Quasars and Pulsars

Quasars and Pulsars 

The word “quasar” refers to a “quasi-stellar radio source.” The first quasars were discovered in the 1960s when astronomers measured their very strong radio emissions. Later, scientists discovered that quasars are actually radio-quiet, with very little radio emission. However, quasars are some of the brightest and most distant objects we can see.

An artist’s rendering of the most distant quasar

An artist’s rendering of the most distant quasar

These ultra-bright objects are likely the centers of active galaxies where supermassive black holes reside. As material spirals into the black holes, a large part of the mass is converted to energy. It is this energy that we see. And though smaller than our solar system, a single quasar can outshine an entire galaxy of a hundred billion stars.

To date, astronomers have identified more than a thousand quasars.

Joining the dots:

from starburst to elliptical galaxies

Starburst galaxies appear in red. Credit: ESO, APEX (MPIfR/ESO/OSO), A. Weiss et al., Spitzer
Starburst galaxies appear in red. Credit: ESO, APEX (MPIfR/ESO/OSO), A. Weiss et al., Spitzer  
 

By Amanda Doyle at SEN

27 January 2012

(Sen) – Astronomers observing ancient starburst galaxies have made a connection between them and the elliptical galaxies we see today.

There are many different types of galaxies in the Universe and astronomers have long desired to join the dots and solve the puzzles of galaxy evolution. Looking at galaxies that are far, far away is also a way of looking back in time. Their light has taken billions of years to reach us, and thus we see those galaxies as they were billions of years ago. Galaxies in the ancient Universe are often very different than the host of spiral and elliptical galaxies that we are surrounded by today. For example, the extremely bright quasars are common in the distant Universe and yet none exist locally.

However, astronomers using NASA’s Spitzer Space Telescope along with ESO’s Very Large Telescope and 12 metre Atacama Pathfinder Experiment (APEX) telescope have managed to see how distant submillimetre galaxies, quasars, and modern elliptical galaxies fit together in the jigsaw of the Universe.

Sub~millimetre galaxies (SMGs) are situated 10 billion light years from us, and are extremely bright in the infrared region of the spectrum, specifically the submillimetre band. Because the SMGs are located so far away, the light emitted by the galaxies is shifted to much longer wavelengths. These galaxies are also starburst galaxies, meaning that for a short while there is a phenomenal rate of star formation. A supernova explosion would occur every few years and on a planet in a starburst galaxy the night sky would be almost as bright as day.

Astronomers have been able to measure the mass of the dark matter halos surrounding a group of SMGs. Dark matter is invisible and we don’t know what it is, but indirect detections tells us that galaxies are usually engulfed in it. The dark matter typically extends far beyond the edge of the visible galaxy. But measuring the mass of dark matter halos 10 billion light years away is no easy task. Ryan Hickox, lead author of the paper on the subject, explains to Sen how this was done.

“We measure how strongly the galaxies are clustered together in space, using a statistical tool called a ‘correlation function’. If the galaxies were distributed randomly, the correlation function would be equal to zero. However if they are clustered together (sort of like buildings in towns and cities) then they have a positive correlation function. We know from simulations of the Universe how halos of dark matter are clustered together, and this clustering depends strongly on the mass of the halos. Galaxies that live in these halos will be clustered the same way. So by measuring the clustering of the galaxies, we can tell how massive the typical halos that host them are.”

By knowing the mass of the halos of the SMGs, Hickox and his colleagues were able to use computer simulations to fast forward to the present day and show that these galaxies will eventually form giant elliptical galaxies in the modern Universe. However, elliptical galaxies are typically devoid of star formation. So what stopped the immense star formation in the SMGs? Continue Reading

Quasars

Light that is bent by a galaxy can be used to measure the galaxy’s mass. Credit: Joerg Colberg, Ryan Scranton, Robert Lupton, SDSS
Light that is bent by a galaxy can be used to measure the galaxy’s mass. Credit: Joerg Colberg, Ryan Scranton, Robert Lupton, SDSS  

By Amanda Doyle at SEN

14 February 2012

Researchers have used advanced computer simulations to show that the space between galaxies is teeming with dark matter.

Everything that we can see around us in the Universe only makes up around 4.5 per cent of the total mass of the Universe. The remaining “missing mass” is made up of dark matter and dark energy, and the origin of both of these is still a mystery.

While dark matter cannot be directly detected, its presence can be inferred from an effect known as gravitational lensing. Light from a distant object, such as a quasar, is bent around a foreground galaxy so that the light from the quasar becomes distorted. The way in which the light is bent depends on the mass of the “lens” galaxy.

