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-    Airlines sometimes change routes during extreme solar storms to avoid this happening.

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-    Several upcoming space missions are expected to improve forecasting of the sun's intense and unpredictable weather, aiming to give Earth more time to prepare.

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June 2, 2024         SOLAR  STORMS  -  heading our way?                     4494

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

--------  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”  -----------

--------------------- ---  Friday, June 7, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Friday, June 7, 2024

4493 - SUPERNOVAE EXPLOSIONS - produce the heavier elements?

 

-    4493  -   SUPERNOVAE  EXPLOSIONS  -   produce the heavier elements?  -    A recent study investigated one long gamma ray burst in particular, GRB 221009. This has been dubbed the BOAT, “the brightest of all time”. This GRB was picked up as a pulse of intense radiation sweeping through the solar system on October 9, 2022.


------------------------  4493    -   SUPERNOVAE  EXPLOSIONS  -   produce the heavier elements?

-    After its "birth" in the Big Bang, the “universe” consisted mainly of hydrogen and a few helium atoms. These are the lightest elements in the periodic table. More-or-less all elements heavier than helium were produced in the 13.8 billion years between the Big Bang and the present day.

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-    Stars have produced many of these heavier elements through the process of nuclear fusion. However, this process only makes elements as heavy as iron. The creation of any heavier elements would consume energy instead of releasing it.

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-   In order to explain the presence of these heavier elements today, it's necessary to find phenomena that can produce them. One type of event that fits the bill is a gamma-ray burst (GRB)which are the most powerful class of explosion in the universe. These can erupt at a quintillion (10 followed by 18 zeros) times the luminosity of our sun, and are thought to be caused by several types of events.

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-    GRBs can be subdivided into two categories: long bursts and short bursts. Long GRBs are associated with the deaths of massive and fast-rotating stars. According to this theory, the fast rotation beams material ejected during the collapse of a massive star into narrow jets that move at extremely fast speeds.

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-   The short bursts last only a few seconds. They are thought to be caused by the collision of two neutron stars which are compact and dense "dead" stars. In August, 2017, an important event helped support this theory. Ligo and Virgo, two gravitational wave detectors in the US, discovered a signal that seemed to be coming from two neutron stars moving in for a collision.

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-   A few seconds later, a short gamma-ray burst, known as “GRB 100817A”, was detected coming from the same direction in the sky. For a few weeks, virtually every telescope on the planet was pointing at this event in an unprecedented effort to study its aftermath.

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-    The observations revealed a kilonova at the location of GRB 170817A. A “kilonova” is a fainter cousin of a supernova explosion. More interestingly, there was evidence that many heavy elements were produced during the explosion. This kilonova seemed to produce two different categories of debris, or ejecta. One was composed primarily of light elements, while another consisted of heavy elements.

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-    Nuclear fusion can only feasibly produce elements as heavy as iron in the periodic table. But there's another process which could explain how the kilonova was able to produce even heavier ones.  Rapid neutron-capture process, or r-process, is where the nuclei (or cores) of heavier elements such as iron capture many neutron particles in a short time.

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-    The kilonova can then rapidly grow in mass, yielding much heavier elements. For r-process to work, however, you need the right conditions: high density, high temperature, and a large number of available free neutrons. Gamma ray bursts happen to provide these necessary conditions.

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-   However, mergers of two neutron stars, like the one that caused the kilonova GRB 170817A, are very rare events. In fact, they may be so rare as to make them an unlikely source for the abundant heavy elements we have in the universe. But what of long GRBs?

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-   The “BOAT” sparked a similar astronomical observation campaign as the kilonova. This GRB was 10 times more energetic than the previous record holder, and so close to us that its influence on the Earth's atmosphere was measurable on the ground and comparable to a major solar storm.

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-   Among the telescopes studying the aftermath of the BOAT was the James Webb Space Telescope (JWST). It observed the GRB about six months after it exploded, so as not to be blinded by the afterglow of the initial burst. The data JWST collected showed that, despite the event's extraordinary brightness, it was caused by a merely average supernova explosion.

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-    Previous observations of other long GRBs indicated that there is no correlation between the brightness of the GRB and the size of the supernova explosion associated with it. The BOAT seems no exception.

