It was recentlly learned that our sun likely coalesced from the gas in a globular cluster containing some 3000 stars, probably about 10 light years across. The first million years or so of the sun's existence it shone by the light of gravitational collapse, from the heat of colliding atoms. Once the sun's core temperature reached a critical threshhold, nuclear fusion began to occur, producing the light of a "true" sun.
The sun drifted around the galaxy, about once every 220 million years, some 20 times until now. It will continue to do so for another three or four billion years, at which time it will gradually begin getting larger and hotter. As the hydrogen fuel is consumed, it will expand fairly rapidly (over about a hundred thousand years) into a red giant. It will burn that way for awhile, liberating lots of heat, and then collapse into a small bright white dwarf. As a white dwarf it will burn several billion years more, eventually fading to a brown dwarf before blackening out altogether.
It's thought to be about halfway through its main squence life (burned half the avalable hydrogen) ,
so it's 4.5 billion years old ... and has about 5 billion years to go (before it turns into a red-giant and swallows the inner planets.
The next stage of the sun would be a red giant. It would expand to many times it's present size. It is about a million miles across. Then the fusion will cause it to expand to like a hundred million miles across or greater.
The sun is about half way through its life. it has been around for 4.5 billion years and has another 5 billion years until it dies.
our sun is a middle aged star. It's lived about half its life.
The Sun is estimated to be about 4.6 billion years old, and is expected to burn for another 5 billion years. This puts its expected lifetime at around 10 billion(10,000,000,000) years.
Our Sun is about half way through it's life. It is on the main sequence.
Main sequence
The Main Sequence stage.
The Sun is in the main sequence stage.
The Sun is approximately halfway through its main-sequence process of evolution.
The Sun is halfway through it's life whereas Antares is nearing it's end.
the sun is a cool wave
The red giant.
in star life cycle terms its pretty young
The Sun is approximately halfway through its main-sequence process of evolution.
It is approx half-way through its 10 billion year life cycle.
The Sun is halfway through it's life whereas Antares is nearing it's end.
It is commonly understood that the sun, at 4.567 billion years is in it's mid-life, or about 1/2 way through it's life expectancy.
middle age
I think ur a gay. when you die the sun will end on its life cycle! :D >>>Jushki
dubstep
the sun is a cool wave
Life on Earth is sustained through the flow of energy from the sun, the cycle of matter through the biosphere, and gravity. These factors are essential to all biotic processes.
from nuclear fusion on the surface of the sun when it went nova, but it was also formed by plant life through the calvin cycle
Well, evry life cycle starts with the sun. It depends. Like sun, monkey, banana, and a banana eats nothing.
Life cycle of a sun like star. A sun like star will start out as a nebula to a protostar to a main sequence star to a red giant and into a white dwarf and will simply fade out.