6 Fascinating Facts About the Nucleosynthesis Era.

6 Fascinating Facts About the Nucleosynthesis Era

These are 6 fascinating facts about the Nucleosynthesis Era. From 10-billion degrees Fahrenheit to our universe’s first star. If you want to learn 6 fascinating facts about the Era of Nucleosynthesis, this is the article for you. Let’s jump right in! #1 Still Hot, Hot, Hot Currently, the universe continues undergoing rapid “cooling.”  However, we quote the term “cooling” because temperatures during the Era of Nucleosynthesis sit at 10-billion degrees Fahrenheit.  Actually, compared to the big bang and following epochs, these temps truly are much colder. #2 Electrons Everywhere During the Era of Nucleosynthesis, basic atoms, like hydrogen have formed.  In other words, atoms with single-proton nuclei.  However, these nuclei are still so hot that electrons are unable to stick to the atoms.  Ultimately, the universe has freely-floating electrons, flying aimlessly throughout space. #3 The Whole Universe Is the Sun’s Core During the Era of Nucleosynthesis, the universe was still amazingly hot and dense.  In fact, our entire universe acted very similar to stars’ core, like our Sun.  Plus, spooky things happen under such tremendous heat and pressure, like atoms smashing together to form different atoms.  Actually, we still see this today within our Sun. It’s called nuclear fusion. #4 Nuclear Fusion Powers On Despite the universe cooling dramatically, atoms stay hot.  In fact, the nuclei inside of atoms stays hot and pressurized enough for nuclear fusion to carry out.  Therefore, hydrogen atoms with a single proton nucleus smash together to form heavier helium.  Plus, trace amounts of even heavier elements arise, like lithium. #5 Still No Light… at All During nuclear fusion, photons of intense gamma radiation are generated.  In fact, this also happens within the core of our Sun and all stars.  Actually, these photons eventually escape the Sun’s core, flying out into space. We call this LIGHT.  Except, light photons during the Era of Nucleosynthesis had nowhere to go.  No matter which direction they float, only more dense, hot space exists. #6 The Perfect Star Recipe Finally, upon nucleosynthesis, our universe has a composition that resembles modern times.  In other words, 75% hydrogen, 25% helium, and less than 1% trace elements, like lithium.  Actually, these will eventually become the perfect ingredients to make our universe’s first stars.

10 Fascinating Facts About the Particle Era.

10 Fascinating Facts About the Particle Era

These are 10 fascinating facts about the Particle Era. From 1 million miles in 1 second to the stuff we’re made of. If you want to learn the best Particle Era facts, this is the article for you. Let’s jump right in! #1 A Rapid Growth Spurt Previously, in other epochs, the universe was microscopic. In fact, epochs like the Planck Era saw a universe that was smaller than a single atom.  But, suddenly, in the Particle Era, the universe expands to more than 100-million-miles in diameter.  Not to mention, this expanse took place in under one second. #2 A Lot Has Happened in a Short Time As noted above (see #1), a tremendous amount of change has occurred within the universe.  Furthermore, this amazing change has happened in mere fractions of a single sentence.  Rapid inflation, matter creation, wild temperature fluctuations.  And, all of this within a mere fraction of time since the big bang. #3 Relatively “Cool” Outside Today During these early time, in the universe’s infancy, things were extreme.  In fact, temperatures during the Particle Era were considered drastically “cooler.”  Yet, “cool,” simply meant a staggering 18-trillion degrees Fahrenheit. #4 A World of Quarks and Antiquarks During the Particle Era, matter had not yet begun. No protons, neutrons, nor a single electron had been born.  However, during this odd epoch, the universe was filled with quarks and antiquarks.  Quarks serve as foundational particles, making up protons and neutrons.  However, when the Particle Era began, these particles were still unable to “stick” together. Hence, an endless sea of quark soup! #5 The Most Legendary War in History During the Particle Era, the universe begins pumping out equal amounts of matter and antimatter.  Antimatter is identical to its matter counterpart but with an opposite charge—for instance, quarks and antiquarks.  However, when the two particles come in contact, they instantly annihilate each other. All that is left is pure energy in the form of gamma rays. #6 Nuclear Strong Force Takes Hold Finally, all four fundamental forces were separate and unique during the Particle Era.  Plus, the universe had cooled enough for the strong nuclear force to take effect.  As the name denotes, this strongest of the forces firmly binds particles together, allowing nuclei to be created.  Ultimately, this is the first time the universe saw formal nuclei. Finally, matter! #7 We Could Have Been Pure Energy As mentioned previously, when matter and antimatter collide, they destroy each other, leaving only pure energy behind.  Therefore, had the universe permanently continued creating equal amounts of both matter and antimatter particles, the universe would have been pure energy.  Essentially, the universe would have remained a larger version of the big bang aftermath. #8 Nothing Could Have Never Existed Technically, had matter not won the legendary matter-antimatter battle, we would have never existed.  Indeed, the two particles would have continuously destroyed each other. Thus, disallowing any matter to exist. No planets, stars, galaxies, or anything else. After all, everything we know is made of matter. #9 We Are All Here Because of the Particle Era Matter comprises 100% of human beings.  You, your family, your friends, pets, and everybody else are made of it. Therefore, the matter-antimatter battle during the Particle Era ultimately created… us.  Basically, an event that lasted less than one millisecond gave way to everything we know in our existence. Mind blown? #10 One of the Universe’s Greatest Mysteries Somehow, in a seemingly dead-even match-up, matter won out over antimatter.  Plus, the entire war took place in less than one second during the Particle Era.  However, nobody has a clue how or why matter won. For all we know, antimatter could have just as easily won.  Fortunately, matter won, allowing life and everything we know to occur.  Yet, this remains one of astronomy’s greatest unsolved mysteries.