The image on the left shows a simulation of how light from distant sources should appear if there is no intervening “lens,” while the image on the right shows how light can be distorted when there is a galaxy between us and the distant light sources.

However the mass of galaxies is usually much greater than what is expected from looking at the amount of matter that is visible. It has been known for some time that large dark matter halos exist around galaxies, which stretch up to 100 million light years from the centre of the galaxies.

New computer simulations now show that the dark matter does not end at 100 million light years, but instead knows no boundaries as it extends into intergalactic space.  Continue Reading

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Ancient Galaxy Cluster Still Producing Stars

Black hole quasar NASA

Space dot Com Video

Astronomers have found a quasar that’s more than five times more powerful than any previously seen. Quasars are mega-bright geysers of matter and energy powered by super-massive black holes at the centers of young galaxies.
Credit: SPACE.com / ESO

NGC 1132: A Mysterious Elliptical Galaxy (An e...

Quasars: Radio Stars 

from Sea and Sky

Quasars are the brightest and most distant objects in the known universe. In the early 1960’s, quasars were referred to as radio stars because they were discovered to be a strong source of radio waves. In fact, the term quasar comes from the words, “quasi-stellar radio source”. Today, many astronomers refer to these objects as quasi-stellar objects, or QSOs. As the resolution of our radio and optical telescopes became better, it was noticed that these were not true stars but some type of as yet unknown star-like objects. It also appeared that the radio emissions were coming from a pair of lobes surrounding these faint star-like objects. It was also discovered that these objects were located well outside our own galaxy. Quasars are very mysterious objects. Astronomers today are still not sure exactly what these objects are. What we do know about them is that they emit enormous amounts of energy. They can burn with the energy of a trillion suns. Some quasars are believed to be producing 10 to 100 times more energy than our entire galaxy. All of this energy seems to be produced in an area not much bigger than our solar system.

Distant Lights

We do know that quasars are extremely distant. In fact, they may be the most distant objects in the universe. They also have the largest red shift of any other objects in the cosmos. Astronomers are able to measure speed and distance of far away objects by measuring the spectrum of their light. If the colors of this spectrum are shifted toward the red, this means that the object is moving away from us. The greater the red shift, the farther the object and the faster it is moving. Since quasars have such a high red shift, they are extremely far away and are moving away from us at extremely high speeds. It is believed that some quasars may be moving away from us at 240,000 kilometers per second or nearly 80% the speed of light. Quasars are, in fact, the most distant objects to ever be detected in the universe. We know that light travels a certain distance in a year. Quasars are so far away that the light we see when we observe them has been traveling for billions of years to reach us. This means that quasars are among the most ancient objects known in the universe. The most distant quasars observed so far are over 10 billion light-years away. This means we are seeing them as they appeared 10 billion years ago. It is entirely possible that some or all of the quasars we see today may not even exist any more.

Peering back to the early Universe, Europe’s Very Large Telescope has found gas-filled galaxies that lacked the gravity dynamics to form stars. A long-sought faint fluorescent glow was detected, revealing these previously invisible objects.
Credit: ESO, Digitized Sky Survey 2, Akira Fujii/David Malin Images. Music: Disasterpeace

What is a Quasar

We still do not know exactly what a quasar is. But the most educated guess points to the possibility that quasars are produced by super massive black holes consuming matter in an acceleration disk. As the matter spins faster and faster, it heats up. The friction between all of the particles would give off enormous amounts of light other forms of radiation such as x-rays. The black hole would be devouring the equivalent mass of one Sun per year. As this matter is crushed out of existence by the black hole, enormous amounts of energy would be ejected along the black hole’s north and south poles. Astronomers refer to these formations as cosmic jets. Another possible explanation for quasars is that they are very young galaxies. Since we know very little about the evolutionary process of galaxies, it is possible that quasars, as old as they are, represent a very early stage in the formation of galaxies. The energy we see may be ejected from the cores of these very young and very active galaxies. Some scientists even believe that quasars are distant points in space where new matter may be entering our universe. This would make them the opposite of black holes. But this is only conjecture. It may be some time before we really understand these strange objects.

