Giving us a rare, unique window into the environment and emission history of the strongest magnets in the cosmos
Space news (astrophysics: wind nebulas; Swift J1834.9-0846) – 13,000 light-years toward the constellation Scutum in the midst of a vast cloud of high-energy, particles surrounding supernova remnant W41 –
Astronomers studying the strongest magnets discovered during the human journey to the beginning of space and time, magnetars, have detected one they haven’t seen before.A magnetar, a rare highly magnetic neutron star with a vast cloud of high-energy, recently-emitted particles called a wind nebula streaming from it. Offeringa unique window into the characteristics, environment and emission history of one of the most enigmatic and eye-opening objects ever detected.
“Right now, we don’t know how J1834.9 developed and continues to maintain a wind nebula, which until now was a structure only seen around young pulsars,” said lead researcher George Younes, a postdoctoral researcher at George Washington University in Washington. “If the process here is similar, then about 10 percent of the magnetar’s rotational energy loss is powering the nebula’s glow, which would be the highest efficiency ever measured in such a system.”
An object around 13 miles (20 kilometers) in diameter, or about the length of Manhattan Island, only 29 magnetars have been detected, so far. In this particular case, the source of detected emissionsis called Swift J1834.9-0846, a rare type of ultra-magnetic neutron stardetected by the Swift Gamma-ray Burst Satellite on August 7, 2011. It was subsequently looked at closer a month later by a team led by Younes using the European Space Agency’s (ESA) XMM-Newton X-ray Observatory. It was at this time astronomers realized and confirmed the first wind nebula ever detected around a magnetar.
“For me, the most interesting question is, why is this the only magnetar with a nebula? Once we know the answer, we might be able to understand what makes a magnetar and what makes an ordinary pulsar,” said co-author ChryssaKouveliotou, a professor in the Department of Physics at George Washington University’s Columbian College of Arts and Sciences.
Neutron stars are the crushed cores of massive stars left over after they have gone supernova and the densest objects astrophysicists have been able to directly observe during the human journey to the beginning of space and time. All neutron star magnetic fields detected, so far, are 100 to 10 trillion times stronger than Earth’s, and magnetar fields reach levels thousands of times stronger. Astrophysicists have no ideas on howmagnetic fields of such immense strength are formed.
“Making a wind nebula requires large particle fluxes, as well as some way to bottle up the outflow so it doesn’t just stream into space,” said co-author Alice Harding, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland. “We think the expanding shell of the supernova remnant serves as the bottle, confining the outflow for a few thousand years. When the shell has expanded enough, it becomes too weak to hold back the particles, which then leak out and the nebula fades away. This naturally explains why wind nebulae are not found among older pulsars, even those driving strong outflows.“
“The nebula around J1834.9 stores the magnetar’s energetic outflows over its whole active history, starting many thousands of years ago,” said team member Jonathan Granot, an associate professor in the Department of Natural Sciences at the Open University in Ra’anana, Israel. “It represents a unique opportunity to study the magnetar’s historical activity, opening a whole new playground for theorists like me.”
Astrophysicists think a magnetar outburst’s powered by energy stored in itssuper-strong magnetic fieldproduced gamma rays and x-rays, along with the gales of accelerated particles making up the nebulawind detected in the case of Swift J1834.9-0846. Now, they have a mystery to figure out, and new theories to deduce to explain the way a magnetar produces anebula wind.
Transform surrounding regions and actively evolve host galaxies
Space news (astrophysics: spinning black holes; bigger, brighter plasma jets) – in the core of galaxies across the cosmos, observing the spin of supermassive black holes –
Have you ever had the feeling the world isn’t the way you see it? That reality’s different than the view your senses offer you? The universe beyond the Earth is vast beyond comprehension and weird in ways human imagination struggles to fathom. Beyond the reach of your senses, the fabric of spacetime warps near massive objects, and even light bends to the will of gravity. In the twilight zone where your senses fear to tread, the cosmos twists and turns in weird directions and appears to leave the universe and reality far behind. Enigmas wrapped in cosmic riddles abound and mysteries to astound and bewilder the human soul are found.