10 Stars Which Turn Supernova Next.

10 Stars Which Turn Supernova Next

Here are the 10 stars most likely to go supernova next: RS Ophiuchi 119 Tauri Pi Puppis Rigel Gamma Velorum Betelgeuse Antares Alpha Lupi Spica IK Pegasi Supernovas are visible during the day for up to several weeks or months. So if you want to learn all about which stars are most likely to supernova next, then you’re in the right place. Let’s jump right in! Stars and Supernovas Stars are delicate machines, using perfect balances of gravity pushing in and nuclear power pushing out.  When a massive enough star runs out of nuclear fuel, gravity wins, and the star collapses on itself.  Now, a massive explosion happens, a supernova. But, what is the next star to go supernova? Supernovas emit tremendous energy.  In fact, a supernova would temporarily shine brighter than everything except the Moon in our sky.  Actually, it would even be visible during the day for up to several weeks or months. Now, that would be a true sight. Unfortunately, supernovas in our region of the Milky Way only occur once every 50 to 100 years. Therefore, the science community is constantly trying and hoping to predict which nearby star will explode next.  So, here are the top 10 candidates for the next star to go supernova. Keep reading! #1 RS Ophiuchi Nearly 4,000 light-years away in the constellation, Ophiuchus, RS Ophiuchi is a white dwarf nova system.  Plus, it’s in its late evolutionary stages. RS Ophiuchi is relatively close and prime to go supernova. #2 119 Tauri 119 Tauri is 1,700 light-years away, in the constellation Taurus.  And, as one of the reddest stars seen with the naked eye, 119 Tauri is also 600 times the mass of our Sun and ready to explode. #3 Pi Puppis The next star to go supernova could be Pi Puppis. Constellation Puppis’ second brightest star is only 1,100 light-years from Earth.  Plus, Pi Puppis is a supergiant that has already consumed all of the hydrogens in its core. #4 Rigel The next star to go supernova could be the seventh brightest star in the sky, Rigel.  Actually, Rigel is part of a triple or quadruple star system.  Plus, at 860 light-years away in the constellation Orion, Rigel would put on quite a show. #5 Gamma Velorum Gamma Velorum lies 800 light-years away in the constellation, Vela.  And, as one of the brightest stars in the night sky, Gamma Velorum is part of a four-star system.  Now, Gamma Velorum has already shed its outer layers and is on the way to going supernova. #6 Betelgeuse One of the most notable stars in Orion, and the ninth brightest in the ski, is Betelgeuse. At 640 light-years away, Betelgeuse is a massive red giant star.  In fact, if Betelgeuse were our solar system’s star, it would extend beyond Jupiter’s orbit.  Plus, nearing the end of its life, Betelgeuse is expected to go supernova any day now. #7 Antares Scorpius’ brightest star, Antares, is possibly the next star to go supernova. Not to mention, this massive red supergiant is only 600 light-years away.  In other words, this explosion would create an unparalleled sight in our sky. #8 Alpha Lupi Constellation Lupus’ brightest star, Alpha Lupi, may be the next star to go supernova.  At a measly 460 light-years from Earth, Alpha Lupi has a mass of more than 10 Suns.  Alpha Lupi is locked and ready to go supernova. #9 Spica Spica is the Virgo constellation’s brightest star. It’s also a likely candidate for the next star to go supernova.  Plus, at only 240 light-years away, Spica would put on a display, possibly brighter than a full Moon.  Spica’s explosion would be seen in broad daylight for several weeks. #10 IK Pegasi Only 150 light-years from Earth, IS Pegasi is now a white dwarf.  In other words, the star is in the late evolutionary stages of its life.  Now, it’s only a matter of time before it explodes, giving us an incredible sight in the night and daytime skies.

