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Graphite Whiskers, Rather Than Dark Energy, Could Explain Dimness Of Stellar Explosions
ScienceDaily (Feb. 29, 2008) — Interstellar space may be strewn with tiny whiskers of carbon, dimming the light of far-away objects. This discovery by scientists at the Carnegie Institution may have implications for the "dark energy" hypothesis, proposed a decade ago in part to explain the unexpected dimness of certain stellar explosions called Type1a supernovae.
See also:
Space & Time
* Astrophysics
* Astronomy
* Dark Matter
* Sun
* Space Station
* NASA
Reference
* Interstellar medium
* Blue supergiant star
* Nucleosynthesis
* Supergiant
Type1a supernovae are among the brightest objects in the universe. Astronomers use them as "standard candles" to gauge cosmological distances: brighter-appearing supernovae are closer, dimmer ones are farther away. In the late 1990s some astronomers noticed that some seemed too dim--too far away--to be explained by conventional theories of the universe's expansion. This led to the hypothesis that the expansion was accelerating, pushed along by an unknown form of energy -- dark energy.
In the current study, published in the February 29 issue of Science, Andrew Steele and Marc Fries of the Carnegie Institution's Geophysical Laboratory report the discovery of an unusual new form of carbon in minerals within meteorites dating from the formation of the solar system. These "graphite whiskers" were likely produced from carbon-rich gas at high temperatures and were found within features called calcium-aluminum inclusions, which at around 4.5 billion years old are the oldest known solids in our solar system.
"During this time when the sun was young, the solar wind was very strong," says Fries. "So graphite whiskers formed near the sun could have been blown into interstellar space. The same thing may have happened around other young stars as well."
Graphite whiskers might also be produced and dispersed into space by supernovae explosions.
A thin interstellar haze of graphite whiskers spewed from stars and supernovae would affect how different wavelengths of light pass through space. It has been postulated that wavelengths in the near infrared would be particularly affected. It is the dimming of light from Type 1a supernovae at these wavelengths that first led researchers to think that the universe's expansion was accelerating and that therefore a hitherto unknown force "dark energy"must exist. However, since the 1970s it has been postulated that graphite or other whisker-like materials could explain the observations. The presence of graphite whiskers in space has never been confirmed until this study.
With the discovery of graphite whiskers in the meteorite, researchers can test their properties against the cosmological models and astronomical observations.
"If graphite whiskers in space are absorbing supernovae's light," says Steele, "then this could affect measurements of the rate of the universe's expansion. While we cannot comment further on the effects of whiskers on the dark energy hypothesis it is important to study the characteristics of this form of carbon carefully so we can understand its impact on dark energy models. We'll then feed this data forward to the upcoming NASA and ESA (European Space Agency) missions that will look for the effects of dark energy."
Adapted from materials provided by Carnegie Institution, via EurekAlert!, a service of AAAS.
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Carnegie Institution (2008, February 29). Graphite Whiskers, Rather Than Dark Energy, Could Explain Dimness Of Stellar Explosions. ScienceDaily. Retrieved August 24, 2009, from http://www.sciencedaily.com /releases/2008/02/080228143538.htm
Two closely orbiting violet-hot carbon-oxygen white dwarfs are spiraling into one another. The two stars are destined to merge, leading to carbon/oxygen fusion and a Type Ia supernova explosion. Graphite whiskers might be produced and dispersed into space by supernovae explosions. (Credit: Creative Commons License/Drew Taylor)
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Related Stories
What Can Swiss Cheese Teach Us About Dark Energy? (Dec. 28, 2008) — About 10 years ago, scientists reached the astonishing conclusion that our universe is accelerating apart at ever-increasing speeds, stretching space and time itself like melted cheese. The force ... > read more
NASA'S Swift Sees Double Supernova In Galaxy (June 27, 2007) — In just the past six weeks, two supernovae have flared up in an obscure galaxy in the constellation Hercules. Never before have astronomers observed two of these powerful stellar explosions occurring ... > read more
Cosmic Lighthouses: Astrophysicists Explain Differences In Brightness Of Supernova Explosions (Feb. 23, 2007) — Supernovae stand out in the sky like cosmic lighthouses. Scientists at the Max Planck Institute for Astrophysics and at the National Astronomical Institute of Italy have now found a way to use these ... > read more
New Class Of Dim Supernovae (June 7, 2009) — The colossal stellar explosions called supernovae come in many kinds and flavors. Some of them are produced when a massive star reaches the end of its life in a sudden gravitational collapse. ... > read more
Dark Energy May Be Vacuum (Jan. 16, 2007) — Researchers at the University of Copenhagen's Dark Cosmology Centre at the Niels Bohr Institute have brought us one step closer to understanding what the universe is made of. The new data shows that ... > read more
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Graphite Whiskers, Rather Than Dark Energy, Could Explain Dimness Of Stellar Explosions
ScienceDaily (Feb. 29, 2008) — Interstellar space may be strewn with tiny whiskers of carbon, dimming the light of far-away objects. This discovery by scientists at the Carnegie Institution may have implications for the "dark energy" hypothesis, proposed a decade ago in part to explain the unexpected dimness of certain stellar explosions called Type1a supernovae.
