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New Kind of "Runt" Supernovae Could be Lurking Unseen - 0 views

  • Until now, supernovae have come in two main versions
  • In one scenario, a huge star, 10 to 100 times more massive as our Sun, collapses causing a colossal stellar explosion
  • Type Ia supernovae, occurs when material from a parent star streams onto the surface of a white dwarf. Over time, so much material falls onto the white dwarf that it raises the core temperature igniting carbon and causing a runaway fusion reaction. This event completely disrupts the white dwarf and results in a colossal stellar explosion
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  • Now astronomers have found a third type that is fainter and less energetic than a Type Ia. Called a Type Iax supernova
  • essentially a mini supernova
  • only about one-hundredth as bright as their supernova siblings
  • calculates that Type Iax supernovae are about as third as common as Type Ia supernovae
  • The researchers also did not find them in elliptical galaxies, filled with older stars, suggesting that Type Iax supernovae come from young star systems
  • team identified 25 examples of this new type of supernova
  • Based on observations, the team found that the new Type Iax supernovae come from binary star systems containing a white dwarf and a companion star that has burned all of its hydrogen, leaving an outer layer that is helium rich
  • not sure what triggers the Type Iax supernova
  • One explanation involves the ignition of the outer helium layer from the companion star. The resulting shockwave slams into the white dwarf and disrupts it, causing the explosion.
  • Alternately, the white dwarf might ignite first due to the overlying helium shell it has collected from the companion star.
  • it appears that in many cases the white dwarf survives the explosion unlike in a Type Ia supernova where the white dwarf is completely destroyed
  • Supernovae explosions release so much energy as heat and light that they outshine entire galaxies for brief periods of time
  • The extremely hot conditions naturally create new heavier elements, such as gold, lead, nickel, zinc and copper
  • Type Iax supernovas aren’t rare, they’re just faint
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ScienceShot: A New Class of Supernova - ScienceNOW - 0 views

  • type Iax, release somewhere between 1% and 50% the energy of a type Ia supernova
  • spectra of type Iax stars don't include any signs of hydrogen
  • Type Iax supernovae most likely form in binary star systems when a superdense, carbon- and oxygen-rich white dwarf star (center of disk at left) robs material from its helium-rich partner, eventually accumulating enough mass on its surface to trigger an explosion
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  • Astronomers likely have discovered so few type Iax supernovae only because they are faint, not because they are rare
  • estimates that for every 100 type Ia supernovae explosions that occur, there are about 31 type Iax supernovae
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What a Star About to Go Supernova Looks Like - 0 views

  • This nebula with a giant star at its center
  • th stars had identical rings of the same size and age, which were travelling at similar speeds; both were located in similar HII regions; and they had the same brightness
  • no one can predict when a star will go supernova,
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  • But astronomers are certainly hoping they’ll have the chance to watch it happen.
  • has striking similarities to a star that went supernova back in 1987, SN 1987A.
  • SN 1987A is the closest supernova to that we’ve been able to study since the invention of the telescope and it has provided scientists with good opportunities to study the physical processes of an exploding star
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Supernova Candidate Stars May Signal "Impending Doom" - 0 views

  • very visible supernova event. Hosted in the Whirlpool Galaxy (M51),
  • researchers at Ohio State University, a galaxy survey may have captured evidence of a “stellar signal” just before it went supernova
  • OSU team was undertaking a survey of 25 galaxies for stars that changed their magnitude in usual ways
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  • goal was to find a star just before it ended its life
  • a binary star system located in M51 produced just the results they were looking fo
  • ne star dropped amplitude just a short period of time before the other exploded
  • Maybe stars give off a clear signal of impending doom, maybe they don’t
  • But we’ll learn something new about dying stars no matter the outcome
  • it was a binary star system being studied by the OSU team
  • consisted of both a blue and red star
  • At this point, the astronomers surmise the red star was the one that dimmed significantly over the three-year period while the blue one blew its top
  • reviewing the LBT data
  • when compared with Hubble images, the red star dimmed at about 10% over the final three-year period at an estimated 3% per previous years
  • researchers surmise the red star may have actually survived the supernova event
  • After the light from the explosion fades away, we should be able to see the companion that did not explode
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New Type of Star Explosion Discovered | Type Iax Supernovas | Space.com - 0 views