What Is the Hottest Planet in Our Universe?

KELT-9b: Hottest Planet in Our Universe?

This is about the hottest planet in our universe: KELT-9b. The hottest planet in our solar system is Venus. So if you want to know more about the hottest planet in our universe is, you’re in the right place. Let’s get right into it! Hottest Planet in Our Universe Since confirming our first official exoplanet discovery in the early 1990s, we have spotted all shapes, sizes, speeds, and more.  However, a new champion for the hottest known planet was crowned in 2017, KELT-9b. Hottest of Hot Jupiters In our exoplanet search, it’s not uncommon to find Hot Jupiters, gas giant of Jupiter’s size and mass with a close, almost Mercury-like orbit around its star.  Often earning the alternate nickname, roasters, these planets clearly experience wildly hot temperatures.  Yet, the discovered KELT-9b has officially blown the competition away, experiencing daytime temperatures of 7,800º Fahrenheit.  In other words, KELT-9b is hotter than most stars. No, that’s not a typo. Announced at the 230th meeting of the American Astronomical Society by B. Scott Gaudi (Ohio State) and Karen Collins (Vanderbilt University), KELT-9b was discovered during the KELT survey (Kilodegree Extremely Little Telescope).  KELT surveys the sky for abnormally bright and large stars, typically left unexplored by other exoplanet missions, like NASA’s Kepler. At three times Jupiter’s mass and twice its size, even KELT’s small telescopes could spot KELT-9b orbiting its parent star. All in the Parent Star KELT-9b owes its record-setting temperatures mostly to its Sun, KELT-9.  The large A-type blue giant star is around 2.5 times our Sun’s mass.  However, KELT-9 produces staggering temperatures, blasting out lethal ultraviolet radiation. The scorching radiation is causing the planet to simply evaporate as it orbits the star.  In fact, it may be losing 100 billion to 100 trillion grams of atmosphere per second, according to Gaudi. The evaporating material likely gives KELT-9b a comet-style tail. Plus, the KELT-9 parent star rotates so rapidly that it takes on an egg-like shape (depicted in article feature image).  Actually, this same effect can be seen in our own solar system’s Saturn. Weird Behaviors of KELT-9b A planet slowly evaporating is strange enough. However, it is only one of many other odd things about KELT-9b. KELT-9b is tidally locked with its Sun, meaning the same side constantly faces the star.  Our Moon is tidally locked with Earth, causing its so-called permanently “dark side.”  As a result, this side experiences the sweltering 7,800º temperatures.  Not to mention, molecules and potential for life are simply unable to be produced on this side. Alternatively, the “dark side” of KELT-9b lies in eternal darkness. But, with the planet’s minuscule atmosphere, heat is likely not easily transferred from the daytime side.  As a result, the planet’s dark side is drastically “cooler.” However, under such radiation, the planet’s sheer surface temperature ensures truly hot conditions, regardless of side. Existing so close to its Sun, like Mercury, KELT-9b orbits rapidly in only 1.5 days! Not all that uncommon, right? But, unlike most planets, KELT orbits perpendicular to its star’s axis of rotation.  In other words, the planet orbits over and under the star’s north and south poles. That is rather uncommon. Unlivable, but Worth It Indeed, this planet is completely unsuitable for human life as we know it. But, studying the mysterious planet is well worth our efforts. According to Gaudi, Earth-like planets orbiting Sun-like stars are both desirable and relatively easy targets.  Yet, worlds like this help us learn how planetary systems form around hotter, brighter, more massive stars.  While living on KELT-9b may be out of the question, it may provide one more puzzle piece for understanding our fascinating universe.

