African tribe claims to have been visited by alien beings in ancient times
Ancient Astronomy – Sirius 1 is the main star in the star group Canis Majoris and the brightest in the night sky. Called the Dog Star by both ancient star watchers and modern astronomers, Sirius is mentioned in the cosmology and myths of many ancient cultures. In 1836, European astronomer Friedrich Bessel measured an imperceptible wobble in the orbit of Sirius, he believed was caused by something pulling on the Dog Star. After studying Sirius astronomers determined the Dog Star is orbited by a fainter companion star about every fifty years.
This unseen companion star, called Sirius B, was finally seen around 1862 by American telescope designer Alvin Clark, through an 18.5-inch refractor which was the most powerful telescope in the world at the time. It would be half a century before astronomers at California’s Mount Wilson Observatory discovered Sirius B is, in fact, a new type of super dense star they called a white dwarf.
The puzzle concerning the Dog Star deepened in 1950, when two noted French anthropologists just back from what’s today the Republic of Mali, reported that the unseen companion star had been the celestial keystone of the Dogon tribe’s cosmology for centuries. The French scientists had lived with the Dogon tribe for over a decade, by which time they had come to learn their cosmology. They reported watching Dogon holy people use sticks to scratch a rough diagram of the Dog Star, with a companion star circling it in an elliptical orbit, along with a third body astronomers had not detected yet.
Dogon holy people had told the two men the elliptical orbit of the unseen companion star stood for fertility. They said the small companion star orbited the main star every fifty years and was called po. It was made of a metal the Dogon called sagala, according to Dogon holy people, and was brighter than iron and so heavy the population of Earth couldn’t lift it.
The mystery went even further when the Frenchmen indicated the cosmology of the Dogon goes far beyond the star Sirius. They discovered the Dogon believe Jupiter has four large moons, Saturn is ringed, and the Earth orbits the Sun.
The mystery is how can a tribal cosmology that predates the invention of the telescope be so near to the truth? Do Dogon holy people have some means of viewing the universe using divination or some type of psychic power?
Some scientists indicate the Dogon were probably not as primitive or as isolated as first reported. In fact, they indicate the traditional homelands of the tribe are close to ancient trade routes that once linked West Africa with ancient Egypt. They also border a major trade road that connected regions in Africa during ancient times, the Niger River. Timbuktu, the home of one of the greatest Muslim universities of 400 years ago, was once just south of their lands. All of these things lead scientists to believe the Dogon’s cosmology could be due to these facts or even just outrageous lying.
Alien visitors from the stars
The Dogon cosmology could be due to cultural interactions, but some investigators still point to the similarities between the real Sirius star system and the Dogon cosmology as a mystery. The Dogon, however, say there’s no mystery involved. Hundreds of years ago, they were visited by a race of beings from the Sirius star system, they call the nommo. This ancient race told them things about the cosmology of the universe before they returned to their home planet.
Very few scientists or people believe the Dogon were in fact visited by beings from the star system Sirius. There has been no forthcoming explanation, however, for how the Dogon possess astronomy knowledge concerning bodies they can’t possibly have seen. Enough knowledge according to reports to accurately sketch unseen star systems in the sand.
Astronomy news (November 28, 2013) – The Hubble Space Telescope, along with the light magnifying ability of the effect called gravitational lensing, has provided the first views of the most distant galaxy seen during the human journey to the beginning of space and time. The astronomers of the Cluster Lensing and Supernova Survey with Hubble (CLASH) recently discovered three gravity-lensed images of a galaxy that existed over 13.7 billions years ago taken using Hubble’s new panchromatic imaging capabilities. Designated MACS 0647-JD, this ancient star city is currently the most distant galaxy located to date using the Hubble Space Telescope and gravitational lensing.
The CLASH program
The astronomers of CLASH used the Hubble Space Telescope to look at 25 distant galaxy clusters during the period from November 2010 to July 2013. They were looking for light which had been magnified due to the effect known as gravitational lensing as predicted by Einstein’s General Theory of Relativity. They wanted to detect additional Type Ia supernovae, map the distribution of dark matter in galaxy clusters, detect the most distant galaxies ever and study the internal structure and evolution of the galaxies in and behind these clusters.
The three gravity-lensed images taken by Hubble are of a small galaxy, now designated MACS 0647-JD, which could have been one of the first galaxies to exist in the universe. Astronomers’ analysis of the images suggests this small galaxy was less than 600 light-years across, which may indicate it was in the first stages of galaxy formation. In fact, this smaller galaxy may have been just one building block in the construction of a larger galaxy, and during the past 13.7 billions years could have been part of dozens, hundreds and even thousands of merging events with other galaxies.