  • It remains unclear what precisely happens
  • The helium in the companion star's outer shell might undergo nuclear fusion, blasting a shock wave at the white dwarf that makes it detonate
  • On the other hand, all the helium the white dwarf accumulated from its companion star could alter the density and temperature of the white dwarf's interior, forcing carbon, oxygen and maybe helium within the star to fuse, triggering an explosion
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  • No Type Iax supernovas have been seen so far in elliptical galaxies, which are filled with old stars
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Discovery of two types of neutron stars points to two different classes of supernovae - 0 views

  • Neutron stars are the last stage in the evolution of many massive stars
  • the mass of a single neutron star exceeds that of the entire sun, but squeezed into a ball whose diameter is smaller than that of London
  • to reveal how they have discovered two distinct populations of neutron stars that appear to have formed via two different supernova channels
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  • speculated before about the possible existence of different types of neutron stars, but there has never been any clear observational evidence that there is really more than one type
  • astronomers analysed data on a large sample of high-mass X-ray binaries
  • double star systems in which a fast-spinning neutron star orbits a massive young companion
  • neutron star in these systems also periodically siphons off material from its partner
  • neutron star becomes an X-ray pulsar
  • because by timing their pulses, astronomers can accurately measure the neutron star spin periods
  • detected two distinct groupings in a large set of spin periods measured in this way
  • one group of neutron stars typically spinning once every 10 seconds
  • the other once every 5 minutes
  • led them to conclude that the two distinct neutron star populations formed via two different supernova channels
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Mysterious Extragalactic Explosions Baffle Astronomers | Fast Radio Bursts | Space.com - 0 views

  • known as fast radio bursts (FRBs), above the plane of our Milky Way Galaxy.
  • These bursts gave off more energy in a millisecond than the sun does in 300,000 years
  • The bursts ranged from 5.5 to 10 billion light-years away, meaning it took the light from some of them 10 billion years to reach Earth. (The Big Bang 
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  • occurred 13.8 billion years ago
  • These newfound objects allowed the researchers to calculate that an FRB should occur once every 10 seconds
  • whether the new signals came from inside or outside the Milky Way.
  • they studied how the radio waves were affected by the material they pass through — a technique that could allow these new objects to shed light on the components of space.
  • As radio waves travel in space, they are stretched and slowed by the ionized material through which they move
  • Using models, the team concluded that the FRBs traveled billions of light-years — much farther than the edge of Earth's galaxy
  • the source is likely located in another galaxy
  • They are so bright and narrow that we can limit the size of the emission region at the source to just a few hundred kilometers
  • Although the explosions are brief, the astronomers can pinpoint the bursts' locations pretty accurately
  • No corresponding object could be observed in optical, gamma or X-ray wavelengths, so the explosions' origins remain unknown to scientists
  • Possible sources
  • intersecting magnetic fields from two neutron stars, extremely dense city-size bodies packing the mass of the sun.
  • A special kind of supernova orbited by a neutron star could potentially produce radio bursts as the star's magnetic field interacts with the explosion of the supernova
  • such combinations would be rare
  • favorite explanation is a giant burst from a magnetar, a highly magnetized type of neutron star
  • performed approximately a year after the FRBs were first spotted, looked at whether the objects continued to produce emission, but the signals appear to be nonrepeating
  • Efforts are ongoing at the moment to detect FRBs in close to real time, such that they can be followed up quickly
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April 30 - Today in Science History - Scientists born on April 30th, died, and events - 0 views

  • Supernova
  • In 1006, Chinese and Arabic astronomers noted a supernova. The speed of the still-expanding shock wave was measured nearly a millenium later.* This is was history's brightest "new star" ever recorded, at first seen to be brighter than the planet Venus. It occurred in our Milky Way galaxy, appearing in the southern constellation Lupus, near the star Beta Lupi. It was also recorded by observers in Switzerland, Italy, Japan, Egypt and Iraq. From the careful descriptions of the Chinese astronomers of how the light varied, that it was of apparently yellow color and visible for over a year, it is possible that the supernova reached a magnitude of up to -9. Modern measurements of the speed of the shock wave have been used to estimate its distance
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Hubble Space Telescope Passes Major Science Milestone | Hubble 10,000th Science Paper |... - 0 views