Dragonfly 44 Galaxy - 99.9% Dark Matter.

Dragonfly 44 Galaxy: 99.9% Dark Matter

This is about the galaxy Dragonfly 44. Dragonfly 44 is made of 99.9% dark matter. So if you want to learn more about the Dragonfly 44 galaxy, you’re in the right place. Let’s jump right in! Galaxy Dragonfly 44 Discoverd Using the W.M. Keck Observatory on Mauna Kea in Hawaii, astronomers have located a unique galaxy, Dragonfly 44.  Tucked 70,000 light-years away in the Coma Cluster, Dragonfly 44 has approximately the same mass as our own Milky Way galaxy.  Yet, it contains less than one-hundredth of our star count. But, how can that be?  If this galaxy contains drastically less matter than ours, how could it have the same mass?  Astronomers believe this inconsistency is because Dragonfly 44 is composed of around 99.9% dark matter. What Is Dark Matter? The short answer: nobody really knows. But, dark matter is a type of matter that does not interact with the electromagnetic spectrum.  In other words, it does not interact with the matter that our entire worlds and lives are based upon.  Because of this, scientists are not able to directly observe, test, or see dark matter, hence the name. In fact, we now know that all of the normal matter in our known universe only accounts for less than 5% of its total mass.  That means that all of the stars, planets, galaxies, and everything else you can imagine is only a fraction of the universe.  So, when you look at the night sky, the black space in between stars is not quite as empty as you may think. How Do We Know Dragonfly 44 Is Made of Dark Matter? Currently, we are only able to observe dark matter through its impacts on surrounding visible matter.  Astronomers can accurately measure a galaxy’s mass based on the motions of the galaxy’s stars.  Basically, certain levels of mass cause specific speeds and motions of stars. However, when astronomers observed Dragonfly 44, stars were moving remarkably fast compared to the mass contained in the galaxy.  Actually, their measurements indicated that around one one-hundredth of one percent of Dragonfly 44’s mass was in the form of visible matter, like stars.  They knew something must be causing these puzzling speeds. This was when researchers became convinced that the missing mass must be in the form of dark matter. Why Is Dragonfly 44 Important?  Unraveling the dark matter mystery is currently at the top of nearly very astronomers’ and physicists’ lists. This invisible matter that accounts for a very large portion of the known universe will be the discovery of the century, no doubt. Dragonfly 44 is relatively nearby in cosmic terms, allowing it to be observed much easier than distant, ancient galaxies.  Also, if the galaxy truly is composed almost entirely of dark matter then, what better place to study the elusive material? Finally, with an unusually low surface brightness and sparse star count, Dragonfly 44 allows for clear, uncluttered observation. But, again, this can only help with attempting to understand dark matter. What Is Next For Dragonfly 44? Needless to say, the dark matter debacle will not likely be resolved in the very near future. But, Dragonfly 44 will certainly be a nice stepping stone to help with the quest. This galaxy sits in a group of more than a thousand identified galaxies, known as the Coma Cluster.  Researchers are already seeking and identifying other galaxies in the cluster with similar low brightness to Dragonfly 44.  Perhaps these peculiar entities will be one of the keys to solving modern astronomy’s arguably biggest mystery, dark matter.

Proxima Centauri B: Earth-Like Planet in Our Cosmic Backyard.