Astronomers look at other possibilities
The astronomers of the Cluster Lensing and Supernova Survey with Hubble recently used the ability of NASA’s Spitzer Space Telescope to help rule out other possible identities of the three images they found. Next, astronomers will use the Spitzer Space Telescope, and other telescopes, to confirm the existence of the galaxy and try to get a better estimate of its age.
Prehistoric Irish astronomers built sunbeams for the dead
Ancient Astronomy – Archaeoastronomy
Just thirty miles north of Dublin stands Newgrange, one of the great astronomical wonders of the prehistoric world. Poised on a long, low ridge overlooking the narrow Boyne River, ancient farmers over 5,000 years ago built an oddly shaped temple mound more than 260 feet in diameter and 30 feet high. A wall of sparkling white quartz lines the river-facing southern edge of the mound, with an entryway in the middle guarded by a massive, intricately carved stone. This ancient house of the dead is more than a heap of stones gathered by prehistoric farmers to celebrate and remember the dead. It’s also believed to have been a cathedral to the life-giving force embodied in the sun.
The entrance leads to a passage sixty-two feet long, lined with forty-three stones, each taller than a man and weighing ten to twelve tons. At the end of the passage lies an intricate structure of massive rocks, some carved with symbolic designs, forming a cross-shaped chamber that rises into a vault over twenty feet above the floor. Set in the floor of each arm of the chamber is a large, flat rock with a shallow indentation carved into it, called a basin stone. It was here over 5,000 years ago bodies of the deceased were placed and once a year a slender beam of sunlight brought intimations of life to the remains of the dead at the exact moment of midwinter sunrise for seventeen minutes.
Newgrange Astronomers Built Over Thirty Houses of the Dead
Newgrange is the largest and most elaborate of three similar New Stone Age tombs built by ancient Irish farmers near this part of the Boyne River. This house of the dead is also just one of over thirty mounds in the region and predates the building of Stonehenge by over 1,000 years and Egypt’s pyramids by several centuries. A true monument to the astronomical knowledge and tomb building skills of the prehistoric sky watchers of Ireland. Newgrange and other mounds in the region stand as testimony to their desire to understand the mysteries of the universe.
Click on this link to watch a YouTube video called “The Cygnus Enigma”, on the discussion on the astronomical significance of Newgrange.
The portion of the sky the Hubble Space Telescope is currently looking at is full of planets both big and small
Astronomy News – One of the greatest things about being an astronomer is the excitement of mystery and wonder you feel every time you discover something you never even suspected. This must have been the feeling running through the minds of astronomers looking at the data provided by the Hubble Space Telescope indicating the presence of planets around distant stars. The rush of adrenalin as they went over the data they had worked and waited for must have been truly euphoric.
What kind of planets would they find? Smaller rocky worlds like Earth, larger gas planets like Jupiter, or some unusual planet never before dreamed of. All of their hard work and dedication to the task-at-hand is about to open a door of discovery to worlds of wonder. Worlds with environments unlike anything we have experienced on Earth, where life we could never envision might have evolved. This is why astronomers spend countless days, weeks, months and ultimately lives studying the sky above our heads.
Astronomers see a sky full of planets
The small portion of the sky being studied by astronomers using the Hubble Space Telescope is full of planets. Some appear to be of a similar rocky composition to our home planet while others appear to be totally inhospitable to Earth-type life. Planets like Earth are thought to be mainly composed of rocky material, which is denser and thus heavier than the materials making up gas planets. The planets being found orbiting stars in the portion of the sky being surveyed by Hubble are helping to rewrite planet formation theory and other areas of astronomical study. Astronomers are finding planets of types they were expecting to find, and a few they weren’t expecting to see.
The first planets found by the Hubble Space Telescope were large gas giants, like Jupiter and Saturn, but more recent finds have included planets similar in size and possible composition to Earth. Astronomers want to study Earth-like planets in an effort to uncover more secrets concerning the birth of our own solar system and the planet, which could give us clues to the development and evolution of Earth-like life in our universe. More recent developments even include the first direct imaging of a planet orbiting a distant star.
The truly amazing part is Hubble is only surveying a portion of the sky with around 100,000 suns and we’re finding more and more planets as astronomers continue to refine their planet finding techniques and instruments. Once we extrapolate and calculate the number of possible planets, using the available data so far gathered, we find the number of possible planets to be beyond count.
