Thermonuclear fusion of hydrogen occurs during the red giant phase. Helium to carbon fusion, or dredge up, also occurs at this time.
All red giant stars will start helium fusion when their core is compressed.
When aÊstar completes it's Red Giant phase they become White Dwarfs. The Red Giant phase of stars takes about a billion years.
Red giant is a type of star.
The Sun is a G-type main sequence star. The Sun is 4.5 billion years old and will continue to fuse hydrogen into helium for approximately another 5 billion years. At this point the Sun will leave the main sequence as strong convection currents arise, becoming a red giant. During it's red giant phase, the Sun will fuse helium into heavier elements such as carbon.The outer layers of the Sun will escape as a planetary nebula, marking the end of the red giant phase. The core of the Sun will cool and contract, becoming a white dwarf.
Hadar is in its giant stage.
Thermonuclear fusion is still going on in the core of a red giant, but it is a different type of thermonuclear fusion. The center of the core has reached high enough temperature and pressure that it can now burn helium, producing carbon. 3 4He --> 12C The large amount of energy released by this type of fusion pushes the outer layers away, making a giant star. The expansion of volume of the surface layer causes it to cool, appearing red. Thus a red giant.
helium capture
A fusion reaction.
A Lunar eclipse occurs only when the moon is in its full moon phase.
All red giant stars will start helium fusion when their core is compressed.
red giant (k12)
When aÊstar completes it's Red Giant phase they become White Dwarfs. The Red Giant phase of stars takes about a billion years.
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.
It is a star that has entered the super-giant phase. Its stellar classification is K2 1b.
This physical change is called freezing.
Fusion is a type of
Nuclear fusion is the type of nuclear reaction that occurs in stars. Older stars with a collapsing center can exceed a temperature of one hundred million Kelvin.