Imagine an object containing the mass of millions even billions of stars like the Sun. Squeeze that matter into a region of infinitely small volume, a region so dense the gravitational force it exerts warps spacetime and prevents even light from escaping its grasp. This object’s what astronomers call a supermassive black hole, a titanic monster your eyes can’t see with a gravitational pull that would stretch your body to infinity as you approached and crossed its outer boundary, the event horizon. Beyond this point, spacetime and reality take a turn toward the extreme, and the rules of science don’t apply. You have entered the realm of one of the most mysterious and enigmatic objects discovered during the human journey to the beginning of space and time.
Astronomers hunting for supermassive black holes have pinpointed their realms to be the center of massive galaxies and even the center of galaxy clusters. From this central location in each galaxy, the gravitational well of each supermassive black hole appears to act as an anchor point for the billions of stars within, and astronomers believe a force for change and evolution of every galaxy and galaxy cluster in which they exist. Surrounded and fed by massive clouds of gas and matter called accretion disks, with powerful particle jets streaming from opposite sides like the death ray in Star Wars, fierce, hot winds sometimes moving at millions of miles per hour blow from these supermassive monsters in all directions.
“A lot of what happens in an entire galaxy depends on what’s going on in the minuscule central region where the black hole lies,” said theoretical astrophysicist David Garofalo of NASA’s Jet Propulsion Laboratory in Pasadena, Calif. Garofalo is the lead author of a new paper that appeared online May 27 in the Monthly Notices of the Royal Astronomical Society. Other authors are Daniel A. Evans of the Massachusetts Institute of Technology, Cambridge, Mass., and Rita M. Sambruna of NASA Goddard Space Flight Center, Greenbelt, Md.
Astronomers studying powerful particle jets streaming from supermassive black holes use to think these monsters spin either in the same direction as their accretion disks, called prograde black holes, or against the flow, retrograde black holes. For the past few decades, Garofalo and team have worked with a theory that the faster the spin of a black hole, the more powerful the particle jets streaming from it. Unfortunately, anomalies in the form of some prograde black holes with no jets have been discovered. This has scientists turning their ideas upside down and sideways, to see if flipping their “spin paradigm” model on its head explains recent anomalies in the theory.
Using data collected during a more recent study that links their previous theory with observations of galaxies at varying distances from Earth across the observable universe. Astronomers found more distant radio-loud galaxies with jets are powered by retrograde black holes, while closer radio-quiet black holes have prograde black holes. The study showed supermassive black holes found at the core of galaxies evolve over time from a retrograde to prograde state.
“This new model also solves a paradox in the old spin paradigm,” said David Meier, a theoretical astrophysicist at JPL not involved in the study. “Everything now fits nicely into place.”
Astrophysicists studying backward spinning black holes believe more powerful particle jets stream from these supermassive black holes because additional space exists between the monster and the inner edge of the accretion disk. This additional space between the monster and accretion disk provides more room for magnetic fields to build-up, which fuels the particle jet and increases its power. This idea is known as Reynold’s Conjecture, after the theoretical astrophysicist Chris Reynolds of the University of Maryland, College Park.
“If you picture yourself trying to get closer to a fan, you can imagine that moving in the same rotational direction as the fan would make things easier,” said Garofalo. “The same principle applies to these black holes. The material orbiting around them in a disk will get closer to the ones that are spinning in the same direction versus the ones spinning the opposite way.”
Scientists believe the powerful particle jets and winds emanating from supermassive black holes found at the center of galaxies also play a key role in shaping their evolution and eventual fate. Often even slowing the formation rate of new stars in a host galaxy and nearby island universes as well.
