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helium flash

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(astronomy) The sudden beginning of the burning of helium in the core of stars of intermediate mass or on the surface of an accreting white dwarf.

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combustión explosiva de helio

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flash del helio

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The helium flash did not happen.
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"Sakurai's Object—A Possible Final Helium Flash in a Planetary Nebula Nucleus".
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The eyes of Tara of Helium flashed, but she made no comment.
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Sir, it' s a helium flash
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It is located at the center of a planetary nebula and is believed to currently be in thermal instability and within its final shell helium flash phase.
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As above, the gravitational hold on the upper layers is weakened, and they may be shed into space by violent events such as the beginning of a helium flash in the core.
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Red giant Red supergiant Betelgeuse Coronal mass ejection Helium flash Seeds, Michael A., Astronomy: The Solar System and Beyond, Brooks/Cole 2005 Simulation of a Red Supergiant displaying instability and mass loss
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When it does happen, the only warning that we' re likely to get... is a fast helium flash, at which point we' il have to jump out of here... before it obliterates the entire planetary system
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When a star runs out of hydrogen fuel it undergoes an enormous expansion during which its volume increases by a factor of a few millions and the outer layers of the star are expelled in a 'helium flash'.
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Finally, when the temperature increases sufficiently, helium fusion begins explosively in what is called a helium flash, and the star rapidly shrinks in radius, increases its surface temperature, and moves to the horizontal branch of the HR diagram.
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During these shell helium flashes, the mass loss from the star is significant, and after many shell helium flashes, an AGB star is transformed into a hot white dwarf and its atmosphere becomes material for a planetary nebula.
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When the degenerate core reaches a critical mass of about 0.45 solar masses, helium fusion is ignited and takes off in a runaway fashion, called the helium flash, briefly increasing the star's energy production to a rate 100 billion times normal.
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'The exciting thing about finding a planet around this star is that it indicates that planetary systems can survive the giant phase and the helium flash of their parent star,' commented Steve Kawaler of Iowa State University, one of the authors of the paper.
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However, over periods of 10,000 to 100,000 years, helium from the hydrogen shell burning builds up and eventually the helium shell ignites explosively, a process known as a helium shell flash.
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Low mass stars (including the Sun), with a mass between 0.5 M☉ and 1.8–2.5 M☉ depending on composition, do become red giants as their core hydrogen is depleted and they begin to burn helium in core in a helium flash; they develop a degenerate carbon-oxygen core later on the asymptotic giant branch; they finally blow off their outer shell as a planetary nebula and leave behind their core in the form of a white dwarf.
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It was then flash-frozen in liquid helium before it could chemically self-destruct.
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Intermediate-mass stars, between 1.8–2.5 M☉ and 5–10 M☉, pass through evolutionary stages similar to low mass stars, but after a relatively short period on the red giant branch they ignite helium without a flash and spend an extended period in the red clump before forming a degenerate carbon-oxygen core.
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The explosive nature of the helium flash arises from its taking place in degenerate matter.
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The Sun has become unstable and it's been predicted that, in a few years, a helium flash will completely burn all the planets of the solar system.
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The object is actually a small white dwarf star undergoing a helium flash — one of only a handful of examples of such an event ever witnessed by astronomers.
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If that is the case, the outburst may have been a so-called helium flash, a thermonuclear event where a shell in the star containing helium suddenly ignites and starts to fuse carbon.
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If that is the case, the outburst may have been a so-called helium flash, a thermonuclear event where a shell in the star containing helium suddenly ignites and starts to fuse helium.
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In some cases, however, the star reignites in a helium flash and expands to return to a red giant state, ejecting huge amounts of gas and dust in the process, before once again shrinking to... Read more
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The brightening may have been a so-called helium flash, where the core of a dying low-mass star suddenly ignites helium fusion disrupting, but not destroying, the star. Such an event is known to have occurred in Sakurai's Object.
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In the first one, a final helium shell flash occurs on a cooling white dwarf star or a very late thermal pulse is experienced by a post-AGB star.
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32 sinne gevind in 18 ms. Hulle kom uit baie bronne en word nie nagegaan nie.