  • Hubble Space Telescope has crossed a major milestone, accumulating 10,000 science papers based on its observations
  • After 21 years
  • it's actually in the best shape of its life
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  • last space shuttle servicing mission was in May 2009.
  • Papers describing discoveries in nearly every field of astronomy and cosmology have been published based on data gathered by the Hubble Space Telescope.
  • conducted by scientists in more than 35 countries
  • most papers written by researchers in the United States, the United Kingdom, Germany, Italy, France, and Spain
  • Hubble's top five most referenced papers are on
  • The search for distant supernovas used to characterize dark energy
  • The precise measurement of the universe's rate of expansion
  • The apparent link between galaxy mass and central black hole mass
  • Early galaxy formation in the Hubble Deep Field
  • The evolutionary models for low-mass stars and brown dwarfs
  • 10,000th Hubble science paper
  • announces the discovery of the faintest supernova ever associated with a cosmic explosion called a long-duration gamma-ray burst, which spews high-energy radiation into space when a star dies
  • The first science paper based on Hubble data came about six months after the telescope's launch
  • a paper on observations of the center of galaxy NGC 7457, where scientists suspected a huge black hole lurked
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Did NASA's Voyager 1 Spacecraft Just Exit the Solar System? | Space.com - 0 views

  • Scientists are crunching one more set of numbers to find out for sure.
  • New data from the spacecraft indicate that the historic moment of its exit from the solar system might have come and gone two months ago
  • For two years now, data beamed back to Earth by Voyager 1 has hinted at its close approach to the edge of the solar system, a pressure boundary called the heliopaus
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  • bubble of electrically charged particles blowing outward from the sun (called the heliosphere) exactly counterbalances the inward pressure of the gas and dust from interstellar space, causing equilibrium between the two
  • scientists have had trouble figuring out what, exactly, happens at or near this boundary — making it hard to tell whether Voyager has crossed it
  • In 2010, Voyager passed the point where the solar wind, a stream of charged particles flowing outward from the sun, seemed to
  • indicated that the wind had suddenly died down, and all the surrounding solar particles were at a standstill
  • "stagnation region" came as a surprise
  • expected to see the solar wind veer sideways
  • the perplexing collapse of the solar wind at the edge of the heliosphere left them without a working model for the outer solar system
  • no well-established criteria of what constitutes exit from the heliosphere
  • "All theoretical models have been found wanting."
  • a space scientist at Johns Hopkins who works with Voyager 1 data, said that in any model of the heliopause, an object exiting through it should experience three changes: a sharp rise in the number of collisions with cosmic rays (high-energy particles from space), a dramatic drop in the number of collisions with charged particles from the sun, and a change in the direction of the surrounding magnetic field.
  • Based on two of those criteria, Voyager 1 looks as if it passed through the heliopause at the end of the summer
  • The level of these cosmic ray collisions jumped significantly in late August.
  • spacecraft has experienced a steady rise in the number of collisions with particles whose energies are greater than 70 Mega-electron-volts, indicating they are probably cosmic rays emanating from supernova explosions far beyond the solar system
  • in late August, cosmic ray collisions sharply rose, and solar particle collisions sharply fell: two indicators of a transition through the heliopause
  • To officially declare Voyager's crossing, the scientists need to check if the third condition holds
  • change in magnetic field direction
  • e interstellar field beyond the influence of the sun) is critical because, even though there is debate among astrophysicists as to what direction the field will lie in
  • unlikely that it is the direction that we have been seeing at Voyager 1 throughout the most recent years
  • scientists could not say when the magnetic field analysis would be finished. But when it is
  • Once we have a consensus within the team we will inform NASA for a proper announcement,
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Frenchman, American win Nobel for quantum physics (Update 6) - 0 views

  • American physicist David Wineland
  • and French physicist Serge Haroche speaks to the media in Paris after they were named winners of the 2012 Nobel Prize in physics.
  • for experiments on quantum particles that have already resulted in ultra-precise clocks and may one day help lead to computers many times faster than those in use today.
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  • A Frenchman and an American shared the Nobel Prize in physics Tuesday for inventing methods to peer into the bizarre quantum world of ultra-tiny particles, work that could help in creating a new generation of super-fast computers
  • quantum computers could radically change people's lives in the way that classical computers did last century, but a full-scale quantum computer is still decades away
  • in a quantum computer, an individual particle can essentially represent a zero and a one at the same time
  • If scientists can make such particles work together, certain kinds of calculations could be done with blazing speed.
  • The prizes are always handed out on Dec. 10, the anniversary of prize founder Alfred Nobel's death in 1896.
  • 2012: Serge Haroche of France and David Wineland of the U.S. for "for ground-breaking experimental methods" that enable measuring and manipulation of individual quantum systems
  • 2011: American physicist Saul Perlmutter, U.S.-Australian researcher Brian Schmidt and American professor Adam Riess "for the discovery of the accelerating expansion of the Universe through observations of distant supernovae."
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Mars Science Laboratory: Data From NASA Rover's Voyage To Mars Aids Planning - 0 views