“Jets transport huge amounts of energy to the outskirts of galaxies, displace large volumes of the intergalactic gas, and act as feedback agents between the galaxy’s very center and the large-scale environment,” said Sambruna. “Understanding their origin is of paramount interest in modern astrophysics.”
What lies just beyond the reach of our senses and technology, beneath the exterior of these supermassive black holes? Scientists presently study these enigmatic stellar objects looking for keys to the doors of understanding beyond the veil of gas and dust surrounding these titanic beasts. Keys they hope one day to use to unlock even greater secrets of reality just beyond hidden doors of understanding.
Stretching over 300 light-years from the supernova remnant
Space news (astrophysics: supernovae; Cassiopeia A remnant) – 11,000 light-years from Earth toward the northern constellation Cassiopeia the Queen –
On the day in 1667 when a brilliant new star appeared in the sky in Cassiopeia the Queen, no written account is left to tell of the stellar event. The supernova remnant left over is called Cassiopeia A. It consists of a neutron star, with the first carbon atmosphere ever detected, and an expanding shell of material that was ejected from the star as it contracted under its own mass. The progenitor star of this supernova remnant was a supermassive star estimated to be between 15 to 20 times as massive as Sol.
The composite image of the Cassiopeia A supernova remnant seen above was made using six processed images taken over a three year period by NASA’s Spitzer Space Telescope. It shows the largest light echoes ever detected at over 300 light-years in length, which were created as light from the explosion passed through clumps of dust surrounding the supernova remnant. This light illuminated and heated surrounding dust clumps, making them briefly glow in infrared, like a series of colored lights lighting up one after the other. This resulted in an optical illusion in which the dust appears to be traveling away from the remnant at the speed of light. This apparent motion is represented in this image by different dust colors, with dust features unchanged over time appearing gray, and changes in surrounding dust over time represented by blue or orange colors.
Supernova remnant Cassiopeia A is the brightest radio emission source in the night sky above the frequency of 1 Gigahertz. It’s expanding shell of material reaches speeds above 5,000 km/s and temperatures as high as 50 million degrees Fahrenheit. First detected by Martin Ryle and Francis Graham-Smith in 1948, since this time it has become one of the most studied supernova remnants during the human journey to the beginning of space and time.
The startling false-color image above shows the many brilliant, stunning faces of the supernova remnant Cassiopeia A. Composed of images collected by three of the greatest space observatories in history, in three different wavebands of light. This view highlights the beauty hidden within one of the most violent events ever detected close by in the Milky Way.
NASA’s Spitzer Space Telescope infrared images used to create this stunning picture show warm dust in the outer shell of the supernova remnant Cassiopeia A highlighted in red. Hubble Space Telescope images added reveal delicate filaments of hot gas around 10,000 degrees Kelvin (18,000 degrees Fahrenheit) in yellow, while x-ray data collected by NASA’s Chandra X-ray Observatory is shown in green and blue. Look a little closer and deeper at the image and one sees hints of older infrared echoes from after the supernova hundreds of years ago.
Forming rings of X-ray light that expand with time, creating a shooting target effect
Space news (astrophysics: binary star systems; black hole/sun-like star systems) – 8,000 light-years away toward the constellation Cygnus, next to flaring 10 solar mass black hole –
It all started just before 2:32 p.m. on June 15, 2015, when NASA’s Swift X-ray Burst Alert Satellite detected a rising wave of high-speed, extremely-energetic X-rays emanating from the direction of the constellation Cygnus. Additional detections of the same flare ten minutes later by a Japanese experiment on the International Space Station called the Monitor of All-sky X-ray Image (MAXI) and other detectors. Allowed astronomers to determine the outburst detected originated 8,000 light-years away in low-mass X-ray binary V404 Cygni, where previous data indicated a stellar-mass black hole and sun-like star orbited each other. A black hole and sun-like star binary system that up to this point had been sleeping since its last outburst in 1989.