Astronomers will use the James Webb Space Telescope to journey to the beginning of space and time
During the 2013 human space odyssey, astronomers explored a portion of the night sky with the Hubble Space Telescope and exclaimed. It’s full of planets! In the years ahead during the human journey to the beginning of space and time, we expect astronomers to discover undreamed-of worlds, revolving around suns we humans can’t even conceive of. Especially once the James Webb Space Telescope comes online we should expect to visit undreamed of planets.
Best to buckle your seatbelt and prepare for the ride of your life! The human journey to the beginning of space and time is about to take off to planets beyond imagination. In the months and years ahead we expect to visit worlds with environments we would find inhospitable at best. Worlds where human survival would be doubtful and any life we found would be unusual beyond imagination.
Click this link to watch a YouTube video on weird planets in the universe.
“Blink, blink, Demon Star. We know not what you are”
Ancient Astronomy –
Tonight the human journey to the beginning of space and time travels 93 light years to the constellation Perseus, to check out Algol, a bright blue beacon in the sky astronomers in Egypt and China studied extensively for centuries. Called the Demon Star by some stargazers, this bright blue star was believed by ancient Greeks to represent the blinking eye of Gorgon the Medusa, held high in the hands of Perseus the Hero. This is thought to be the case due to periodic changes in the Demon Star that occur every few days. The word Algol comes from the Arabic for al-Ghul – the ghoul.
Ancient astronomers in Egypt and China studied Algol
Modern astronomers studying Algol believe the Demon Star has a macabre habit to match its moniker. You see Algol’s a multiple star system composed of one star in the act of consuming the outer layers of the other. According to theory, two such stars in close proximity should be interacting
Modern astronomers have been studying Algol’s periodic blinking every few days, since sometime in the 17th century. In 1783, a young astronomer called John Goodricke sent a letter to the Royal Society of London suggesting this blinking could be due to a darker body passing in front of a star. It wasn’t until 1881 that University of Harvard astronomer Edward Dickering confirmed Algol has more than one sun. In fact, around 1912 a team of astronomers in Helsinki determined Algol has a brilliant blue star and bloated red star orbiting periodically close together, with a third star orbiting the pair at a distance.
Modern astronomers studied the Demon Star
The periodic blinking of the Demon Star occurs when the red bloated star passes in front of the blue star, merging the pair into a single point of light, which accounts for Algol turning blood red, before turning blue again around 10 hours later.
Click this link to watch a YouTube documentary on Algol. The documentary is a mix of different videos on the dying star, which the site has put into one show. Pretty cool stuff.
Understanding how large star clusters form could tell us more about star formation when the universe was young
Astronomers news (2013-10-14) – Tonight we’ll journey to the truly titanic 30 Doradus nebula (also called the Tarantula nebula), 170 light-years away in the Large Magellanic Cloud, aboard the Hubble Space Telescope. The Large Magellanic Cloud is a smaller satellite galaxy to the Milky Way, where astronomers recently discovered something they suspected about the formation of larger star clusters.
Using Hubble’s Wide Field Camera 3, we’ll be able to look at images of the Tarantula nebula filled with startling reds, greens and blues, which indicates to astronomers the elemental composition of the stars in the region. Blue light is from the hottest, most massive stars astronomers have found to date. Red light is from fluorescing hydrogen gas, while green light is the glow of oxygen.
Every element on the periodic table gives off light with a specific signature upon fluorescing. Scientists use this knowledge to analyze the light reaching Hubble’s Wide Field Camera 3 from the Tarantula nebula to determine the elemental composition of the stars in the region .They hope to use this knowledge to answer questions they have concerning star formation when the universe was still in its infancy.
NASA astronomers see something different going on in 30 Doradus
We’ll specifically journey to a region of the 30 Doradus nebula where astronomers recently discovered a pair of star clusters which they first thought was a single star cluster, is in fact a pair of star clusters in the initial stages of merging into a larger star cluster. Astronomers now think the merging of star clusters could help explain the abundance of large star clusters throughout the visible universe.
Lead scientist Elena Sabbi of the Space Telescope Science Institute in Baltimore, Maryland and her team first started looking at the region to find runaway stars. Runaway stars are fast-moving stars that have been kicked out of the stellar nursery where they first formed. Astronomers found the region surrounding 30 Doradus has a large number of runaway stars, which according to current star formation theories could not have formed at their present location. Astronomers now believe the runaway stars outside 30 Doradus could have been ejected out of the region at high speed due to dynamic interactions with other stellar bodies as the two star clusters merge into one larger star cluster.