  • Curiosity's Radiation Assessment Detector (RAD) is the first instrument to measure the radiation environment during a Mars cruise mission from inside a spacecraft that is similar to potential human exploration spacecraft
  • The findings,
  • indicate radiation exposure for human explorers could exceed NASA's career limit for astronauts if current propulsion systems are used.
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  • Two forms of radiation pose potential health risks to astronauts in deep space. One is galactic cosmic rays (GCRs), particles caused by supernova explosions and other high-energy events outside the solar system. The other is solar energetic particles (SEPs) associated with solar flares and coronal mass ejections from the sun
  • NASA has established a three percent increased risk of fatal cancer as an acceptable career limit for its astronauts currently operating in low-Earth orbit
  • The RAD data showed
  • Only about three percent of the radiation dose was associated with solar particles because of a relatively quiet solar cycle and the shielding provided by the spacecraft
  • In terms of accumulated dose, it's like getting a whole-body CT scan once every five or six days
  • Current spacecraft shield much more effectively against SEPs than GCRs. To protect against the comparatively low energy of typical SEPs, astronauts might need to move into havens with extra shielding on a spacecraft or on the Martian surface, or employ other countermeasures
  • GCRs tend to be highly energetic, highly penetrating particles that are not stopped by the modest shielding provided by a typical spacecraft.
  • RAD data collected during Curiosity's science mission will continue to inform plans to protect astronauts as NASA designs future missions to Mars in the coming decades.
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Nearby Ancient Star is Almost as Old as the Universe - 0 views

  • A metal-poor star located merely 190 light-years from the Sun is 14.46+-0.80 billion years old, which implies that the star is nearly as old as the Universe
  • results emerged from a new study
  • Such metal-poor stars are (super) important to astronomers because they set an independent lower limit for the age of the Universe
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  • can be used to corroborate age estimates inferred by other means
  • In the past, analyses of globular clusters and the Hubble constant
  • yielded vastly different ages for the Universe, and were offset by billions of years
  • based on the microwave background and Hubble constant, but it must have formed soon after the big bang
  • Within the errors, the age of HD 140283 does not conflict with the age of the Universe, 13.77 ± 0.06 billion years
  • Metal-poor stars can be used to constrain the age of the Universe because metal-content is typically a proxy for age
  • Heavier metals are generally formed in supernova explosions, which pollute the surrounding interstellar medium.
  • Stars subsequently born from that medium are more enriched with metals than their predecessors
  • each successive generation becoming increasingly enriched
  • HD 140283 exhibits less than 1% the iron content of the Sun, which provides an indication of its sizable age.
  • had been used previously to constrain the age of the Universe, but uncertainties tied to its estimated distance (at that time) made the age determination somewhat imprecise
  • obtain a new and improved distance for HD 140283 using the Hubble Space Telescope (HST), namely via the trigonometric parallax approach
  • distance uncertainty for HD 140283 was significantly reduced by comparison to existing estimates, thus resulting in a more precise age estimate for the star
  • The reliability of the age determined is likewise contingent on accurately determining the sample’s metal content
  • analyses of globular clusters and the Hubble constant yielded vastly different ages for the Universe
  • discrepant ages stemmed partly from uncertainties in the cosmic distance scale
  • determination of the Hubble constant relied on establishing (accurate) distances to galaxies
  • One of the key objectives envisioned for HST was to reduce uncertainties associated with the Hubble constant to <10%, thus providing an improved estimate for the age of the Universe
  • the mean implying an age near ~14 billion years
  • Determining a reliable age for stars in globular clusters is likewise contingent on the availability of a reliable distance
  • the study reaffirms that there are old stars roaming the solar neighborhood which can be used to constrain the age of the Universe
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