Fifteen days later on June 30, a team of scientists from around the world led by Andrew Beardmore of the University of Leicester in the United Kingdom investigated V404 Cygni a little closer using NASA’s Swift X-ray Burst Alert Satellite. Images taken (above) revealed a series of concentric rings of X-ray light centered on a 10 solar mass black hole (dot at the center of image).
Astronomers believe the x-ray rings are the result of echoing x-ray light from a large flare on June 26, 2016, at 1:40 p.m. EDT. The flare emitted x-rays in all directions. Multiple dust layers at around 4,000 and 1,000 light-years from V404 Cygni reflected some of these x-rays towards Earth. This reflected light travels a greater distance and reaches us slightly later than light traveling a straighter path. The small time difference produced an x-ray echo, formed x-ray rings expanding in spacetime.
“The flexible planning of Swift observations has given us the best dust-scattered X-ray ring images ever seen,” Beardmore said. “With these observations, we can make a detailed study of the normally invisible interstellar dust in the direction of this black hole.”
The team is currently watching V404 Cygni, waiting for its next outburst, and preparing Swift to collect additional data to determine exactly what’s going on here. They hope to hit the bulls eye in human understanding of the collection on x-ray sources detected across the cosmos. Regular monitoring of this binary system using a suite of telescopes and instruments could give us clues to how a stellar-mass black hole and sun-like star end up orbiting each other. About the origin and formation of the unusual types of binary systems detected during the human journey to the beginning of space and time.
Three Type Ia supernovae they study in order to measure cosmic distances and lift the veil of mystery surrounding dark energy
Space news (astrophysics: supernovae; 3 new candidates) – billions of light-years from Earth –
A team of determined astronomers studying the largest explosions viewed during the human journey to the beginning of space and time recently found three new candidates. Three candidates, they found after viewing 400 galaxies for two years using NASA’s Kepler Space Telescope.
“Kepler’s unprecedented pre-event supernova observations and Swift’s agility in responding to supernova events have both produced important discoveries at the same time but at very different wavelengths,” says Paul Hertz, Director of Astrophysics for NASA’s Science Mission Directorate. “Not only do we get insight into what triggers a Type Ia supernova, but these data allow us to better calibrate Type Ia supernovae as standard candles, and that has implications for our ability to eventually understand the mysteries of dark energy.”
In the data they collected over this two year period using NASA’s Kepler Space Telescope, this amazing team of explorers found three new and distant Type Ia supernovae, designated KSN 2011b, KSN 2011c, KSN 2012a. Due to the frequent observations of Kepler in the direction of the three distant supernovae, the data collected even contains the first moments of each tremendous blast. Measurements that will allow scientists to piece together the events leading to these events and the reasons for such a tremendous release of energy.
Astrophysicists believe Type Ia supernovae erupt with the same apparent brightness because in all cases the exploding body is a white dwarf star. It’s this property scientists use as a standard candle to more accurately measure the distance to objects around the cosmos than was previously possibly.
Astronomers also believe that every Type Ia supernovae are either the result of two white dwarf stars merging, or a white dwarf gathering so much material from a nearby companion star, it causes a thermonuclear reaction resulting in the white dwarf going supernova.
“Our Kepler supernova discoveries strongly favor the white dwarf merger scenario, while the Swift study, led by Cao, proves that Type Ia supernovae can also arise from single white dwarfs,” said Robert Olling, a research associate at the University of Maryland and lead author of the study. “Just as many roads lead to Rome, nature may have several ways to explode white dwarf stars.”
In the case of KSN 2011b, KSN 2011c, and KSN 2012a, astronomers found no evidence to support the existence of material being taken from a companion star. This leads them to believe the cause in these cases is collision and merger between two closely orbiting white dwarf stars.
Now, astronomers will use NASA’s Kepler Space Telescope and other Earth and space-based telescopes to search for Type Ia supernovae among thousands of galaxies included in the study. This will allow them to determine the distance of stellar objects across the cosmos more accurately. It will also help them delve deeper into the mystery surrounding dark energy and its true nature.