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-    The JWST team also inferred the number of heavy elements produced during the BOAT explosion. They found no indication of elements produced by the r-process. This is surprising as, theoretically, the brightness of a long GRB is thought to be associated with the conditions in its core, most likely a black hole. For very bright events, especially one as extreme as the BOAT, the conditions should be right for the r-process to occur.

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-   These findings suggest that gamma ray bursts may not be the hoped-for crucial source of the universe's heavy elements. Instead, there must be a source or sources still out there.

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June 6, 2024      SUPERNOVAE  EXPLOSIONS  -   produce the heavier elements?       4493

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

--------  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”  -----------

--------------------- ---  Friday, June 7, 2024  ---------------------------------

 

 

 

 

 

           

 

 

4491 - WEBB TELESCOPE - new discoveries?

 

-   4491  -   WEBB  TELESCOPE  -  new discoveries?   -    How did the first stars and galaxies form? NASA's James Webb Space Telescope is already providing new insights into this question. One of the largest programs in Webb's first year of science is the JWST Advanced Deep Extragalactic Survey, or JADES, which will devote about 32 days of telescope time to uncover and characterize faint, distant galaxies.


-------------------------------------  4491   -  WEBB  TELESCOPE  -  new discoveries? 

-     JADES already has discovered hundreds of galaxies that existed when the universe was less than 600 million years old. The team also has identified galaxies sparkling with a multitude of young, hot stars.

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-     How did the earliest galaxies assemble themselves? How fast did they form stars? Why do some galaxies stop forming stars?.

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-    Galaxies that existed 500 to 850 million years after the Big Bang was during a crucial time known as the “Epoch of Reionization”. 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.

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-     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 this reionization.

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-    Almost every single galaxy that they find 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 univers, 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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-   The gold standard for 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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-   These “photometric redshifts” identified more than 700 candidate galaxies that 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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-    Previously, the earliest galaxies we could see just looked like little smudges. And yet those smudges represent millions or even billions of stars at the beginning of the universe.   Now, we can see that some of them are actually extended objects with visible structure. We can see groupings of stars being born only a few hundred million years after the beginning of time.

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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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-   The Webb telescope has unleashed a torrent of scientific discovery since becoming operational last year, peering farther than ever before into the universe's distant reaches, looking back in time.  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.

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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.   These 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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-    That is the greatest distance ever observed by astronomers.    The Webb telescope also 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.

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-   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.  But the galaxies are "very active in star formation in proportion to their mass.  Those stars were forming at around the same rate as the Milky Way.

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-    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 in February, 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.   If confirmed, the standard model could need updating.

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June 7, 2024          WEBB  TELESCOPE  -  new discoveries?                     4491

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

--------  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”  -----------

--------------------- ---  Friday, June 7, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Monday, June 3, 2024

4490 - BLACKHOLE DISCOVERIES?

 

-    4490  -   BLACKHOLE   DISCOVERIES?  -  Latest astronomy  reveals magnetic fields around Our Galaxy’s giant Black Hole.  The “Event Horizon Telescope” traces the lines of powerful magnetic fields spiraling out from the edge of the supermassive black hole at the center of our Milky Way galaxy, and suggests that strong magnetism may be common to all supermassive black holes.


----------------------------------------  4490    -    BLACKHOLE   DISCOVERIES?

-   The black hole known as Sagittarius A*, which is about 27,000 light-years from Earth, observed using radio-wave observations from the Event Horizon Telescope’s network of observatories around the world.

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-    Sagittarius A* wasn’t the first black hole whose shadow was imaged by the EHT.   In 2019, astronomers showed off a similar picture of the supermassive black hole at the center of the galaxy M87, which is more than a thousand times bigger and farther away than the Milky Way’s black hole.

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-    In 2021, the EHT team charted the magnetic field lines around M87’s black hole by taking a close look at the black hole in polarized light, which reflects the patterns of particles whirling around  magnetic field lines. Researchers used the same technique to determine the magnetic signature of Sagittarius A*, or Sgr A*.

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-     The resulting picture is that there are strong, twisted and organized magnetic fields near the black hole at the center of the Milky Way galaxy.   Along with Sgr A* having a strikingly similar polarization structure to that seen in the much larger and more powerful M87* black hole, we’ve learned that strong and ordered magnetic fields are critical to how black holes interact with the gas and matter around them.

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-   The structure of the magnetic fields around Sgr A* suggests that the black hole is launching a jet of material into the surrounding environment. Previous research has shown that to be the case for M87’s black hole.