Astrophysicists and astronomers started looking for clues
The first clue to the true nature of the event astronomers were viewing was the fact that parts of the star cluster varied in age by about 1 million years. Upon further study the team noticed the distribution of low-mass stars detected by Hubble were not spherical in shape as astronomers expected, but resembled the elongated shape of two merging galaxies. Now astronomers are studying this region of space and time to find clues to help them understand the way larger star clusters are formed in the universe. They also hope this discovery will help determine interesting and enlightening facts concerning the formation of star clusters when the universe was still young.
Astronomers are also looking further at this region of space and time to find other star clusters in the process of merging in the 30 Doradus nebula. They plan on using the ability of the James Webb Space Telescope to detect infrared light , once it comes on line, to take a closer look at areas within the Tarantula nebula where they think stars hidden within cocoons of dust are blocked from the view of telescopes and instruments detecting visible light.
Stars begin life as clouds of cold gas and dust that transform into blazing hot fireballs
Star dust, star dust, burning bright
Amid the glare of ancient light
Eternity stares back from the past
Reborn we’ll be one day at last
NASA astronomy: stellar astrophysics
Astronomy questions and answers – September 19, 2013 – Walk out to a dark viewing spot anywhere on the Earth on a clear night and look up at the night sky. Your eyes will take in ancient light from stars in the Milky Way that covers the whole sky above you. Deep within the stellar nurseries of the Milky Way new stars are being formed using processes NASA astronomers are currently studying in an attempt to understand how stars are born. Star forming processes responsible for the formation of the stars you see in the night sky. Processes they can see at work in the stellar nurseries of the Milky Way, like the Orion Nebula (M42) and Cygnus X.
Journey with me to stellar nurseries deep within the dark regions of the Milky Way, the dark patches you can see in the night sky above. The birthing grounds of young stars in the Milky Way, these dark patches in the night sky are in fact clouds of interstellar gas that appear dark because they block the starlight from distant stars. Astronomers believe deep within the birthing grounds of the Milky Way, new stars are being formed at the rate of about 2 or 3 new stars each year.
Star formation theories
Present theories on star formation put forth by NASA astronomers show star formation is a complicated process affected by nearby massive stars, other star forming regions, and even the spiral structure of the Milky Way. These theories only become more complicated when astronomers look at the formation of groups of stars.
In order to try to simulate star formation, some astronomers use sophisticated computer models, while others incorporate observations in different wavelengths and use them to create three-dimensional images of the sky. Working together these two different groups of astronomers are trying to determine exactly how stars are born.
NASA astronomers working on present theories of star formation think the Milky Way is filled with clouds of gas and dust they call the interstellar medium. They also think slight over densities within these clouds of gas and dust could trigger star formation, over densities that could be produced by the turbulent forces present in these clouds of gas and dust. Astronomers studying slight over densities within star forming clouds of gas and dust believe these slightly denser regions could eventually become main sequence stars within a few million years.
Some NASA astronomers believe the intense radiation from groups of hot, bright stars located close to one another could create the necessary turbulence in the interstellar medium to trigger star formation. Other astronomers believe nearby galaxies and even large clouds of gas and dust could cause turbulence in the interstellar medium which could also be part of the star forming process. Many astronomers also believe the resulting shock wave after a supernova could create spiral density waves capable of compressing material and initiating star formation.
Gravity at Work
Present theories on the formation of main sequence stars being proposed by NASA astronomers involves the force of gravity. Gravity pulls the gas and dust within the interstellar medium into denser regions, which results in a cloud increasing in size and contracting. The rotation velocity of the cloud increases as it contracts due to conservation of angular momentum, in the same way a figure skater’s spin speed increases as they bring their arms closer to their body.
At the same time the temperature in the core of the cloud increases as it shrinks due to the force of gravity. The charged particles within the cloud at this time can only move in specific directions in the magnetic field in the region. This results in the rotational velocity of the cloud slowing, but not stopping, otherwise astronomers think stars would never form in these dense clouds of gas and dust.
In the case of main sequence stars astronomers think regions of dense clouds of gas and dust would begin to contract to an area the size of our solar system tens of thousands of years after beginning to slow. At this time astronomers think the temperature at the centre of dense clouds of dust and gas would be in the region of 10,000 kelvins. They call the central region of such a cloud at this time a protostar.