The search for supernovae continues
“The Kepler spacecraft has delivered yet another surprise, playing an unexpected role in supernova science by providing the first well-sampled early time light curves of Type Ia supernovae,” said Steve Howell, Kepler project scientist at NASA’s Ames Research Center in Moffett Field, California. “Now in its new mission as K2, the spacecraft will search for more supernovae among many thousands of galaxies.”
Characteristics of 30-year old supernova remnant SN 1979C are consistent with predicted theory on birth of black hole or possibly a rapidly spinning neutron star
Space news (December 11, 2015) – 50 million light-years from Earth, in galaxy M100 –
One of the most enigmatic cosmic objects discovered during the human journey to the beginning of space and time, black holes continue to entrance and mystify both astronomers studying them and common people trying to imagine the possibility of such monsters existing. Black holes are also one of the most difficult celestial objects to detect since not even light rays can escape from the strength of their gravitational-embrace, once they travel beyond the imaginary point-of-no-return astronomers call the “event horizon” of a black hole.
Astronomers working with NASA’s Chandra X-ray Observatory, after analysis of additional data provided by NASA’s Swift Gamma-ray Burst Explorer, the European Space Agency’s XMM-Newton spacecraft, and German’s ROSAT Observatory, believe they have evidence to suggest 30-year old supernova remnant SN 1979C could be a black hole.
Supernova remnant SN 1979C shined X-rays steadily during constant observation from 1995 to 2007. This suggests to astronomers either a black hole eating material left over from the supernova or a hidden binary companion feeding hot material to the monster hidden within.
“If our interpretation is correct, this is the nearest example where the birth of a black hole has been observed,” said Daniel Patnaude of the Harvard-Smithsonian Center for Astrophysics in Cambridge, Mass. who led the study.
Astronomers have detected new black holes that existed during the ancient past through gamma-ray bursts (GRBs) associated with them. SN 1979C is listed in a class of supernovae not expected to produce GRBs, which theory predicts could be the most common way to make a black hole.
“This may be the first time the common way of making a black hole has been observed,” said co-author Abraham Loeb, also of the Harvard-Smithsonian Center for Astrophysics. “However, it is very difficult to detect this type of black hole birth because decades of X-ray observations are needed to make the case.“
The idea SN 1979C is a young, recently-formed black hole made from the remnants of a star with 20 times the mass of Sol, that went supernova some thirty Earth-years ago, is consistent with present theory. In 2005, a theory was put forth claiming the bright source of X-rays detected steaming from the supernova remnant is powered by a jet emanating from the monster that’s unable to penetrate the thick hydrogen envelope surrounding it.
Astronomers think there could be one other possibility for the identity of SN 1979C. It could be a rapidly spinning neutron star, with an extremely powerful wind of high energy particles. Present theory predicts this would produce the bright X-ray emissions detected during 12 years of constant observation.
If this is true, this would make this supernova remnant the youngest known example of a celestial object called a pulsar wind nebula. The Crab Nebula is the best-known example of a bright pulsar wind nebula, but we would have to go back over 900 years to view it as a 30-year old. SN 1979C is a lot younger, which is a great opportunity to study one of the most enigmatic, yet difficult to detect celestial objects viewed during the human journey to the beginning of space and time.
“It’s very rewarding to see how the commitment of some of the most advanced telescopes in space, like Chandra, can help complete the story,” said Jon Morse, head of the Astrophysics Division at NASA’s Science Mission Directorate.
Astronomers will now continue to study SN 1979C, to see if they can determine its identity. No matter it’s true identity or nature, we can expect this celestial object to be one of the most studied examples of a young supernova remnant during recent times.
Bizarre and mysterious stellar objects, studying black holes keeps astronomers up all night. One of the more puzzling mysteries of these unique objects are gigantic flares of X-rays (relativistic jets) detected erupting from disks of hot, glowing dust surrounding them. X-ray flares astronomers are presently studying in order to better understand these enigmatic, yet strangely attractive stellar objects.