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-   A computer simulation of the disk of plasma around M87’s supermassive black hole shows how magnetic fields help launch jets of matter at near the speed of light.   The Milky Way’s black hole appears to be doing something similar.

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-    The fact that the magnetic field structure of M87* is so similar to that of Sgr A* is significant because it suggests that the physical processes that govern how a black hole feeds and launches a jet might be universal among supermassive black holes, despite differences in mass, size and surrounding environment.

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-    In the seven years since the EHT began gathering observations, the collaboration has been adding to its array of radio telescopes, which is resulting in the production of higher-quality imagery.

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-    Gravity is the oldest known, but the least understood force in nature.  For students of gravity, black holes are amongst the most interesting objects to study because gravity is the dominant force there, it is infinitely strong!   Black holes is that they are very ‘simple’ especially when compared to stars and other astrophysical objects. This is a consequence of the so-called ‘no hair’ theorem that states that black holes can be fully characterized by only 3 attributes — their mass, charge and spin.

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-    Black holes are known for exhibiting gravity so strong that light can’t even escape, and while Albert Einstein’s theory of general relativity in 1915 is often credited with first proposing the concept of black holes, the concept of an object whose size and gravity would not allow light to escape was first proposed in a November 1784 letter by English philosopher and clergyman, John Mitchell.

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-     In this letter, Mitchell referred to these objects as “dark stars” since he postulated that stars whose diameters exceeded 500 times that of our Sun’s diameter would trigger the formation of these objects. Additionally, he suggested that gravitational waves influencing nearby celestial bodies would enable these objects to be detected.

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-    Einstein’s theory of general relativity, which also predicted both the existence of black holes and gravitational waves, both of which continued to be scrutinized throughout the 20th century, which includes what’s called the “golden age of general relativity” during the 1960s and 1970s. -

-    This includes the first object accepted by the scientific community as a black hole, called Cygnus X-1, which was discovered in 1964. However, it took another 52 years for the existence of gravitational waves to be confirmed through a black hole merger, which was accomplished by the LIGO Scientific Collaboration.

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-    To develop a complete understanding of the quantum nature of gravity, black holes are the key to unlocking that mystery.    Black holes can only be observed indirectly. Unlike stars, since they don’t emit radiation themselves, it is difficult for astronomers to collect data on them. At best, we can observe their influence on their environment (like gas, stars, etc.) and infer their properties and behavior.

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-    While it took over 100 years between Einstein introducing his theory of general relativity in 1915 and the confirmation of gravitational waves in 2016, it only took another three years for astronomers to publish the first direct image of a black hole at the center of the Messier 87 galaxy.

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-    While Messier 87 is located approximately 53 million light-years from Earth, the closest hypothesized black hole, Gaia BH1, is located approximately 1,560 light-years from Earth. In 2022, astronomers published a direct image of Sagittarius A*, which is the supermassive black hole at the center of our Milky Way Galaxy.

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-    Scientists have hypothesize the number of black holes in our Milky Way Galaxy is in the hundreds of millions, despite only a few dozen known black holes having been confirmed, thus far.

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-     Black holes are studied by astronomers, who use a combination of theory and observations to construct what black holes might look like, and in rare cases, obtain direct images of them.  It is important to note that these direct images  capture the gases that are encircling the black hole’s “event horizon”.  

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-    In recent years, computer simulations have advanced rapidly, and one can now make major discoveries about deep questions using computational tools. In the long run, computer programming would be a very promising tool for advancing research in this field.

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-   Sagittarius A* wasn’t the first black hole whose shadow was imaged by the EHT. Back in 2019, astronomers showed off a similar picture of the supermassive black hole at the center of the galaxy M87, which is more than a thousand times bigger and farther away than the Milky Way’s black

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-   The structure of the magnetic fields around Sgr A* suggests that the black hole is launching a jet of material into the surrounding environment. Previous research has shown that to be the case for M87’s black hole.

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May 22, 2024                      BLACKHOLE   DISCOVERIES?            4490 --------------------------------------------------------------------------------------------                                                                                                                       --------  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 3, 2024  ---------------------------------

 

 

 

 

 

           

 

 

Saturday, June 1, 2024

- 4488 - RARE EARTH METALS - how did they get here?