Proxima Centauri B: Earth-Like Planet in Our Cosmic Backyard

This is about the exoplanet Proxima Centauri B. There might be life on Proxima Centauri B. So if you want to know more about Proxima Centauri B, this is the article for you. Let’s get started! Exoplanet Centauri B Proxima Centauri B looks to be the leading candidate for a cosmic home. In recent years, the search for exoplanets (planets beyond our solar system) has been productive and exciting.  Since its official start in 1988, we have discovered over 3,500 confirmed exoplanets. More specifically, the search is for Earth-like planets.  Most importantly, we seek planets orbiting within a particular distance from their star, known as the habitable zone. It is in this specific zone that a planet can support the presence of liquid water.  Where this is liquid water, there is oxygen, and where there is oxygen, there is, or could be, life. How Far Away Is Proxima Centauri B? The exciting new exoplanet was confirmed orbiting the star Proxima Centauri, which is 4.42 light-years away.  In cosmic terms, this is right in our backyard. Truly, this is the closest star to our solar system. Now, in human terms, this is nearly 25 trillion miles away, which poses obvious problems. Unfortunately, even traveling at 150,000 miles per hour would take us nearly 18,000 years to reach the neighboring star. But, as technology advances over upcoming decades, experts hope this time diminishes greatly. As it has always been, the goal is to find ways to increase our travel speeds and methods.  Since light speed is the universe’s official speed limit, the goal is to travel as close to this velocity as possible.  If we could travel at light speeds someday, journeying to Proxima Centauri B would be a short 4-year voyage. Could There Be Life on Proxima Centauri B? Confirming that a planet orbits in the habitable zone are only one step to determining whether it can harbor life.  For instance, Venus is just inside our habitable zone and is one of the most lethal places in our entire solar system.  Like many planets, Venus likely lost its atmosphere in its young life due to the harsh bombarding materials from the Sun. Two primary features are key for a planet’s habitability: atmosphere and magnetic field. Both items shield a planet from deadly incoming materials of stars and the rest of the universe.  Without these protectors, even planets in the habitable zone, like Proxima Centauri B, can be barren, freezing wastelands. Proxima Centauri B Characteristics Part of searching for a human-friendly planet is mass.  As we see in large planets like Jupiter, too much mass creates environments entirely unsuitable for human life.  Fortunately, Proxima Centauri B is thought to be around 1.3 times Earth’s size, which is a completely acceptable (and exciting) size for a planet. Plus, if Proxima Centauri B does still have its atmosphere, its temperatures may be as high as 86º F on the sunny side and as low as -22º on the shaded side. These are absolutely manageable temperatures for human lifeforms. What Comes Next For Proxima Centauri B? Similar to most astronomical findings, the next step is research, research, and more research.  Instead of jetting off to visit the newly found planet, astronomers will likely push telescopes to their limits to further investigate the world. Regardless, this discovery marks a turning point in science. This is a shot of hope and confidence that Earth-like planets orbiting similar stars in habitable zones are not out-of-the-question. Furthermore, finding a planet orbiting the closest star to Earth after years of observations tells us that we are likely to find these planets in many places if we continue searching. Thus, this kind of boost will only continue to heat up the search for habitable exoplanets.

How Big Is the Milky Way (Human Comprehendible Format)

How Big Is the Milky Way Really?

