[earth science] u1 test

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48 Terms

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came into existence w/ the big bang

time matter and space

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antimatter

opposite electric charge, opposite magnetic moment, same mass and lifetime (of matter)

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formed when the universe began to cool down from protons and nuetrons

nuclei of hydrogen and helium

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hubbles law

galaxies are moving away from earth at speeds proportional to their distance, the further the galaxies are, the faster they move away

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cosmic microwave background radiation

faint remnant glow of the big bang

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big bang nucleosynthesis

formation of light and atomic nuclei within the first few minutes after the big bang when nuclear fusion occured

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doppler effect

apparent change in frequency of a wave caused by relative motion and source of the wave and observer
farther away a galaxy is, greater redshift, signifying a faster recession and speed from us

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redshift

hydrogens spectral lines, when a light source is moving away, its spectral lines are shifted toward the red end of the spectrum

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definition of a star

balls of gas made mostly of hydrogen, produce energy through nuclear fusion, classified by physical characteristics

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ways astronomers classify stars

color, temperature, size, chemical composition, luminosity, brightness

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what color and temperature reveal about a star

coolest stars appear red, hottest apear blue

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chemical composition

most stars made up of 73% hydrogen, 25% helium, and 2% other elements

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luminosity

total light energy output per second of an object that produces its own light, hotter stars produce more light

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brightness

related to how much light reaches a point per second

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hertzsprung-russel diagram

classify stars and how they change over time, 90% of stars are in the main sequence (including the sun)

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life of a star

determined by its mass

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all stars begin as a

nebula (large cloud of gas and dust that gravity pulls together to create a protostar)

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small mass stars

burn slowly, live longer

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when a star runs out of fuel it becomes a

redgiant or supergiant

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supernova

when a supergiant runs out of fuel and explodes suddenly

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nuetron stars

material left over from a supergiant explosion, very small, 3x the mass of the sun

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lifecycle of a low-mass star

nebula → main sequence → red giant → planetary nebula → white dwarf

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lifecycle of a high-mass star

nebula → main sequence → red supergiant → supernova ->[nuetron star (high) or black hole (very high)]

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stellar nucleosynthesis

stars produce elements through this, lighter elements fuse into heavier

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age of the sun

4.6 billion years old

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how much hydrogen has the sun burned through

about half with 5 billion years left

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how far away the sun is from earth

1 AU

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how much is 1 AU

93 million miles or 150 million kilometers

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how long it takes for light to reach earth

8 minutes 20 seconds

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the sun’s classification

g-type yellow dwarf main sequence star

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sun’s surface temperature

9,932 F

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revolution

orbiting around the milky way

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how long 1 revolution takes

230 million years

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sun’s radius

696,340 kilometers

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movement of the equator

25 days for one rotation

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movement of the poles

35 days for a full rotation

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layers of the sun

core → radiative zone → convection zone → photosphere → chromosphere → corona

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what happens in the core

where fusion occurs by combining hydrogen and helium

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what happens in the radiative zone

energy moves very slowly away from the core as photons (100,000 years to pass through)

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what happens in the convection zone

plasma heats up and rises, then it cools and sinks to transport heat towards the surface

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photosphere

visible surface of the sun, sunspots occur here

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chromosphere

thin reddish layer where temperatures start increasing, magnetic spicules happen here

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corona

outer atmosphere of the sun (over 1 million C), solar winds and coronal mass ejection occur here

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fusion

joining two or more things to create a single entity

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nuclear fusion

small nuclei join together to make larger nuclei, lots of energy released

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energy released as

heat and light

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location of heavier/denser elements

core because gravity pulls them in

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fusion only happens when

theres a high enough pressure and temperature