 

-    4488  -     RARE  EARTH  METALS  -  how did they get here?  -   Before exploding, this star puffed out a sun's worth of mass.  This supernova could prove to be a lynchpin in our understanding of massive star deaths.   The massive star, in the final year or so of its life, ejected large amounts of matter into space before going supernova.

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------------------------  4488    -    RARE  EARTH  METALS  -  how did they get here?

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-  This supernova  exploded in the Pinwheel Galaxy in May, 2024, and it appears to have unexpectedly lost approximately one sun's worth of ejected mass during the final years of its life before going supernova. This new discovery reveals more about the mysterious end days of massive stars.

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-   This star had exploded in the nearby Pinwheel Galaxy (Messier 101), which is just 20 million light-years away in the constellation of Ursa Major, the Great Bear.   That's pretty close.

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-   Amateur astronomers around the world started gazing at “SN 2023ixf” because the Pinwheel in general is a popular galaxy to observe. Haste is key when it comes to supernova observations: Astronomers are keen to understand exactly what is happening in the moments immediately after a star goes supernova. Yet all too often, a supernova is spotted several days after the explosion took place, so they don’t get to see its earliest stages.

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-   The race to decode a supernova began measuring the supernova's light spectrum, and how that light changed over the coming days and weeks. When plotted on a graph, this kind of data forms a "light curve."  The spectrum from “SN 2023ixf” showed that it was a type II supernova.

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-    This is a category of supernova explosion involving a star with more than eight times the mass of the sun.    Archival images of the Pinwheel suggested the exploded star  may have had a mass between 8 and 10 times that of our sun. The spectrum was also very red, indicating the presence of lots of dust near the supernova that absorbed bluer wavelengths but let redder wavelengths pass. 

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-    Normally, a type II supernova experiences what astronomers call a 'shock breakout' very early in the supernova's evolution, as the blast wave expands outwards from the interior of the star and breaks through the star's surface. Yet a bump in the light curve from the usual flash of light stemming from this shock breakout was missing. It  didn’t turn up for several days. Was this a supernova in slow motion?

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-    The delayed shock breakout is direct evidence for the presence of dense material from recent mass loss.    Observations revealed a significant and unexpected amount of mass loss, close to the mass of the sun, in the final year prior to explosion.

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-    An unstable star puffing off huge amounts of material from its surface creates a dusty cloud of ejected stellar material all around the doomed star. The supernova shock wave therefore not only has to break out through the star, blowing it apart, but also has to pass through all this ejected material before it becomes visible.   This took several days for this supernova.

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-    Other massive stars often shed mass.    Betelgeuse has shed mass over late 2019 and early 2020, when it belched out a cloud of matter with ten times the mass of Earth’s moon that blocked some of Betelgeuse’s light, causing it to appear dim.

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-     Betelgeuse isn’t ready to go supernova just yet, and by the time it does, the ejected cloud will have moved far enough away from the star for the shock breakout to be immediately visible. In the case of SN 2023ixf, the ejected material was still very close to the star, meaning that it had only recently been ejected, and astronomers were not expecting that.

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-   The only way to understand how massive stars behave in the final years of their lives up to the point of explosion is to discover supernovae when they are very young, and preferably nearby, and then to study them across multiple wavelengths.  Using both optical and millimeter telescopes they effectively turned SN 2023ixf into a time machine to reconstruct what its progenitor star was doing up to the moment of its death.

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-    Stars, they're just like onions.  An evolved massive star as being like an onion, with different layers. Each layer is made from a different element, produced by sequential nuclear burning in the star's respective layers as the stellar object ages and its core contracts and grows hotter.

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-    The outermost layer is hydrogen, then you get to helium. Then, you go through carbon, oxygen, neon and magnesium in succession until you reach all the way to silicon in the core. That silicon is able to undergo nuclear fusion reactions to form iron, and this is where nuclear fusion in a massive star’s core stops.

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-    Iron requires more energy to be put into the reaction than comes out of it, which is not efficient for the star.    Thus the core switches off, the star collapses onto it and then rebounds and explodes outward.

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-    One possibility is that the final stages of burning high-mass elements inside the star, such as silicon (which is used up in the space of about a day), is disruptive, causing pulses of energy that shudder through the star and lift material off its surface.

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-    What the story of SN 2023ixf does tell us is, at the very least, that despite all the professional surveys hunting for transient objects like supernova.  Without early detection we would have missed the opportunity to gain critical understanding of the evolution of massive stars and their supernova explosions. 