Finding Quasars

The first identified quasar was called 3C 273 and was located in the constellation Virgo. It was discovered by T. Matthews and A. Sandage in 1960. It appeared to be associated with a 16th magnitude star like object. Three years later, in 1963, It was noticed that the object had an extremely high red shift. The true nature of this object became apparent when astronomers discovered that the intense energy was being produced in a relatively small area. Today, quasars are identified primarily by their red shift. If an object is discovered to have a very high red shift and appears to be producing vast amounts of energy, it becomes a prime candidate for quasar research. Today more than 2000 quasars have been identified. The Hubble space telescope has been a key tool in the search for these elusive objects. As technology continues to enhance our windows to the universe, we may one day fully understand these fantastic lights

Pulsars

Cosmic Beacons

Pulsars are among the strangest objects in the universe. In 1967, at the Cambridge Observatory, Jocelyn Bell and Anthony Hewish were studying the stars when they stumbled on something quite extraordinary. It was a star-like object that seemed to be emitting quick pulses of radio waves. Radio sources had been known to exist in space for quite some time. But this was the first time anything had been observed to give off such quick pulses. They were as regular as clockwork, pulsing once every second. The signal was originally thought to be coming from an orbiting satellite, but that idea was quickly disproved. After several more of these objects had been found, they were named pulsars because of their rapidly pulsing nature. Bright pulsars have been observed at almost every wavelength of light. Some can actually be seen in visible light. Many people tend to get pulsars confused with quasars. But the two objects are totally different. Quasars are objects that produce enormous amounts of energy and may be the result of a massive black hole at the center of a young galaxy. But a pulsar is a different animal entirely.

Alien worlds that orbit the energetic dead stars known as pulsars may leave electric currents behind them – anomalies that could help researchers find more of these strange planets.

Astronomers know of only four “pulsar planets” so far, and much remains unknown about such worlds, but scientists propose that they formed in the chaos after the supernova explosions that gave birth to the pulsars.

pulsar is a kind of neutron star, a stellar corpse left over from a supernova, a giant star explosion that crushes protons with electrons to form neutrons. Neutron star matter is the densest known material: A sugar cube-size piece weighs as much as a mountain, about 100 million tons. The mass of a single neutron star surpasses that of the sun while fitting into a ball smaller in diameter than the city of London.

The Lighthouse Factor

A pulsar is basically a rapidly spinning neutron star. A neutron star is the highly compacted core of a dead star, left behind in a supernova explosion. This neutron star has a powerful magnetic field. In fact, this magnetic field is about one trillion times as powerful as the magnetic field of the Earth. The magnetic field causes the neutron star to emit strong radio waves and radioactive particles from its north and south poles. These particles can include a variety of radiation, including visible light. Pulsars that emit powerful gamma rays are known as gamma ray pulsars. If the neutron star happens to be aligned so that the poles face the Earth, we see the radio waves every time one of the poles rotates into our line of sight. It is a similar effect as that of a lighthouse. As the lighthouse rotates, its light appears to a stationary observer to blink on and off. In the same way, the pulsar appears to be blinking as its rotating poles sweep past the Earth. Different pulsars pulse at different rates, depending on the size and mass of the neutron star. Sometimes a pulsar may have a binary companion. In some cases, the pulsar may begin to draw in matter from this companion. this can cause the pulsar to rotate even faster. The fastest pulsars can pulse at well over a hundred times a second

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Quasar

Quasar

From @Spacedotcom >

The Nine Most Brilliant Comets Ever Seen

And a History of Comets

Excitement is riding high in the astronomical community with the recent discovery of Comet ISON, which is destined to pass exceedingly close to the sun in late November 2013 and might possibly become dazzlingly bright.

The latest information issued by NASA’s Jet Propulsion Laboratory suggests that this comet could get as bright as magnitude -11.6 on the astronomers’ brightness scale; that’s as bright as nearly full moon!  That would also be bright enough for Comet ISON to be visible during the daytime.

Comets that are visible to the naked eye during the daytime are rare, but such cases are not unique.  In the last 332 years, it has happened only nine other times.  Here is a listing of past comets that have achieved this amazing feat.

In this list we quote the brightness of the comets in terms of magnitude.  On this scale, larger numbers represent dimmer objects; the brightest stars are generally zero to first magnitude, while super-bright objects such as Venus and the moon achieve negative magnitudes. [Spectacular Comet Photos (Gallery)]

Great Comet of 1680 —This comet has an orbit strikingly similar to Comet ISON, begging the question of whether both objects are one and the same or at the very least are somehow related.  Discovered on Nov. 14, 1680 by German astronomer Gottfried Kirsch, this was the first telescopic comet discovery in history. By Dec. 4, the comet was visible at magnitude +2 with a tail 15 degrees long.  On Dec. 18 it arrived at perihelion — its closest approach to the sun — at a distance of 744,000 miles (1.2 million kilometers).

A report from Albany, N.Y. indicated that it could be glimpsed in daylight passing above the sun.  In late December, it reappeared in the western evening sky, again of magnitude +2, and displaying a long tail that resembled a narrow beam of light that stretched for at least 70 degrees. The comet faded from naked-eye visibility by early February 1681.