Astronomers observing supermassive black holes using NASA’s Swift spacecraft and Nuclear Spectroscopic Telescope Array (NuSTAR) recently caught one in the middle of a gigantic X-ray flare. After analysis, they discovered this particular flare appeared to be a result of theCorona surrounding the supermassive black hole – region of highly energetic particles – being launched into space. A result making scientists and astronomers rethink their theories on how relativistic jets are created and sustained.
This result suggests to scientists that supermassive black holes emit X-ray flares when highly energized particles (Coronas) are launched away from the black hole. In this particular case, X-ray flares traveling at 20 percent of the speed of light, and directly pointing toward Earth. The ejection of the Corona caused the X-ray light emitted to brighten a little in an effect called relativistic Doppler boosting. This slightly brighter X-ray light has a different spectrum due to the motion of the Corona, which helped astronomers detect this unusual phenomenon leaving the disk of dust and gas surrounding this supermassive black hole.
“This is the first time we have been able to link the launching of the Corona to a flare,” said Dan Wilkins of Saint Mary’s University in Halifax, Canada, lead author of a new paper on the results appearing in the Monthly Notices of the Royal Astronomical Society. “This will help us understand how supermassive black holes power some of the brightest objects in the universe.“
Astronomers currently propose two different scenarios for the source ofcoronas surrounding supermassive black holes. The “lamppost” scenario indicates coronas are analogous to light bulbs sitting above and below the supermassive black hole along its axis of rotation. This idea proposes coronas surrounding supermassive black holes are spread randomly as a large cloud or a “sandwich” that envelopes the disk of dust and material surrounding the black hole. Some astronomers think coronas surrounding supermassive black holes could alternate between both the lamppost and sandwich configurations.
The latest data seems to lean toward the “lamppost” scenario and gives us clues to how the coronas surrounding black holes move. More observations are needed to ascertain additional facts concerning this unusual phenomenon and how massive X-ray flares and gamma rays emitted by supermassive black holes are created.
“Something very strange happened in 2007, when Mrk 335 faded by a factor of 30. What we have found is that it continues to erupt in flares but has not reached the brightness levels and stability seen before,” said Luigi Gallo, the principal investigator for the project at Saint Mary’s University. Another co-author, Dirk Grupe of Morehead State University in Kentucky, has been using Swift to regularly monitor the black hole since 2007.
“The Corona gathered inward at first and then launched upwards like a jet,” said Wilkins. “We still don’t know how jets in black holes form, but it’s an exciting possibility that this black hole’s Corona was beginning to form the base of a jet before it collapsed.”
“The nature of the energetic source of X-rays we call the Corona is mysterious, but now with the ability to see dramatic changes like this we are getting clues about its size and structure,” said Fiona Harrison, the principal investigator of NuSTAR at the California Institute of Technology in Pasadena, who was not affiliated with the study.
Astronomers will now continue their study of supermassive black holes in the cosmos in order to remove the veil of mystery surrounding the X-ray flares they emit and other bizarre mysteries surrounding these enigmatic stellar objects. In particular, they would love to discover the reasons for the ejection of Coronas surrounding black holes.
Erupting X-ray flares every day, a ten-fold increase in bright flares from previous observations of Sagittarius A
Space news (October 01, 2015) – 26,000 light-years from Earth, near the center of the Milky Way
Astrophysicists combining the telescopic talents of NASA’s Chandra X-ray Observatory and Swift spacecraft, with the European Space Agency’s X-ray Space Observatory XMM-Newton, recently detected an increase in X-ray flares erupting from the supermassive black hole (Sagittarius A) at the center of the Milky Way.
By analyzing data collected during extensive periods of monitoring by all three spacecraft, space scientists determined the Monster of the Milky Way – the supermassive black hole at the center with more than 4 million times the mass of Sol– has been more active during the past 15 years than first thought.