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May 30, 2024        RARE  EARTH  METALS  -  how did they get here?         4488

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

--------  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”  -----------

--------------------- ---  Saturday, June 1, 2024  ---------------------------------

 

 

 

 

 

           

 

 

4489 - EINSTEIN - how did he get so smart?

 

-    4489  -   EINSTEIN  -   how did he get so smart?  -    Albert Einstein was arguably the most famous scientist of the 20th century. Most people are familiar with his iconic E=mc^2 equation, but his life and work encompassed so much more than that. For instance, the brilliant physicist actually won the Nobel Prize for very different work. From his humble beginnings as a patent clerk to the offer to run a small country (that he turned down).

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-------------------------------------  4489    -    EINSTEIN  -   how did he get so smart?

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-     Albert Einstein was much more than a scientific genius. From his political beliefs to his hatred of socks.

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-    Einstein discovered that the universe has a "speed limit."   His special theory of relativity, which explains the relationship between mass, time and space, suggests that as an object approaches the speed of light, its mass and energy become infinite.   That means that it's impossible for an object to travel faster than light.

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-    He argued that space and time are interwoven.   While Einstein didn't invent the concept of space-time, which was first proposed by German mathematician Hermann Minkowski, his special theory of relativity showed that space and time grow and shrink relative to one another in order to keep the speed of light constant for the observer.

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-    Based on his theory, when we travel through space, time moves a tiny bit slower. At incredible speeds, like the speed of light, “time stands still”.

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-   The photoelectric effect is the observation that metal plates eject electrons when hit by beams of high-energy light. The photoelectric effect can't be explained by classical physics, which saw light as a wave. Einstein proposed that we view light as both a particle and a wave with the frequency of the wave determining the energy of the particle and vice versa.

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-    Einstein transformed the way physicists view light.  Before Einstein's special theory of relativity, physicists thought that light traveled through a substance called "the luminiferous ether." Throughout the late 19th century, scientists ran experiments to try to prove its existence.

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-    Beginning at age 5, Einstein became captivated by the invisible forces that moved the needle of his compass. That led to a lifelong quest to explain those invisible forces.   At the age of 12, he taught himself geometry.   To study, he read out of a textbook, which he dubbed his "holy geometry book" and "second miracle" (the first being his compass needle).

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-      He wasn't well-liked by his teachers.   One of the instructors at the Luitpold-Gymnasium in Munich, where Einstein received much of his early education, told the young Einstein that nothing good would ever come of his life.

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-   At 5 years old, his mother signed him up for music lessons. At first, he didn't enjoy playing the violin at all.   But, after discovering Mozart, he developed a love for the hobby and played into his old age.

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-    He wrote his first scientific paper at the age of 16.   Einstein writing by hand.  It was titled "On the Investigation of the State of the Ether in a Magnetic Field," the essay asked how magnetic fields impact "ether," the theoretical substance that at the time was believed to transmit electromagnetic waves.

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-   After university, Einstein was rejected from every academic position he applied for.

There was a row of folders at the a patent office, with a label tab that reads "new patent applications"  Eventually, he settled for a job evaluating patent claims for the Swiss government. He described the job, which gave him the time and energy to focus on solving the physics problems that underlie our world, as "a kind of salvation."

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-    He helped convince the physics world that atoms exist. Einstein was interested in the problem of “Brownian motion”, the observation that if you put tiny objects (like pollen) in water, they appear to jump around erratically. Einstein proposed that invisible particles were colliding with the pollen, causing it to move, and came up with a formula describing this phenomenon.

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-    In 1908, French physicist Jean Baptiste Perrin tested and confirmed Einstein's theory, swaying the physics world to accept the existence of atoms.

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-   Einstein was a pacifist.   At 16, he left Germany to escape mandatory military service. Later, he was one of only four German intellectuals to openly declare their opposition to German participation in World War I, calling nationalism "the measles of the human race."

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-    Einstein's theories of relativity challenged the view that the universe was static.  His equations predicted a dynamic universe, one that was expanding or contracting. Flummoxed by this finding, Einstein assumed there was a flaw in his equations and introduced a "cosmological constant" which allowed for a universe that didn't change size. When Edwin Hubble confirmed that the universe is, indeed, expanding, Einstein called the cosmological constant "his greatest mistake."