See also:
Space & Time
* Astrophysics
* Astronomy
* Dark Matter
* Sun
* Space Station
* NASA
Reference
* Interstellar medium
* Blue supergiant star
* Nucleosynthesis
* Supergiant
Type1a supernovae are among the brightest objects in the universe. Astronomers use them as "standard candles" to gauge cosmological distances: brighter-appearing supernovae are closer, dimmer ones are farther away. In the late 1990s some astronomers noticed that some seemed too dim--too far away--to be explained by conventional theories of the universe's expansion. This led to the hypothesis that the expansion was accelerating, pushed along by an unknown form of energy -- dark energy.
In the current study, published in the February 29 issue of Science, Andrew Steele and Marc Fries of the Carnegie Institution's Geophysical Laboratory report the discovery of an unusual new form of carbon in minerals within meteorites dating from the formation of the solar system. These "graphite whiskers" were likely produced from carbon-rich gas at high temperatures and were found within features called calcium-aluminum inclusions, which at around 4.5 billion years old are the oldest known solids in our solar system.
"During this time when the sun was young, the solar wind was very strong," says Fries. "So graphite whiskers formed near the sun could have been blown into interstellar space. The same thing may have happened around other young stars as well."
Graphite whiskers might also be produced and dispersed into space by supernovae explosions.
A thin interstellar haze of graphite whiskers spewed from stars and supernovae would affect how different wavelengths of light pass through space. It has been postulated that wavelengths in the near infrared would be particularly affected. It is the dimming of light from Type 1a supernovae at these wavelengths that first led researchers to think that the universe's expansion was accelerating and that therefore a hitherto unknown force "dark energy"must exist. However, since the 1970s it has been postulated that graphite or other whisker-like materials could explain the observations. The presence of graphite whiskers in space has never been confirmed until this study.
With the discovery of graphite whiskers in the meteorite, researchers can test their properties against the cosmological models and astronomical observations.
"If graphite whiskers in space are absorbing supernovae's light," says Steele, "then this could affect measurements of the rate of the universe's expansion. While we cannot comment further on the effects of whiskers on the dark energy hypothesis it is important to study the characteristics of this form of carbon carefully so we can understand its impact on dark energy models. We'll then feed this data forward to the upcoming NASA and ESA (European Space Agency) missions that will look for the effects of dark energy."
Adapted from materials provided by Carnegie Institution, via EurekAlert!, a service of AAAS.
Email or share this story:
| More
Need to cite this story in your essay, paper, or report? Use one of the following formats:
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Carnegie Institution (2008, February 29). Graphite Whiskers, Rather Than Dark Energy, Could Explain Dimness Of Stellar Explosions. ScienceDaily. Retrieved August 24, 2009, from http://www.sciencedaily.com /releases/2008/02/080228143538.htm
Two closely orbiting violet-hot carbon-oxygen white dwarfs are spiraling into one another. The two stars are destined to merge, leading to carbon/oxygen fusion and a Type Ia supernova explosion. Graphite whiskers might be produced and dispersed into space by supernovae explosions. (Credit: Creative Commons License/Drew Taylor)
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Double Helix Life is God
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www.lavonn.net
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www.informarehpv.ro
Int. Diabetes Monitor
A free online review journal on trends in clinical diabetes.
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"How To Lose Belly Fat"
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Related Stories
What Can Swiss Cheese Teach Us About Dark Energy? (Dec. 28, 2008) — About 10 years ago, scientists reached the astonishing conclusion that our universe is accelerating apart at ever-increasing speeds, stretching space and time itself like melted cheese. The force ... > read more
NASA'S Swift Sees Double Supernova In Galaxy (June 27, 2007) — In just the past six weeks, two supernovae have flared up in an obscure galaxy in the constellation Hercules. Never before have astronomers observed two of these powerful stellar explosions occurring ... > read more
Cosmic Lighthouses: Astrophysicists Explain Differences In Brightness Of Supernova Explosions (Feb. 23, 2007) — Supernovae stand out in the sky like cosmic lighthouses. Scientists at the Max Planck Institute for Astrophysics and at the National Astronomical Institute of Italy have now found a way to use these ... > read more
New Class Of Dim Supernovae (June 7, 2009) — The colossal stellar explosions called supernovae come in many kinds and flavors. Some of them are produced when a massive star reaches the end of its life in a sudden gravitational collapse. ... > read more
Dark Energy May Be Vacuum (Jan. 16, 2007) — Researchers at the University of Copenhagen's Dark Cosmology Centre at the Niels Bohr Institute have brought us one step closer to understanding what the universe is made of. The new data shows that ... > read more
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Astronomers removed light from closer and better known galaxies and stars from pictures taken with the Spitzer Space Telescope. The remaining images. ... > full story
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