This is about how big the milky way is. In plain numbers, the milky way is 52,850 light-years big. However, if you want to understand the milky way’s size and distances in a human comprehendible format, then you’re in the right place. Let’s do this! Milky Way’s Size in a Human Comprehendible Format Indeed, our universe is truly gigantic.  But, even small parts of our universe are still absolutely vast.  In fact, even our home galaxy proves truly mind-boggling when it comes to distance.  So, just how vast is our native galaxy?  We break it down with Milky Way distances on scales that even we tiny humans can understand. Let’s get started! What is a Light-Year? As we explore the amazing Milky Way distances in this article, it’s helpful to understand the speed of light.  Simply put, light is the fastest thing in our universe, our cosmic speed limit. So, how fast is that? Without anything in its way, light travels at a staggering 186,000 miles per second.  Yes, per second.  In other words, light can travel all the way around planet Earth seven times in a single second. Compared to Our Solar System Previously, we explained our solar system distances in human-friendly terms.  But, our solar system is a mere blip or pixel of our entire galaxy, the Milky Way.  In fact, over 500 solar systems have been discovered in our Milky Way.  Not to mention, our Milky Way is simply one of at least 100 billion galaxies in our observable universe.  But what does that mean for our galaxy’s size? Simply put, our solar system is a speck compared to the Milky Way.  Our Milky Way galaxy is a whopping 587 trillion light-years across.  In other words, you could travel across our entire solar system 53,000 times and still not equal one trip across the Milky Way. Even NASA’s New Horizons, known for its ground-breaking 2015 Pluto flyby, currently holds the spacecraft speed record at 36,000 miles per hour.  Still, New Horizons would take 1.9 million years to journey across the Milky Way galaxy.  Put another way, that is the time since the Bible was written, multiplied by 930. Compared to Earth Next, how does our life-bearing home planet, Earth, compare to the Milky Way.  After all, Earth is just one of at least 100 billion planets thought to exist in our galaxy.  Plus, Earth’s size is, at best, very average and quite unimpressive. Still, at over 7,900 miles wide, Earth is huge to humans.  But, you would have to line up nearly 75 billion Earths to stretch across the Milky Way galaxy.  Plus, at 24,000 miles around, it would take more than 24 billion trips around planet Earth to equal one cross-Milky-Way trip. Even the United States of America, at 2,600 miles across, feels truly large to us.  Still, 220 billion trips across the USA would not quite equal one journey across our Milky Way.  Mount Everest, standing tall at 29,000 feet high, is planet Earth’s highest mountain.  But, it takes almost 107 trillion Everest climbs to equal one Milky Way voyage. Compared to Human Beings Last but not least, we seven billion people are the only life, as we know it, in our entire universe.  No other planet is known to contain animals, spacecraft, technology, insects, or anything else.  So, how big is the Milky Way compared to humans? We all know bullets travel fast. In fact, they are capable of around 1,700 miles per hour.  However, even these lightning speeds are a mere 0.0001 percent of light speed. Therefore, a bullet would take nearly 40,000 years to travel across our Milky Way. Also, sound, another phenomenon synonymous with quick speeds (761 miles per hour).  Therefore, a sound wave would take nearly 88 million years to journey across our galaxy.  In other words, that’s more than 32 billion days, or, 771 billion hours. Currently, The Koenigsegg Agera R holds the record for the fastest automobile at 273 miles per hour.  But, the Agera R, constantly traveling at top speeds, would take almost 90 billion days to cross our galaxy. Now, at 105 miles per hour, man’s fastest baseball pitch would take over 230 billion days to float across the Milky Way. Strike!  Even the fastest known animal, the cheetah, bolting at an impressive 61 miles per hour would take a billion years to span our home galaxy. In other words, that’s 400 billion hours or 9.6 trillion hours. Finally, those truly ambitious aspiring astronauts could choose to walk across the Milky Way.  However, be forewarned that your journey would last for nearly 190 quadrillion hours. Indeed, that is “190,” followed by 12 zeros.  Simply put, a Milky Way walk would take more than 41,000 times planet Earth’s entire life (4.6 billion years).  Otherwise, your trip would require over 2.6 trillion human lifespans.