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-   In 1905, dubbed his "year of miracles," Einstein published his explanation of the photoelectric effect, his theory on Brownian motion, and two papers on his general theory of relativity.

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-    He was friends with Charlie Chaplin.   Chaplin even invited Einstein and his wife, Elsa Einstein, as his guests of honor at the premier of his 1931 film "City Lights." There, Chaplin famously told Einstein: "The people applaud me because everybody understands me, and they applaud you because no one understands you."

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-    Einstein believed in God.   However, he didn't believe in a personal god that answered prayers. Instead, he thought that God revealed himself through the "harmony" of the universe. "He does not play dice,"  he famously wrote.

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-    Einstein was a target for the Nazis.  They sponsored conferences and book burnings against Einstein and labeled his theories "Jewish physics." In 1933, Einstein fled Germany to escape Nazi death threats, settling first in Britain and then eventually in Princeton, New Jersey.

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-   The equation E = mc2 provided the theoretical basis for the weapon's potential, but didn't explain how to build one.    At the start of World War II, he wrote to then-President Franklin D. Roosevelt, warning of possible German nuclear weapons research.

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-    He urged the president to initiate development of an atomic bomb, but later regretted doing so. In an interview with Newsweek, he said: "Had I known that the Germans would not succeed in developing an atomic bomb, I would have done nothing."

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-   After the bombing of Hiroshima and Nagasaki, he formed the Emergency Committee of Atomic Scientists, an organization that educated Americans about the dangers of atomic weapons.

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-    Einstein was a member of the National Association for the Advancement of Colored People.   He saw parallels between the experience of Black Americans and his experience as a Jew living in Nazi Germany.  In a 1946 commencement speech delivered at the historically black college Lincoln University, Einstein decried segregation and called it "a disease of white people,".

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-    The FBI kept a 1,400-page dossier on Einstein.   His pacifist stance and left-leaning politics made him suspicious in the eyes of the agency as a potentially "extreme radical".   This was especially true during the McCarthy era, when many people were accused of communism or blacklisted from work.

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-    Einstein was asked to be the president of Israel.   However, when he was offered the position in 1952, he was already near the end of his life. Due to his poor health and lack of experience "dealing properly with people," he declined.

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-   He did not believe that black holes could exist.  In a 1939 article, he laid out a series of arguments trying to prove that black holes, objects with such high gravity that even light can't escape them, are impossible. Ironically, It's Einstein's general theory of relativity that shows us black holes do, in fact, exist.

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-   He did believe in the possibility of wormholes.   In a 1935 paper published in the journal Physics Reviews, Einstein and physicist Nathan Rosen proposed that near objects of enormous mass, space-time might curve inward like a rubber tube, creating a tunnel between two different regions. If they exist, these objects would enable travel across vast distances of time and space.

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-   Einstein didn't wear socks.  Black holes weren't the only holes this physicist vehemently disagreed with. Because socks invariably develop holes, he disliked them to such an extent that he refused to wear them.

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-  After his death in 1955, pathologist Thomas Harvey dissected and stole Einstein's brain during an autopsy. Harvey, who wanted to discover the anatomical secrets of genius, eventually received permission from Einstein's son to use the brain for scientific research.

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-    The human brain's wrinkled surface gives it a much larger surface area than a smooth brain and is an important part of advanced cognition. Einstein's brain had extra folding in its gray matter, the site of conscious thinking, especially in the frontal lobe, where abstract thought and planning occurs.

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-    He loved sailing.   However, the physicist was terrible at it, so terrible, in fact, that his neighbors frequently had to rescue him when is boat invariably capsized.

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-   His birthday is Pi Day.   March 14 is a special date because written numerically, it matches the first three digits of mathematical constant pi: 3.14. However, that's not the only reason it's significant. It's also the birthday of Einstein, who was born in 1879.

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-    Einstein invented a refrigerator.  The contraption, which he developed alongside colleague Leo Szilard, didn't require motors or coolant. Instead, it used boiling butane to suck energy from a compartment, lowering the temperature inside.

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-   Einstein's ultimate goal was to describe the workings of the entire universe from subatomic particles to the farthest reaches of space in one theory.   He called the concept "The Grand Unified Theory." He never realized this dream, but physicists are still working to find it.

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May 22, 2024               EINSTEIN  -   how did he get so smart?             4489

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