Great Comet of 1744 — First sighted on Nov. 29, 1743 as a dim 4th-magnitude object, this comet brightened rapidly as it approached the sun.  Many textbooks often cite Philippe Loys de Cheseaux, of Lausanne, Switzerland as the discoverer, although his first sighting did not come until two weeks later.  By mid-January 1744, the comet was described as 1st-magnitude with a 7-degree tail.

By Feb. 1 it rivaled the star Sirius in brightness and displayed a curved tail 15 degrees in length.  By Feb. 18 the comet was as bright as Venus and now displayed two tails.  On Feb. 27, it peaked at magnitude -7 and was reported visible in the daytime, 12 degrees from the sun.  Perihelion came on March 1, at a distance of 20.5 million miles (33 million km) from the sun.  On March 6, the comet appeared in the morning sky, accompanied by six brilliant tails that resembled a Japanese hand fan.

Great Comet of 1843 — This comet was a member of the Kruetz Sungrazing Comet Group, which has produced some of the most brilliant comets in recorded history. Such comets actually graze through the outer atmosphere of the sun, and often do not survive.

The 1843 comet passed only 126,000 miles (203,000 km) from the sun’s photosphere on Feb 27, 1843.  Although a few observations suggest that it was seen for a few weeks prior to this date, on the day when of its closest approach to the sun it was widely observed in full daylight.  Positioned only 1 degree from the sun, this comet appeared as “an elongated white cloud” possessing a brilliant nucleus and a tail about 1 degree in length.  Passengers onboard the ship Owen Glendower, off the Cape of Good Hope described it as a “short, dagger-like object” that closely followed the sun toward the western horizon.

In the days that followed, as the comet moved away from the sun, it diminished in brightness but its tail grew enormously, eventually attaining a length of 200 million miles (320 million km). If you were able to place the head of this comet at the sun’s position, the tail would have extended beyond the orbit of the planet Mars!

The great comet of 1881 by Trouvelot
A chromolithograph of the great comet of 1881 by Trouvelot
CREDIT: E.L. Trouvelot/NYPL
View full size image and Story at Space.com

Great September Comet of 1882 — This comet is perhaps the brightest comet that has ever been seen; a gigantic member of the Kreutz Sungrazing Group.  First spotted as a bright zero-magnitude object by a group of Italian sailors in the Southern Hemisphere on Sept.1, this comet brightened dramatically as it approached its rendezvous with the sun.

By Sept. 14, it became visible in broad daylight and when it arrived at perihelion on the 17th, it passed at a distance of only 264,000 miles (425,000 km) from the sun’s surface.  On that day, some observers described the comet’s silvery radiance as scarcely fainter than the limb of the sun, suggesting a magnitude somewhere between -15 and -20!

The following day, observers in Cordoba, Spain described the comet as a “blazing star” near the sun.  The nucleus also broke into at least four separate parts. In the days and weeks that followed, the comet became visible in the morning sky as an immense object sporting a brilliant tail.  Today, some comet historians consider it as a “Super Comet,” far above the run of even Great Comets.

Great January Comet of 1910 — The first people to see this comet —  then already at first magnitude —  were workmen at the Transvaal Premier Diamond Mine in South Africa on Jan. 13, 1910.  Two days later, three men at a railway station in nearby Kopjes casually watched the object for 20 minutes before sunrise, assuming that it was Halley’s Comet.

Later that morning, the editor of the local Johannesburg newspaper telephoned the Transvaal Observatory for a comment.  The observatory’s director, Robert Innes, must have initially thought this sighting was a mistake, since Halley’s Comet was not in that part of the sky and nowhere near as conspicuous. Innes looked for the comet the following morning, but clouds thwarted his view.  However, on the morning of Jan. 17, he and an assistant saw the comet, shining sedately on the horizon just above where the sun was about to rise.  Later, at midday, Innes viewed it as a snowy-white object, brighter than Venus, several degrees from the sun.  He sent out a telegram alerting the world to expect “Drake’s Comet” —  for so “Great Comet” sounded to the telegraph operator.

It was visible during the daytime for a couple more days, then moved northward and away from the sun, becoming a stupendous object in the evening sky for the rest of January in the Northern Hemisphere. Ironically, many people in 1910 who thought they had seen Halley’s Comet instead likely saw the Great January Comet that appeared about three months before Halley. [Photos of Halley’s Comet Through History]

Comet Skjellerup-Maristanny, 1927 —Another brilliant comet, first seen as a 3rd magnitude object in early December 1927, had the unfortunate distinction of arriving under the poorest observing circumstances possible.  The orbital geometry was such that the approaching comet could not be seen in a dark sky at any time from either the Northern or the Southern Hemisphere.

