big bang theory and stars

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30 Terms

1
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stellar nebula

A cloud of gas and dust where stars are born

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main sequence star

A normal star that is undergoing nuclear fusion. Our sun is an example of this.

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massive star

A star that is much larger than a Sun-like Star; will blow up in a supernova and end as a neutron star or black hole

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average star

produces own heat/light, average mass, includes main sequence stars

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hertzsprung diagram

organizes the family of stars into a diagram; across bottom is star's temperature and side is star's absolute magnitude; a star's temperature and color depend on how big the star is

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super red giant

A massive star that has stopped hydrogen fusion

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fusion

Creation of energy by joining the nuclei of two hydrogen atoms to form helium.

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red giants

a large old reddish star that has greatly expanded and cooled as its fuel (hydrogen) has begun to run out

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supernova

A gigantic explosion in which a massive star caves in and throws its outer layers into space

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planetary nebula

A huge cloud of gas that is created when a red giants loses all its fuel

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neutron star

the small, dense remains of a high-mass star after a supernova

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black hole

An object in space whose gravity is so strong not even light can escape.

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white dwarf

A small, hot, dim star that is the leftover center of an old star

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black dwarf

A white dwarf that has burnt out completely.

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big bang theory

The theory that the universe originated in a huge explosion that released all matter and energy.

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singularity

A point in which matter is infinitely dense, as in the center of a black hole or the universe at the very beginning.

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steady state theory

a theory which states that there was no beginning to the universe and that the universe does not change in appearance.

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1/10^43 seconds after the big bang

the universe is beginning to expand and is extremely hot

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1/10^34 seconds after the big bang

universe is the size of a pea, lots of energy and light. as well as cooling beginning to occur

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1/10^4 seconds after the big bang

protons and neutrons begin to form

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1/100 seconds after the big bang

universe now the size of the solar system

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1 second after the big bang

1 trillion, trillion kilometers across in length, at 10 billion degrees celsius

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5 minutes after the big bang

the nuclei of the first three elements form: hydrogen, helium, and small amounts of lithium

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300,000 years after the big bang

atoms finally form as electrons slow down. universe has cooled tremendously

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200 million years after the big bang

first stars and planets form

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doppler effect

An observed change in the frequency of a wave when the source or observer is moving

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red shift

the change in the wavelength of light due to an object moving away from the observer (red moving away and blue moving towards)

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cosmic microwave background radiation (cmb)

A faint glow of light that fills the universe, falling on earth from every direction with nearly uniform intensity. leftovers from the big bang. cannot be seen.

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hydrogen and helium

two most abundant elements in the universe

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photon

particle of light