Protostars at this time in their life cycle are often more luminous than the main sequence star they eventually become, because they have a greater surface from which to radiate energy. This brightness allows NASA astronomers to view protostars as they continue to gravitationally attract more gas and dust, shrink and heat up internally. The luminosity of a protostar begins to decrease as it’s outer surface shrinks under the force of gravity. Astronomers believe the cloud and protostar eventually spin faster and flatten out into a disk.
Astronomers using data collected by several different astronomical instruments recently presented far-infrared images of three Class 0 protostar systems in Perseus: L1448C, the triple system L1448N, and IRAS 03282+3035. Seven hundred and fifty light-years from Earth, all three of these protostars were seen powering bipolar molecular outflows, which astronomers think are in fact epic jets of water being thrust into interstellar space. Calculations by NASA astronomers indicates these jets of water are shooting out into interstellar space at speeds of around 120,000 miles per hour and at a rate equal to about 100 million times the volume of water flowing in the Amazon every second of the day.
Astronomers think these jets of water and material help to channel radiation and mass away from the protostar, which helps to clear the central region of debris and reveal the protostar. They also think it could be possible the galaxy was seeded with water through this process, which might change thoughts on the possibility of life in the galaxy. The remaining material is then accreted by the protostar, or forms part of a residual disk, which NASA astronomers think could form planets.
The core of a protostar will reach 1 million kelvin at sometime during the contraction and heating up of the cloud, at which time it will begin fusing deuterium to helium. Deuterium is the easiest nucleus to fuse, so it makes sense this would be the starting point. Once the core has contracted enough to reach a density where the core reaches 10 million degrees kelvins, hydrogen nuclei will begin fusing into helium. At this point star astronomers also think a protostar will reach an equilibrium point where the radiative energy from fusion balances gravitational pull of its mass. This new star is now a main sequence star, which has formed over millions of years.
Simulating the Birth of a Star
The process of star birth takes millions of years to complete, so how do astronomers determine the way outside factors affect the process by which new stars are born? Modern astronomers are presently using supercomputers to help simulate star formation models in the hope they can determine why the mass distribution of newly formed stars appears to be universal. They want to understand why this average mass of newly formed stars exists. They also want to know the process by which it occurs.
Present star formation models take into account the effects of thermodynamics, magnetic fields, radiative processes, and of course gravity. Star astronomers are also trying to determine other factors they need to include in models, like the way new stars affect their own star forming environments. This includes factors like young stars heating up the gas and dust surrounding them and moving gas and dust around through bipolar molecular flows.
The key question NASA astronomers want to answer at this point is whether or not present star formation models can reproduce the properties of exact parts of the star forming process. Astronomers will also want to determine the most massive star that can be formed depending on the size of a cloud of dust and gas. They’ll try to find answers by looking at the chemical composition, magnetic fields, ionization, age and other factors of large clouds of star forming dust and gas in the night sky.
Peering into Stellar Nurseries
How do NASA astronomers look into the heart of stellar nurseries in the Milky Way? Astronomers use instruments designed to detect specific wavelengths of light radiation emitted during the formation of new stars. During the beginning stages of star birth a new star emits radio waves as it contracts astronomers look for as an indicator of new star formation. At this time the core of a contracting cloud of gas and dust is too cold to emit visible and infrared radiation.
Once the cloud forms a protostar it will begin to emit light radiation, which will be blocked by the material surrounding the new star. The light radiation emitted by a protostar is absorbed by the surrounding material, which radiates infrared radiation toward Earth NASA astronomers detect using space and ground-based telescopes specifically designed for the job.
Astronomers have used the Spitzer Space Telescope to view hundreds of protostars forming in large clouds of gas and dust in the stellar nurseries of the Milky Way. In the future they’ll use instruments and telescopes designed to detect millimetre waves in the microwave range in order to get a better view of the beginning stages of star birth. To date astronomers report detecting a compact source embedded in cold gas within stellar nurseries only detectable at these wavelengths.
NASA astronomers trying to piece together the puzzle of star formation in the Milky Way are also using reconstructed images of star-forming regions from past observations. Using 2-D images, positional data, and velocities for an entire cloud, they have been able to create 3-D models researchers can then analyze. 3-D models that show unforeseen structures hidden within stellar nurseries and even regions of star formation they weren’t expecting to see.
Click this link to watch a You Tube videos on how a star is born