Nonetheless, the comet reached tremendous magnitude at perihelion on Dec. 18.  Located at a distance of 16.7 million miles (26.9 million km) from the sun, it was visible in daylight about 5 degrees from the sun at a magnitude of -6.  As the comet moved out of the twilight and headed south into darker skies, it faded rapidly, but still threw off an impressively long tail that reached up to 40 degrees in length by the end of the month.

40 Years Ago: A Great Comet

This painting of Comet Ikeya-Seki, visible during the day, was done by now-retired Hayden Planetarium artist Helmut K. Wimmer and was based on a description made by Hayden’s Chief Astronomer, Ken Franklin, from an airplane hovering over West Point, New York. It was originally published in the February 1966 issue of Natural History magazine. Republished with permission.

Comet Ikeya-Seki, 1965 — This was the brightest comet of the 20th century, and was found just over a month before it made perihelion passage in the morning sky, moving rapidly toward the sun.

Like the Great Comets of 1843 and 1882, Ikeya-Seki was a Kreutz Sungrazer, and on Oct. 21, 1965, it swept within 744,000 miles (1.2 million km) of the center of the sun.  The comet was then visible as a brilliant object within a degree or two of the sun, and wherever the sky was clear, the comet could be seen by observers merely by blocking out the sun with their hands.

From Japan, the homeland of the observers who discovered it, Ikeya-Seki was described as appearing “ten times brighter than the full moon,” corresponding to a magnitude of -15. Also at that time, the comet’s nucleus was observed to break into two or three pieces.  Thereafter, the comet moved away in full retreat from the sun, its head fading very rapidly but its slender, twisted tail reaching out into space for up to 75 million miles (120 million km), and dominating the eastern morning sky right on through the month of November.

Comet West, 1976 — This comet developed into a beautiful object in the morning sky of early March 1976 for Northern Hemisphere observers.  It was discovered in November 1975 by Danish astronomer Richard West in photographs taken at the European Southern Observatory in Chile. Seventeen hours after passing within 18.3 million miles (29.5 million km) of the sun on Feb. 25, 1976, it was glimpsed with the naked eye 10 minutes before sunset by John Bortle.

In the days that followed, Comet West displayed a brilliant head and a long, strongly structured tail that resembled “a fantastic fountain of light.”  Sadly, having been “burned” by the poor performance of Comet Kohoutek two years earlier, the mainstream media all but ignored Comet West, so most people unfortunately failed to see its dazzling performance.

New Comet is Brightest in 30 Years

Michael Jager and Gerald Rhemann photographed comet C/2006 P1 (McNaught) from Austria in twilight 45 minutes before sunrise on Jan. 3. Rhemann told SPACE.com they used 7×50 binoculars to find the comet. They estimate that today (Jan. 5) it shone at magnitude +1 and they expect to see it with the naked eye next week. 

Comet McNaught, 2007 —Discovered in August 2006 by astronomer Robert McNaught at Australia’s Siding Spring Observatory, this comet evolved into a brilliant object as it swept past the sun on Jan. 12, 2007 at a distance of just 15.9 million miles (25.6 million km).  According to reports received from a worldwide audience at the International Comet Quarterly, it appears that the comet reached peak brightness on Sunday, Jan. 14 at around 12 hours UT (7:00 a.m. EST, or 1200 GMT).  At that time, the comet was shining at magnitude 5.1.

Some observers, such as Steve O’Meara, located at Volcano, Hawaii, observed McNaught in daylight and estimated a magnitude as high as -6, noting, “The comet appeared much brighter than Venus!”

After passing the sun, Comet McNaught developed a stupendously large, fan-shaped tail somewhat reminiscent of the Great Comet of 1744. Unfortunately for Northern Hemisphere observers, the best views of Comet McNaught were mainly from south of the equator.

Joe Rao serves as an instructor and guest lecturer at New York’s Hayden Planetarium. He writes about astronomy for The New York Times and other publications, and he is also an on-camera meteorologist for News 12 Westchester, New York.

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Universe Feature and Star Map of the Galaxy

European Southern Observatory

17 December 2012: Astronomers from around the world have been meeting in Chile to discuss the exciting first year of scientific results from the Atacama Large Millimeter/submillimeter Array (ALMA) telescope. ALMA started Early Science operations at the end of September 2011, and the first scientific papers have recently been appearing in refereed journals. …   Read more

This VLT image of the Thor’s Helmet Nebula was taken on the occasion of ESO’s 50th Anniversary, 5 October 2012

This VLT image of the Thor’s Helmet Nebula was taken on the occasion of ESO’s 50th Anniversary, 5 October 2012

12 December 2012: A video compilation of time-lapse footage of the Atacama Large Millimeter/submillimeter Array (ALMA) is now available. The video is a collection of time-lapse shots of the ALMA site in the Atacama Desert of northern Chile, showing the synchronised dance of the array’s antennas as they observe the clear night sky …      Read more

Current Playlist from ESO

Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole.

