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came into existence w/ the big bang
time matter and space
antimatter
opposite electric charge, opposite magnetic moment, same mass and lifetime (of matter)
formed when the universe began to cool down from protons and nuetrons
nuclei of hydrogen and helium
hubbles law
galaxies are moving away from earth at speeds proportional to their distance, the further the galaxies are, the faster they move away
cosmic microwave background radiation
faint remnant glow of the big bang
big bang nucleosynthesis
formation of light and atomic nuclei within the first few minutes after the big bang when nuclear fusion occured
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
redshift
hydrogens spectral lines, when a light source is moving away, its spectral lines are shifted toward the red end of the spectrum
definition of a star
balls of gas made mostly of hydrogen, produce energy through nuclear fusion, classified by physical characteristics
ways astronomers classify stars
color, temperature, size, chemical composition, luminosity, brightness
what color and temperature reveal about a star
coolest stars appear red, hottest apear blue
chemical composition
most stars made up of 73% hydrogen, 25% helium, and 2% other elements
luminosity
total light energy output per second of an object that produces its own light, hotter stars produce more light
brightness
related to how much light reaches a point per second
hertzsprung-russel diagram
classify stars and how they change over time, 90% of stars are in the main sequence (including the sun)
life of a star
determined by its mass
all stars begin as a
nebula (large cloud of gas and dust that gravity pulls together to create a protostar)
small mass stars
burn slowly, live longer
when a star runs out of fuel it becomes a
redgiant or supergiant
supernova
when a supergiant runs out of fuel and explodes suddenly
nuetron stars
material left over from a supergiant explosion, very small, 3x the mass of the sun
lifecycle of a low-mass star
nebula → main sequence → red giant → planetary nebula → white dwarf
lifecycle of a high-mass star
nebula → main sequence → red supergiant → supernova ->[nuetron star (high) or black hole (very high)]
stellar nucleosynthesis
stars produce elements through this, lighter elements fuse into heavier
age of the sun
4.6 billion years old
how much hydrogen has the sun burned through
about half with 5 billion years left
how far away the sun is from earth
1 AU
how much is 1 AU
93 million miles or 150 million kilometers
how long it takes for light to reach earth
8 minutes 20 seconds
the sun’s classification
g-type yellow dwarf main sequence star
sun’s surface temperature
9,932 F
revolution
orbiting around the milky way
how long 1 revolution takes
230 million years
sun’s radius
696,340 kilometers
movement of the equator
25 days for one rotation
movement of the poles
35 days for a full rotation
layers of the sun
core → radiative zone → convection zone → photosphere → chromosphere → corona
what happens in the core
where fusion occurs by combining hydrogen and helium
what happens in the radiative zone
energy moves very slowly away from the core as photons (100,000 years to pass through)
what happens in the convection zone
plasma heats up and rises, then it cools and sinks to transport heat towards the surface
photosphere
visible surface of the sun, sunspots occur here
chromosphere
thin reddish layer where temperatures start increasing, magnetic spicules happen here
corona
outer atmosphere of the sun (over 1 million C), solar winds and coronal mass ejection occur here
fusion
joining two or more things to create a single entity
nuclear fusion
small nuclei join together to make larger nuclei, lots of energy released
energy released as
heat and light
location of heavier/denser elements
core because gravity pulls them in
fusion only happens when
theres a high enough pressure and temperature