A helium flash occurs because the core of the star is in what is known as a "degenerate" state. This means that the core has contracted so much that the pressure of the electron shells of the atoms making up the core prevent the core from contracting further. Under normal gas conditions (i.e. NOT a degenerate state), an increase in the temperature of the core would cause an increase in core pressure resulting in the core expanding and the temperature then dropping. This state is known as hydrostatic equilibrium. With a degenerate core, the temperature increases but the pressure doesn't. This extra energy ignites the helium creating run-away nuclear reactions. This is what is referred to as a "helium flash."
Helium is a colorless gas that is commonly used to fill balloons to make them float. It is lighter than air and non-flammable, making it safe for use in balloons.
The symbol of Helium is He. Helium's atomic number is 2.
The symbol for hydrogen is H, and the symbol for helium is He.
AnswerThere are two variants of helium -- helium 3 and helium 4. Helium 4 is not magnetic but helium 3 is. Its magnetism is, however, of different nature than e.g. that of iron. The magnetism of helium 3 is used for medical lung imaging.
No, helium gas is not a compound. Helium is an element, which means it consists of only one type of atom.
A helium flash occurs in low-mass stars during the helium burning phase. High-mass stars do not experience a helium flash because they have a higher core temperature and pressure, so helium burning begins smoothly without the need for a sudden ignition event. Additionally, high-mass stars have higher energy production rates, which prevent the conditions required for a helium flash from occurring.
The helium flash converts helium nuclei into carbon nuclei through the fusion process in the core of a star. This process occurs in stars with a mass greater than about 0.8 times the mass of the Sun during the later stages of helium burning. The intense energy released during the helium flash helps stabilize the star against gravitational collapse.
The helium flash in stars of solar masses typically lasts only a few hours to a few days. During this short-lived event, helium is rapidly converted into carbon and oxygen in the star's core, leading to a release of a significant amount of energy.
The luminosity of a low mass star goes down after helium flash. The sudden onset of helium fusion stops core shrinkage and the low-mass star will become smaller, and less luminous than it was as a red giant.
The helium flash occurs during the evolution of a star when the core of the star reaches a high enough temperature for helium fusion to begin, typically after the star has exhausted its hydrogen fuel in the core.
Well, happy little clouds! The helium flash occurs in stars when helium accumulates in the core and reaches a critical temperature where nuclear fusion suddenly ignites, creating a burst of energy. Just like a beautiful sunrise painting, this process helps our stars to continue shining bright and bringing light to the universe. Every bit of knowledge we gain about these cosmic wonders helps us appreciate the beauty of the stars even more.
Well, it's like bringing colors to the canvas – the helium flash happens in a star's core when helium fuses into carbon and releases a sudden surge of energy, causing the core to expand. This expansion is all part of the star's natural process towards a more stable phase, much like adding layers to create a beautiful and harmonious painting. Remember, nature always finds its way to balance and beauty.
Lower-mass stars do not have enough pressure and temperature at their cores to trigger the carbon flash phenomenon, which is necessary for carbon to begin fusion into heavier elements. Carbon flash occurs in higher-mass stars that have undergone helium fusion to build up a core of carbon. Lower-mass stars typically do not reach this stage of fusion.
Helium is a colorless gas that is commonly used to fill balloons to make them float. It is lighter than air and non-flammable, making it safe for use in balloons.
As a G-type star fuses its hydrogen to helium, this helium will gather in the core. As a result, the core will contract under its own weight as hydrogen is being spent. The contraction causes an increased hydrogen fusion rate, increasing the temperature. When insufficient hydrogen remains in the core, the layers above are no longer supported by the outward pressure of radiation, and collapse on top of the core, causing it to contract further, and also initiating hydrogen fusion outside the core. At this point, the star leaves the main sequence, and becomes a red giant. At this stage, the core of the giant may reach critical density for helium fusion to initiate. Since the core is composed of mostly degenerate matter at this stage, there is no regulation of the fusion rate. Also, degenerate matter is less opaque to the energies produced than non-degenerate matter, so conducts them better.Ehr, to summarize: the helium flash occurs during the red giant stage of G-type stars.
If you are comparing two balloons side by side, a hydrogen balloon will have more lift than a helium balloon of the same size and construction.If you open the balloons, the hydrogen is flammable, while the helium is not.
He - Helium