Colour composite image of Centaurus A, revealing the lobes and jets emanating from the active galaxy’s central black hole.

The following image via ESO is a composite image of the brown dwarf object 2M1207 (centre) Picture also links to ESO’s current Star Images.  The fainter object seen near it, at an angular distance of 778 milliarcsec. Designated “Giant Planet Candidate Companion” by the discoverers, it may represent the first image of an exoplanet. read more

a brown dwarf

From NASA Oct 2012

The interstellar boundary region shields our solar system from most of the dangerous galactic cosmic radiation that otherwise would enter the solar system from interstellar space.

› Link to Media Advisory

› Link to Press Release

› Link to Feature Story

› Link to Presenter Bios

› Link to Associated Media

IBEX Full Sky Map 01.31.2012 via NASA

Color-coded full sky neutral atom map, as obtained with IBEX at energies where the interstellar wind is the brightest feature in the maps. In Earth’s orbit, where IBEX makes its observations, the maximum flow (in red) is seen to arrive from Libra instead of Scorpio because the interstellar wind is forced to curve around the Sun by gravity. Credit: NASA/Goddard/UNH

› Link to associated news item

2 Articles From New Scientist

20 December 2012

by Lisa Grossman at New Scientist (< full story link)

We’re about to get a better grasp of one of the biggest ideas in the universe:inflation. The first maps of the cosmos from the European Space Agency’s Planck satellite are due out in early 2013. They should help us to hone descriptions of how, after the big bang, the universe grew from smaller than a proton into a vast expanse in less than a trillionth of a trillionth of a second.

The early universe was a featureless soup of hot plasma that somehow grew into the dense galaxy clusters and cosmic voids we know today. On a large scale, regions far apart from each other should look very different, according to the laws of thermodynamics. But studies of the cosmic microwave background (CMB) – the first light to be released, some 300,000 years after the big bang – show that the universe still looks virtually the same in all directions.

Best ever map of the early universe

From 2006  by  Stephen Battersby

And the new evidence agrees that the universe went through a traumatic growth spurt before it was a billionth of a billionth of a second old

The universe went through a traumatic growth spurt before it was a billionth of a billionth of a second old, according to the latest data from the Wilkinson Microwave Anisotropy Probe (WMAP).

The probe has also given physicists their first clues about what drove that frantic expansion, and revealed that the cosmic “dark age” before the first stars switched on was twice as long as previously thought.

On Thursday, the WMAP team revealed the best map ever drawn of microwaves from the early universe, showing variations in the brightness of radiation from primordial matter. The pattern of these variations fits the predictions of a physical theory called inflation, which suggests that during the first split second of existence the universe expanded incredibly fast.

The variations in the density of matter that the microwave map shows up were created by quantum fluctuations during the expansion, according to the theory. If so, then those fluctuations provided the seeds for the gravitational growth of galaxies and stars – without inflation the universe would still be a featureless cloud of gas.

^^

(Image: NASA/WMAP Science Team)

(Image: NASA/WMAP Science Team)

The white bars on this new, more detailed map of the infant universe show the polarisation direction of the oldest light, which provides clues about events in the first trillionth of a second of the universe (Image: NASA/WMAP Science Team)

new map

The latest (in 2006) WMAP data supports the idea of rapid inflation at the universe’s birth followed by much more gradual expansion

WMAP Team Releases Final Results, Based on Nine Years of Observations

Since its launch in 2001, the Wilkinson Microwave Anisotropy Probe (WMAP) space mission has revolutionized our view of the universe, establishing a cosmological model that explains a widely diverse collection of astronomical observations. Led by Johns Hopkins astrophysicist Charles L. Bennett, the WMAP science team has determined, to a high degree of accuracy and precision, not only the age of the universe, but also the density of atoms; the density of all other non-atomic matter; the epoch when the first stars started to shine; the “lumpiness” of the universe, and how that “lumpiness” depends on scale size.

In short, when used alone (with no other measurements), WMAP observations have made our knowledge of those six parameters above about 68,000 times more precise, thereby converting cosmology from a field of often wild speculation to a precision science.

Now, two years after the probe “retired,” Bennett and the WMAP science team are releasing its final results, based on a full nine years of observations.

