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In the past it was a main sequence star. In the future it will be a giant star and will cool off.

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Q: Outline the history and probable future of your sun?
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What is the probable fate of our sun?

These phenomena, which are all related to the Sun's magnetic field, impact our near-Earth space environment and determine our "space weather" In the near future, the same as now.


can sun rays hurt people?

Probable not.


What is stating what will happen in the future?

What will happen in the future is that the sun will become a red giant and eventually explode.


What is the past and probable future of the sun?

The sun has been shining for about 4.6 billion years and is currently in the middle of its main-sequence phase, during which it fuses hydrogen into helium in its core. In about 5 billion years, it will exhaust its hydrogen fuel and start to expand into a red giant, eventually shedding its outer layers to form a planetary nebula. It will then cool and shrink into a white dwarf, eventually fading into a black dwarf over trillions of years.


What will happen to all life if the sun dies?

The most probable outcome is that there would be a HUGE Ice Age. yet that will not happen


Can the sun turn blue?

depends what space does in the future


What is the future tense of shine?

The future tense of "shine" is "will shine." For example, "The sun will shine tomorrow."


Who went to the sun?

no one ,,,went to the sun ,,, and i guranteed that in future also ,,no one can go ,,bcoz of high temperature of the sun


In what month is the sun closest to the sun?

January, i wish you good luck on all your future endeavors :)


Who wrote the art of war?

Sun Tsu wrote it, around 500BC. This is Chinese History, by the way, not European History


Is Stephenie Meyer continuing midnight sun?

Possibly in the future!


What is the exact mass of the sun?

The Wikipedia lists the mass as (1.98855±0.00025)E30 kilograms. The plus-minus, of course, refers to the probable error in the Sun's mass, as currently known. That means this mass is currently known with a probable error of about 0.01%.It is also necessary to realize that the mass of the sun is slowly but continuously decreasing. due mostly to the conversion of mass to energy in fusion (4.29E9 kilograms/second) but also the solar wind (~1E9 kilograms/second). Admittedly this mass loss is so small compared to the probable error in the total mass that it is usually ignored, but still it makes knowledge of "exact mass of the Sun" impossible.