10 Facinating Facts About the Kuiper Belt.

10 Facinating Facts About the Kuiper Belt

These are 10 fascinating facts about the Kuiper Belt. From the Kuiper Belt was predicted and then discovered to ices from the time our Solar System formed. So if you want to learn 10 Kuiper Belt facts, then this article is for you. Let’s jump right in! #1 The Kuiper Belt Is Way Out There The Kuiper Belt lies beyond the orbit of Neptune in our solar system.  In fact, the icy belt extends from 30 to 55 astronomical units out from the Sun.  In other words, that’s 2.8 – 5.1 billion miles out. #2 Predicted, Then Discovered Like many things in science, the Kuiper Belt was first predicted by Gerard Kuiper in 1951.  Only later, in 1992, did a team of astronomers observed the first Kuiper Belt Object after five years of scouring the skies. #3 Dear Kuiper Belt, Thank You for the Moons Planets Neptune and Saturn are believed to have gotten at least one of their moons from the Kuiper Belt.  Indeed, as large icy bodies became knocked loose, the gas giants roped them into their powerful gravity. #4 The Neighborhood of a Famous Planet The Kuiper Belt is home to several dwarf planets, such as Makemake, Haumea, and more.  However, the belt is also home to Pluto, our beloved former planet.  In fact, Pluto is the largest object in the Kuiper Belt.  Ultimately, planet or not, Pluto has a special place in our hearts and solar system! #5 The First Mission to the Kuiper Belt As of July 2015, a human spacecraft reached the Kuiper Belt.  NASA’s New Horizons mission official reached the belt as it approached the former planet, Pluto.  Originally blasting off from Cape Canaveral in 2006, the craft blazed at 36,000 miles per hour to reach the frozen target for nine years. #6 Close Encounter With a KBO After successfully reaching Pluto and captivating the world, NASA granted New Horizons an extended mission.  The craft is now en route to a Kuiper Belt Object (KBO), which it will reach in early 2019. #7 Snap, That’s a Lot of Comets The Kuiper Belt is believed to contain more than a trillion comets.  In fact, when the gravity of other objects knocks the comets free, they often enter our solar system.  Actually, several of the comets that frequent our inner- and outer solar system are thought to have originated in the Kuiper Belt. #8 Fascinating Retractable Atmospheres Indeed, our universe is full of bazaar objects.  However, some planets in the Kuiper Belt have retractable atmospheres.  As the planets grow increasingly farther from the Sun in their orbits, their atmospheres begin to collapse, only to appear again as they approach the Sun again. #9 Frozen Clues About the Solar System Ices in the Kuiper Belt date back to the time our solar system first formed. Because of this, the ice chunks give us valuable clues about conditions during this time.  In fact, our solar system’s formation is still one of astronomy’s biggest mysteries.  Therefore, scientists are eager to learn more about the Kuiper Belt, and in turn, our solar system. #10 One of Many Kuiper Belts Astronomers have observed Kuiper Belts surrounding at least nine other stars.  Actually, Hubble Space Telescope has even imaged such icy discs around two stars (HD 138664 and HD 53143).  While astronomers are eager to learn more about how and why such belts form, they are still a large mystery.

How to Watch the Birth of Our Universe (Big Bang Static TV).

How to Watch LIVE the Birth of Our Universe

This is how you can watch live the birth of our universe on TV—the so-called Big Bang. Television and radio antennae are sensitive to the Big Bang’s microwave frequency. So if you want to witness live the birth of our universe and all the details about it, then you’re in the right place. Let’s get started! The Big Bang on TV The Big Bang is, flat-out, the single greatest mystery to human beings. It is the missing key to understanding how life began and also how life may end.  But, no matter how mysterious, did you know that you can simply watch our universe’suniverse’s creation from your home through Big Bang TV static? Well, maybe you can’tcan’t actually watch it happen. But, you can observe real evidence from the Big Bang through TV static.  You know those random black and white specs you hear and see when you are in between channels, or your antenna is broken?  These are radiation waves.  And a small percentage of these waves is the afterglow of the universe’suniverse’s biggest mystery, the Big Bang. To understand more about where these waves come from, let’slet’s do a VERY general overview of the Big Bang. Flashback to 13.77 billion years ago. Just after the Big Bang, the universe was an extremely hot and opaque plasma of protons, electrons, and photons.  Typically, these components would combine to form simple atoms, like hydrogen. But, at this time, the universe was so hot that such combinations were not possible.  In fact, photons could not even pass through this dense plasma, rendering them unable to move freely. Now, 378,000 years later, the hot, thick electron-proton stew cooled enough to allow the matter to combine, forming hydrogen elements.  At this point, the universe was no longer opaque but completely transparent, and photons could now freely travel through space. This is the first light in our universe called the Cosmic Microwave Background radiation (CMB). Ever since that era, this light has been traveling through space. It has traveled for billions of years and sextillions of miles to reach our telescopes on Earth.  The light has become stretched out over these unimaginable distances as the universe has expanded, leaving them in the microwave spectrum. Seeing the Big Bang TV Static Fortunately, some of our television and radio antennae are sensitive to this microwave frequency.  So, when you are flipping through channels, or when your cable is down, you witness the Big Bang. Most of this static is caused by things like our Sun, other electronics, and lighting. But, a small portion (around 1%) is, in fact, the afterglow of our universe’suniverse’s creation.  The Internet will lead you across an array of different percentages and debates on the truth of this TV static theory. But, even reputable organizations, like CERN, acknowledge that this is a valid theory. Ultimately, when our televisions switched from analog to digital in 2013, the universe’suniverse’s magical static was canceled. These modernized electronics now receive different frequencies that are not residuals of the Big Bang. So, if you have an “”old school”” television sitting covered in dust in a crawlspace, it could be worth pulling out.  Turn off the Kardashians, and tune in to the beginning of everything we know.  After all, what could be more entertaining than our universe being born? How the Cosmic Microwave Background Radiation Formed Just after the Big Bang, the universe was an extremely hot and opaque plasma of protons, electrons, and photons.  Typically, these components would combine to form simple atoms, like hydrogen.  But, at this time, the universe was so hot that such combinations were not possible.  In fact, photons could not even pass through this dense plasma, rendering them unable to move freely.