“It is almost miraculous, says Bennett, Alumni Centennial Professor of Physics and Astronomy and Johns Hopkins Gilman Scholar at the Johns Hopkins University’s Krieger School of Arts and Sciences. “The universe encoded its autobiography in the microwave patterns we observe across the whole sky. When we decoded it, the universe revealed its history and contents. It is stunning to see everything fall into place.”

WMAP’s “baby picture of the universe” maps the afterglow of the hot, young universe at a time when it was only 375,000 years old, when it was a tiny fraction of its current age of 13.77 billion years. The patterns in this baby picture were used to limit what could have possibly happened earlier, and what happened in the billions of year since that early time. The (mis-named) “big bang” framework of cosmology, which posits that the young universe was hot and dense, and has been expanding and cooling ever since, is now solidly supported, according to WMAP.

WMAP observations also support an add-on to the big bang framework to account for the earliest moments of the universe. Called “inflation,” the theory says that the universe underwent a dramatic early period of expansion, growing by more than a trillion trillion-fold in less than a trillionth of a trillionth of a second. Tiny fluctuations were generated during this expansion that eventually grew to form galaxies.

Remarkably, WMAP’s precision measurement of the properties of the fluctuations has confirmed specific predictions of the simplest version of inflation:  the fluctuations follow a bell curve with the same properties across the sky, and there are equal numbers of hot and cold spots on the map. WMAP also confirms the  predictions that the amplitude of the variations in the density of the universe on big scales should be slightly larger than smaller scales, and that the universe should obey the rules of Euclidean geometry so the sum of the interior angles of a triangle add to 180 degrees.

Recently, Stephen Hawking commented in New Scientist that WMAP’s evidence for inflation was the most exciting development in physics during his career.

The universe comprises only 4.6 percent atoms. A much greater fraction, 24 percent of the universe, is a different kind of matter that has gravity but does not emit any light — called “dark matter”. The biggest fraction of the current composition of the universe, 71%, is a source of anti-gravity (sometimes called “dark energy”) that is driving an acceleration of the expansion of the universe.

“WMAP observations form the cornerstone of the standard model of cosmology, “says Gary F. Hinshaw of the University of British Columbia, who is part of the WMAP science team. “Other data are consistent and when combined we now know precise values for the history, composition, and geometry of the universe.”

WMAP has also provided the timing of epoch when the first stars began to shine, when the universe was about 400 million old.  The upcoming James Webb Space Telescope is specifically designed to study that period that has added its signature to the WMAP observations.

WMAP launched on June 30, 2001 and maneuvered to its observing station near the “second Lagrange point” of the Earth-Sun system, a million miles from Earth in the direction opposite the sun. From there, WMAP scanned the heavens, mapping out tiny temperature fluctuations across the full sky.  The first results were issued in February 2003, with major updates in 2005, 2007, 2009, 2011, and now this final release. The mission was selected by NASA in 1996, the result of an open competition held in 1995. It was confirmed for development in 1997 and was built and ready for launch only four years later, on-schedule and on-budget.

“The last word from WMAP marks the end of the beginning in our quest to understand the Universe,” comments fellow Johns Hopkins astrophysicist Adam G. Riess, whose discovery of dark energy led him to share the 2011 Nobel Prize in Physics. “WMAP has brought precision to cosmology and the Universe will never be the same.”

“WMAP has brought precision to cosmology and the Universe will never be the same.”

Related links:

Bennett’s webpage

Hinshaw’s webpage 

Hawking on WMAP

ALL BELOW LINKS from JOHN HOPKINS UNIVERSITY Related>

December 21, 2012 Tags: 

Posted in Academic DisciplinesHomewood Campus NewsInstitutional NewsPhysics and AstronomyUniversity-Related

All Credits to John Hopkins University, NASA and New Scientists Author’s at all above links
This colour image of the region known as NGC 2264 — an area of sky that includes the sparkling blue baubles of the Christmas Tree star cluster and the Cone Nebula

This colour image of the region known as NGC 2264 — an area of sky that includes the sparkling blue baubles of the Christmas Tree star cluster and the Cone Nebula

Planck Science Team Home

2nd announcement of ESLAB 2013 – The Universe as seen by Planck: An international conference dedicated to an in-depth look at the initial scientific results from the Planck mission. ESA/ESTEC, Noordwijk, The Netherlands, 2-5 April 2013. For more information, please visit http://congrexprojects.com/13a11.

Hubble sees back to the cosmic dawn

by Jenny Winder

(Sen) – Astronomers using the Hubble Space Telescope have discovered a population of six previously unseen galaxies that formed 13 billion years ago. They also refined the distance of a seventh galaxy, identified as UDFj-39546284, as the most distant galaxy on record, which we are seeing as it was when the universe was only 380 million years old, less than 3% of its current age. That is further back in time than any object seen before.

