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## How does a main sequence star stay stable?

For most of its lifetime, a star is a main sequence star. It is stable, with balanced forces keeping it the same size all the time. radiation pressure from the fusion reactions tends to expand the star. forces caused by gravitational attraction and fusion energy are balanced.

## How the sun is able to maintain a stable size?

EXPLAIN how a main sequence star like the sun is able to maintain a stable size. Answer: The nuclear fusion rate increases as the gravity pressures the star. But the energy radiated from fusion reactions heats the gas inside the star. The outward pressure of radiation resists the inward pull of gravity.

## How do stars maintain their stability?

You can imagine a star as a series of layers. The inward force of gravity is balanced out by the outward force of pressure to keep the star stable. This stable balance, the outward pressure of hot gases balancing the inward pull of gravity is called the hydrostatic equilibrium.

## What allows a main sequence star to remain stable in size against gravity?

A star on the main sequence is stable because it is steadily fusing hydrogen into helium in the core. There is a force balance in the star (outward force equals the inward force). While self-gravity pulls the star inward and tries to make it collapse, thermal pressure (heat created by fusion) pushes outward.

## What happens when a star bigger than the sun’s core collapses?

The fate of the left-over core depends on its mass. If the left-over core is about 1.4 to 5 times the mass of our Sun, it will collapse into a neutron star. If the core is larger, it will collapse into a black hole. Only stars with more than 20 times the mass of the Sun will become black holes.

## Why does the size of a star remain stable?

During the main sequence period of its life cycle, a star is stable because the forces in it are balanced. The outward pressure from the expanding hot gases is balanced by the force of the star’s gravity. Gravity pulls smaller amounts of dust and gas together, which form planets in orbit around the star.

## What is the life cycle of a Sun sized star?

And like all stars, it has a lifespan, characterized by a formation, main sequence, and eventual death. This lifespan began roughly 4.6 billion years ago, and will continue for about another 4.5 – 5.5 billion years, when it will deplete its supply of hydrogen, helium, and collapse into a white dwarf./span>

## Is the sun stable?

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. Once all the hydrogen gets used up, the sun will grow out of this stable phase. For about a billion years, the sun will burn as a red giant./span>

## Is the sun a stable star?

The sun is currently classified as a “main sequence” star. This means that it is in the most stable part of its life, converting the hydrogen present in its core into helium. For a star the size of ours, this phase lasts a little over 8 billion years./span>

## Is the sun growing or shrinking?

The sun is growing. And shrinking, and growing again. Every 11 years, the sun’s radius oscillates by up to two kilometres, shrinking when its magnetic activity is high and expanding again as the activity decreases. We already know that the sun is not a static object./span>

## Does our Sun have a name?

Although it’s a star – and our local star at that – our sun doesn’t have a generally accepted and unique proper name in English. We English speakers always just call it the sun. You sometimes hear English-speakers use the name Sol for our sun. Sol is the Roman equivalent of the Greek sun god Helios./span>

## Can other stars be called Suns?

Are all of the points of light in the night sky, other than the moon, planets, and artificial satellites, that we call stars also suns? In that case, the answer is “No, not quite.” Planets are very common around other stars, orbiting as many as 30 percent of stars similar to the Sun./span>

## Why is the sun no longer yellow?

tl;dr: The theory to explain this is the sun just underwent some kind of torsion and is no longer a yellow dwarf star. This has some bonus creepy conspiracy vibe because it might mean carbon dating is wildly inaccurate if the sun can change forms so flippantly.

## Is the sun brighter in space?

How much of the Sun’s visible light will reach your eyes, will vary depending on your location, the time of day and the constituents of the atmosphere through which the Sun’s light is passing. But it is safe to say that the Sun will look brighter from space. In space, there is nothing between your eyes and the Sun.

## Why doesn’t the sun brighten space?

Yes, Leo Cutter is right, the sun does not light up space because there is nothing there to light up. At night, we see darkness because the light of the sun is gone. Therefore, we can assume that where there is no light, there is darkness. Our sun is like many of the stars that we see at night.

## Can the human eye see stars in space?

You can see millions of stars from space with your naked eye, but when you take photographs in space and have something bright in the frame like a spacecraft, spacesuit, or lunar soil, you have to stop the exposure way down to prevent overexposure.

## How far can the human eye see?

Based on the curve of the Earth: Standing on a flat surface with your eyes about 5 feet off the ground, the farthest edge that you can see is about 3 miles away./span>

## How far can humans see into space?

30 billion light-years away

2021-05-14