What will happen when the Sun will run out of hydrogen in the core?

What will happen when the Sun will run out of hydrogen in the core?

When our Sun runs out of hydrogen fuel in the core, it will contract and heat up to a sufficient degree that helium fusion can begin. It will end composed of carbon and oxygen, with the lighter (outer) hydrogen and helium layers blown off. This occurs for all stars between about 40\% and 800\% the Sun’s mass.

How much mass will the Sun lose in solar masses as a result of hydrogen fusion over its lifetime?

A Lifetime of Mass Loss How much mass has the Sun lost over its lifetime? It loses about 5 or 6 million tons of material every second, and that sounds like a lot. The Sun is about 4.5 billion years old, and a year is about 31 million seconds long.

What happens when a star’s core runs out of hydrogen and why does this occur?

When the hydrogen supply in the core begins to run out, and the star is no longer generating heat by nuclear fusion, the core becomes unstable and contracts. The outer shell of the star, which is still mostly hydrogen, starts to expand. As it expands, it cools and glows red.

Is the Sun losing mass and hydrogen?

The Sun actually does lose mass in the process of producing energy. In units of tons, every second, the Sun’s fusion processes are converting about 700 million tons of hydrogen into helium “ashes”. In doing so, 0.7 percent of the hydrogen matter (5 million tons) disappears as pure energy.

What will happen to sun in future?

After fusing helium in its core to carbon, the Sun will begin to collapse again, evolving into a compact white dwarf star after ejecting its outer atmosphere as a planetary nebula. The predicted final mass is 54.1\% of the present value, most likely consisting primarily of carbon and oxygen.

How did they calculate the mass of the sun?

Knowing the mass and radius of the Earth and the distance of the Earth from the sun, we can calculate the mass of the sun (right), again by using the law of universal gravitation. By astronomically determining the distance to the sun, we can calculate the earth’s speed around the sun and hence the sun’s mass.

How much mass does the sun have?

1.989 × 10^30 kg
Sun/Mass

What happens when a star’s core runs out of hydrogen and why does this occur Brainly?

Once a star has exhausted its supply of hydrogen in its core, leaving nothing but helium, the outward force created by fusion starts to decrease and the star can no longer maintain equilibrium. The force of gravity becomes greater than the force from internal pressure and the star begins to collapse.

Is there hydrogen on the Sun?

About three quarters of the sun is hydrogen, which is constantly fusing together and creating helium by a process called nuclear fusion. Helium makes up almost the entire remaining quarter.

What happens to the missing mass in the Sun’s core?

matter can be converted into energy and energy can be converted into matter. where lighter nuclei are combined into heavier nuclei (ELEMENTS) and gives off energy . This fusion reaction turns the missing mass into energy for the sun.

When will the Sun run out of hydrogen?

But in about 5 billion years, the sun will run out of hydrogen. Our star is currently in the most stable phase of its life cycle and has been since the birth of our solar system, about 4.5 billion years ago.

Does the Sun have a finite amount of hydrogen in it?

However, this process cannot last forever since there is a finite amount of hydrogen in the core of the Sun. Currently it has more than 72\% hydrogen. One billion years from now, the Sun will be 10\% brighter than it currently is.

What would happen if the Sun had 10 times its mass?

If, however, the Sun had about 10 times its current mass, the final phase of its lifespan would be significantly more (ahem) explosive. When this super-massive Sun ran out of hydrogen fuel in its core, it would switch over to converting atoms of helium, and then atoms of carbon (just like our own).

What will happen to the Earth when the Sun dies?

It will cool down over billions of years until it reaches the very same temperature as with the universe. Other astronomers theorize that in about 5 billion years, when the Sun has depleted its hydrogen fuel, other gases will be out of control, especially the helium, which shall make all objects here on Earth to melt down and burn.