The Sun will continue as a stable star for at least as long as its supply of hydrogen lasts. (Hydrogen nuclei are fused together to form helium in its core, with energy given off).
This is predicted to be for the next 4-5 billion years. By the end of that time, the Sun will begin to fuse helium, and as a result, expand in diameter to perhaps 300 times its present size.
After it burns out its helium, it will begin to reduce in size, then cool. That process will probably take another 5-8 billion years.
It is probably safe to say that the Sun can support life on Earth fairly well for at least another 3 billion years, possibly more.
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Current scientific research suggests that because the Sun is getting hotter, we may not have more than a billion years left as a species
The Sun is about 4.6 billion years old and is estimated to have a total lifespan of about 10 billion years. It is currently in the middle of its main sequence phase where it is converting hydrogen into helium through nuclear fusion. It is expected to continue shining for another 5 billion years before evolving into a red giant and eventually a white dwarf.
Our sun is just about in the middle of its lifespan. It will die in roughly 5 billion years.
Our Sun is about 5 billion years old, and can be expected to continue along pretty much as it has for another 5 billion years.
A star with a mass of 2solar masses, 2times the mass of the sun, would have a main-sequence stage of half the life of a star with the mass of our sun. More massive stars die faster, less massive stars live longer and therefore have longer main-sequence stages.
The life expectancy of a star (E) depends on its mass (M), roughly following the model of E = M-2.5. For a star with a mass twice that of our sun (enter 2 in place of `M`), then the lifespan will give 0.177. Our suns lifespan is around 10 billion years, so this would equate to 1.77 billion years.
About the same as our Sun. About 10 billion years.
Our sun is just about in the middle of its lifespan. It will die in roughly 5 billion years.
The Sun is about 4.6 billion years old and is estimated to have a total lifespan of about 10 billion years. It is currently in the middle of its main sequence phase where it is converting hydrogen into helium through nuclear fusion. It is expected to continue shining for another 5 billion years before evolving into a red giant and eventually a white dwarf.
Our Sun is an average star and it has an approximate lifespan of
Our Sun is an average star and it has an approximate lifespan of 1 second
Our Sun is about 5 billion years old, and can be expected to continue along pretty much as it has for another 5 billion years.
Because their total lifespan is very short.
Total Eclipse of the Sun was created in 1999.
A star with a mass of 2solar masses, 2times the mass of the sun, would have a main-sequence stage of half the life of a star with the mass of our sun. More massive stars die faster, less massive stars live longer and therefore have longer main-sequence stages.
The life expectancy of a star (E) depends on its mass (M), roughly following the model of E = M-2.5. For a star with a mass twice that of our sun (enter 2 in place of `M`), then the lifespan will give 0.177. Our suns lifespan is around 10 billion years, so this would equate to 1.77 billion years.
um... the lifespan of the sun is 12 billion years, we are about half way to the 12 billion mark. (a little less). I think about 4.2 billion years old. The sun will engulf mercury and venus in the last 2 billion years of its life span, then it will either burn out or explode. If it has a higher mass, then it would explode then turn into a black hole! whopee...
That's what "total" means. If it doesn't completely cover the Sun, it's not a total eclipse.