Erupting a bright X-ray flare every ten days, the Monster of the Milky Way has been eating hot gas falling into its gravity pool. Even more interesting, Sagittarius A during the past year has been erupting ten times as much, producing a bright X-ray flare every day. A discovery that has astrophysicists going over the data looking for a reason for the sudden increase.
“For several years, we’ve been tracking the X-ray emission from Sgr A*. This includes also the close passage of this dusty object” said Gabriele Ponti of the Max Planck Institute for Extraterrestrial Physics in Germany. “A year or so ago, we thought it had absolutely no effect on Sgr A*, but our new data raise the possibility that that might not be the case.”
The mystery started late in 2013, as G2 passed close to the supermassive black hole. At this time, there wasn’t any apparent change in G2 as it approached Sagittarius A, other than being slightly stretched by the gravity pool of the black hole.
Originally astronomers thought G2 was a stretched cloud of gas and dust, but this finding has led scientists to the possibility it could be a dense body embedded in a dusty cocoon. Currently, there’s no consensus among astronomers on the identity of this mysterious object. But the recent ten-fold increase in X-ray flares as G2 passed near the supermassive black hole suggests there could be a connection of some kind.
“There isn’t universal agreement on what G2 is,” said Mark Morris of the University of California at Los Angeles. “However, the fact that Sgr A* became more active not long after G2 passed by suggests that the matter coming off of G2 might have caused an increase in the black hole’s feeding rate.”
At this point, astronomers don’t know if the increase in X-ray flares from the supermassive black hole is common or unusual in nature. These emissions could be part of the normal life cycle of supermassive black holes and totally unrelated to the passage of G2. The ten-fold increase in X-ray flares could also be due to changing solar winds from nearby massive stars feeding gas and dust into the black hole.
Scientists will keep observing Sagittarius A over the next little while to see what pops up next in this mystery. Hopefully, they can shed some light on the reason the Monster of the Milky Way, suddenly started emitting X-ray flares once a day.
“It’s too soon to say for sure, but we will be keeping X-ray eyes on Sgr A* in the coming months,” said co-author Barbara De Marco, also of Max Planck. “Hopefully, new observations will tell us whether G2 is responsible for the changed behavior or if the new flaring is just part of how the black hole behaves.”
In the battle between celestial masses, greater mass means a bigger pull, and usually survival of the more massive body
Space news (April 28, 2015)
– A cosmic mystery unfolds 43,000 light years away in globular cluster NGC 6388
NASA space scientists studying the source of x-rays emanating from a globular cluster on the edge of the Milky Way are on the trail of a cosmic mystery.
Evidence seems to indicate x-rays were created as hot gas was drawn into the intermediate-mass black hole space scientists believe resides at the center of globular cluster NGC 6388.
Taking a closer look at data obtained using the European Space Agency’s INTErnational Gamma-Ray Laboratory (INTEGRAL), and NASA’s Chandra X-ray Observatory and Swift Gamma-Ray Burst Explorer revealed the x-rays emanated from a location slightly off to one side of the center of NGC 6388.
Where does this cosmic mystery lead?
Space scientists looking at theoretical simulations and the data obtained observing the x-ray source for 200 days now believe x-rays were created as a planet, one-third the mass of Earth, was ripped apart as it came to close to a white dwarf star roughly the size of our planet.
How could a body the size of Earth pull apart a planet estimated to be one-third the mass?
A white dwarf star is the remnant of a medium-mass star, similar to our own Sun. In this case, space scientists estimate the white dwarf star was about 1.4 times the mass of our Sun, which means its surface gravity would be over 10,000 times stronger.
As a body thirty-three percent of the mass of Earth travels near a white dwarf star with a surface gravity of this magnitude, space scientists simulations indicate the difference in gravitational forces between the far and near side of the body creates gravitational tides that are greatly enhanced due to the nearness and magnitude of gravitational forces involved.