The survey of a part of the sky called the Ultra Deep Field (UDF) has given scientists the first robust sample of galaxies that show how abundant they were in the era when galaxies first formed, and support the theory that galaxies assembled continuously over time and could have provided enough radiation to reionize the universe just a few hundred million years after the big bang.

Planck spots hot gas bridging galaxy cluster pair

by Sarah Cruddas

(Sen) – The European Space Agency’s Planck telescope has detected a bridge of hot gas connecting a pair of galaxy clusters. It’s the first conclusive detection of hot gas connecting clusters and is measured across a distance of 10 million light years.

Illustration of the Planck spacecraft. Credit: ESA/C. Carreau

Illustration of the Planck spacecraft. Credit: ESA/C. Carreau

The finding is important because it shows the ability of Planck to probe galaxy clusters, examining their connection with the gas that permeates the entire Universe and from which all groups of galaxies formed.

According to ESA “this marks Planck’s first detection of inter-cluster gas using the SZ effect technique”. The SZ effect technique is named after the scientist Sunyaev–Zel’dovich, who discovered it. If the Cosmic Microwave Background light interacts with the hot gas permeating these huge cosmic structures, its energy distribution is modified in a characteristic way, known as the SZ effect.

In the past Planck has used the SZ effect to detect galaxy clusters, but it also provides a way to detect faint filaments of gas that might connect one cluster to another. At the very early stages of the universe, it’s believed that the cosmos was filled with filaments of gaseous matter, with clusters eventually forming in the densest areas.

Up until now much of this tenuous, filamentary gas has remained undetected. However astronomers expect that it could most likely be found between interacting galaxy clusters, where the filaments are compressed and heated up, making them easier to spot. read more at Sen >

Black Hole Outburst in Spiral Galaxy M83 (NASA...

Black Hole Outburst in Spiral Galaxy M83 (NASA, Chandra, Hubble, 04/30/12) (Photo credit: NASA’s Marshall Space Flight Center)

Black Hole Outburst in Spiral Galaxy M83 (NASA...

Black Hole Outburst in Spiral Galaxy M83 (NASA, Chandra, Hubble, 04/30/12) (Photo credit: NASA’s Marshall Space Flight Center)

Vega

Standing almost directly overhead around midnight on July nights is the brilliant bluish-white star, Vega, in the constellation of Lyra, the Harp.

It’s the fifth brightest star in the entire sky and the third brightest visible from mid-northern latitudes, behind Sirius and Arcturus. Also, as seen from mid-northern latitudes such as New York or Madrid, Vega goes below the horizon for only about seven hours a day, meaning that you can see it on any night of the year.

Look directly overhead to find the star Vega in the constellation Lyra. North is at the top of this sky map.
CREDIT: Starry Night Software

This sky map of Vega  shows how the star appears in relation to constellations and other stars.

Astronomers take a fresh look at Vega

Monday, 17 December 2012 by Stuart Gary at ABC

The star Vega is at least two hundred million years older than previously thought, according to a new study.

For thousands of years, scientists have been using Vega as an astronomical yardstick with which to compare other stars and galaxies, as well as develop computer models of stellar life cycles.

vega star

New studies have provided the most accurate estimate yet of the age of Vega, one of the nearest stars to our solar system (Source: NASA/JPL)

But now, new research led by associate professor John Monnier of the University of Michigan, has found Vega is spinning slower than originally estimated, meaning the star is also older.

Reporting in the Astrophysical Journal, Monnier and colleagues determined the star rotates once every 17 hours, rather than once every 12, as previously thought.

By comparison, the Sun’s equator rotates far more slowly, about once every 648 hours or 27 days.

Based on the new analysis of its rotational speed, the researchers determined Vega to be between 700 and 800 million years old, compared to the Sun’s age of 4.567 billion years.

They also found Vega to have about 2.15 times the mass of the Sun.

Using an instrument developed by Monnier called the Michigan Infra-red Combiner, the researchers were able to collect light from six telescopes, increasing the resolution to a hundred times that of the Hubble Space Telescope.

“This allowed us to accurately measure the temperature of Vega, which is seen almost end on from Earth,” says Monnier.

“Because it’s spinning so fast, Vega has an equatorial bulge due to centrifugal force.”

“The greater the bulge, the further away from the star’s centre it’s equator is and that affects its temperature.”

“By measuring the temperature, we could work out how fast Vega is spinning which could then be used to determine its age,” says Monnie