0
What else can I help you with?
What gas is exchanged into helium in a stars nuclear reactions?
In a star's nuclear reactions, hydrogen is converted into helium. This process, known as nuclear fusion, occurs in the core of a star, where high temperatures and pressures cause hydrogen atoms to combine to form helium.
Is the ratio of the amount of hydrogen and helium in the sun increasing or decreasing?
The ratio of hydrogen to helium in the sun has been decreasing over time as hydrogen is being converted into helium through nuclear fusion reactions in the sun's core. This process is gradually shifting the composition of the sun more towards helium.
What fuses during the red giant phase?
During the red giant phase, hydrogen fusion occurs in the shell surrounding the helium core. The core is no longer fusing hydrogen, as it has already converted most of its hydrogen into helium. This causes the outer layers of the star to expand and cool, leading to the red giant phase.
What Makes up 75 percent of the sun's mass?
Hydrogen. Actually the figure is closer to73.46% hydrogen. 24.85% is helium.
The sun's energy is released when what is converted into energy?
The sun's energy is released when nuclear fusion converts hydrogen atoms into energy. This process involves the fusion of hydrogen nuclei to form helium nuclei, releasing large amounts of energy in the form of light and heat.
What is the first element that is converted in a star's core?
The first element that is converted in a star's core is hydrogen. Through nuclear fusion, hydrogen atoms fuse together to form helium, releasing energy in the process. This fusion process is what powers a star and allows it to shine.
What gas is exchanged into helium in a stars nuclear reactions?
In a star's nuclear reactions, hydrogen is converted into helium. This process, known as nuclear fusion, occurs in the core of a star, where high temperatures and pressures cause hydrogen atoms to combine to form helium.
What is in the suns core?
helium and hydrogen
Is the ratio of the amount of hydrogen and helium in the sun increasing or decreasing?
The ratio of hydrogen to helium in the sun has been decreasing over time as hydrogen is being converted into helium through nuclear fusion reactions in the sun's core. This process is gradually shifting the composition of the sun more towards helium.
What fuses during the red giant phase?
During the red giant phase, hydrogen fusion occurs in the shell surrounding the helium core. The core is no longer fusing hydrogen, as it has already converted most of its hydrogen into helium. This causes the outer layers of the star to expand and cool, leading to the red giant phase.
What is the sun formed out of?
The Sun is made up mainly of hydrogen, less helium, and small amounts of heavier elements. Four hydrogen atoms fuse to from one helium atom, in this process a lot of energy & heat is released. The sun will remain stable until the whole hydrogen is converted into helium. When the total hydrogen is exhausted energy production stops in its core and thus the core starts shrinking.
Why do you have helium?
Helium exists because Hydrogen fuses into Helium in the core of hot stars.
Is the sun made up of mostly hydrogen?
Essentially yes; the sun's energy comes from nuclear fusion with hydrogen being converted to helium.
What Makes up 75 percent of the sun's mass?
Hydrogen. Actually the figure is closer to73.46% hydrogen. 24.85% is helium.
The sun's energy is released when what is converted into energy?
The sun's energy is released when nuclear fusion converts hydrogen atoms into energy. This process involves the fusion of hydrogen nuclei to form helium nuclei, releasing large amounts of energy in the form of light and heat.
Where in the sun is hydrogen fused into helium?
Hydrogen is fused into helium in the core of the sun, where temperatures and pressures are high enough to initiate nuclear fusion reactions. The core is where the sun's energy is produced through the fusion of hydrogen nuclei into helium nuclei.
What is the sun's iner core made of?
Hydrogen and helium