Space scientists indicate computer simulations suggest a planet would be first pulled away from its parent star due to the gravitational force created by the dense concentration of stars near the center of globular cluster NGC 6388.
If this planet were to pass near a white dwarf star with a mass close to the one in this news story, computer simulations indicate it could be torn apart by extreme tidal forces created as it passes.
The planetary debris created is then heated and glows in x-rays as it falls into the gravitational field of the white dwarf.
In this case, the observed amount of x-rays is as computer simulations indicate should be detected, so space scientists think they’re at least on the right trail. They’re now going over the data obtained and conducting new experiments to eliminate other possible x-ray sources.
For more information on NASA’s space mission visit here.
Learn more about the Chandra X-ray Observatory here.
Discover more about the mission of the European Space Agency’s INTErnational Gamma-Ray Laboratory (INTEGRAL) here.
For more information concerning the Swift Gamma-Ray Burst Explorer visit here.
Until NASA’s Swift Gamma-ray Burst Space Observatory detected a sequence of seven stellar flares over 10,000 times more powerful than the biggest ever recorded erupting from a red dwarf star in the binary system DG CVn
Space news ( Oct. 30, 2014) – astrophysics: gamma-ray bursts; seven of the most intense, powerful gamma-ray bursts ever detected –
NASA space scientists operating NASA’s Swift Gamma-ray Burst Space Observatory detected a sequence of seven of the most intense, powerful, and long-lasting stellar flares ever seen at 5:07 p.m EDT on April 23, 2014. You can watch a video of the event here. They believe the gamma-rays detected are from stellar flares erupting from the surface of one of a pair of red dwarf stars 60 light-years away in the binary star system DG Canum Venaticorum (DG CVn). They are currently scratching their heads and rethinking theories on the intensity, power, and length of time of major stellar flaring episodes exhibited by red dwarf stars.
“For about three minutes after the BAT trigger, the superflare’s X-ray brightness was greater than the combined luminosity of both stars at all wavelengths under normal conditions,” noted Goddard’s Adam Kowalski, who is leading a detailed study on the event. “Flares this large from red dwarfs are exceedingly rare.”
“We used to think major flaring episodes from red dwarfs lasted no more than a day, but Swift detected at least seven powerful eruptions over a period of about two weeks,” said Stephen Drake, an astrophysicist at NASA’s Goddard Space Flight Center in Greenbelt, Maryland, who gave a presentation on the “superflare” at the August meeting of the American Astronomical Society’s High Energy Astrophysics Division. “This was a very complex event.”
At peak power and intensity, space scientist Rachael Osten of the Space Telescope Institute and Stephen Drake of NASA’s Goddard Space Flight Center indicate this sequence of stellar flares reached 360 million degrees Fahrenheit (200 million Celsius), which is over 12 times hotter than the center of our own sun. Currently, they’re trying to figure out which of the pair of red dwarf stars is the source of the sequence of seven stellar flares they observed.
Space scientists indicate the problem is the pair of red dwarf suns in this binary star system are only about three times the distance apart as the average distance of Earth from the sun. This is too close for instruments to determine which red dwarf star is the culprit in this case.
“This system is poorly studied because it wasn’t on our watch list of stars capable of producing large flares,” said Rachel Osten, an astronomer at the Space Telescope Science Institute in Baltimore and a deputy project scientist for NASA’s James Webb Space Telescope, now under construction. “We had no idea DG CVn had this in it.”
NASA space scientists will now turn their attention to stars within 100 light-years of DG DVn. The majority of these suns are middle-aged, like our own sun, but there are over a thousand young red dwarf stars drifting through this region of space. Studying red dwarf suns of the same age as DG CVn (around 30 million years) will allow the best opportunity to observe similar stellar flares as the seven seen recently. They also plan to keep an eye on DG CVn using the Swift Gamma-ray Burst Explorer in case it unleashes similar stellar flares in the future.
For more information on the Swift Gamma-ray Burst Explorer visit.
You can find more information on NASA and red dwarf stars here.