10 Fascinating Facts About Sirius.

10 Fascinating Facts About Sirius

These are 10 fascinating facts about Sirius. You might observe Sirius during broad daylight. So if you want to learn 10 fascinating facts about Sirius, then you’re in the right place. Let’s get started! 10 Sirius Facts Gaze up at the night sky, anywhere on Earth, and you will see Sirius.  As the brightest star in our Earth skies, Sirius outshines planets, nebulas, and several other wonders.  But, Sirius is a complicated system containing two stars.  Chalked to the brim with fascinating features, both stars are among the most interesting objects the universe has to offer. #1 Smaller but Hotter Being two different types of stars, Sirius A and B have very different attributes. For instance, Sirius A is nearly 1.5 million miles across, whereas Sirius B is only 7,000 miles across.  Yet, Sirius A’s surface temperature is around 18,000º F, whereas Sirius B scorches at 45,000º F.  That’s nearly five times as hot as our Sun. #2 It Will Only Get Brighter Recent observations show that the Sirius system is slowly approaching our solar system.  In fact, during the next 60,000 years, the already bright star will only become brighter.  Eventually, the system will outshine the likes of Venus and other bright objects. #3 All of Your Ancestors Saw Sirius Humans have observed Sirius for centuries.  Actually, Sirius comes from the Ancient Greek term for “glowing.”  Ancient Egyptian civilizations 4,000 years ago based their calendars on Sirius rising and setting.  Even Polynesian civilizations used Sirius as their main navigation. #4 He Star so Bright, It Shines Without Night Sirius is extremely bright.  Plus, its “near” proximity to Earth amplifies its brightness that much more.  Some locations can even observe Sirius during broad daylight.  Naturally, city lights are unusually low in these areas. #5 One Ton of Sugar, Please! White dwarfs are large stars whose mass is smashed into a very small space.  Stars that were once millions of miles wide are now only dozens of miles wide as white dwarfs.  Because of this, gravity and density are immense. In fact, a sugar-cube-sized piece of Sirius B would weigh around one ton (2,200 pounds). #6 The “Dog Star” “Dog star” is a common nickname for Sirius. It earned this name by being the brightest (alpha) star in the constellation Canis Majoris, Latin for “greater dog.” #7 Closest White Dwarf to Earth Sirius B is now a white dwarf.  A massive star has already stopped generating nuclear fuel during this phase, shed its outer layers, and become much smaller and dimmer.  In fact, Sirius B is currently the closest white dwarf star to Earth.  #8 My Older Brother Used To Be Bigger Big and bright Sirius A is far larger and brighter than its companion, Sirius B. This is because Sirius A is a main-sequence star, one that is still alive and ticking.  Whereas Sirius B is now a white dwarf, much smaller, dimmer, and in its twilight years.  Billions of years ago, when Sirius B was still in its prime, it would have been the much larger of the two. #9 Always Together, Forever Apart Two companion stars comprise the Sirius star system, Sirius A and B.  Although gravitationally bound, the pair lies 20 astronomical units apart. This distance equates to around 1.8-billion-miles.  In other words, the same distance between Earth and Uranus. #10 The Two Brightest Star(s)?! Technically, Sirius is a two-star system. In astronomy, this is considered a binary system.  We are most familiar with much brighter Sirius A, which shines visibly in our night sky.  In fact, companion star Sirius B is around 10,000 times less bright. More Planet and Star Facts 10 Mars Facts 5 Mercury Facts 10 Sirius Facts