Astronomy Chapters 14-18 – Flashcards

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states that laws of physics are the same everywhere
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cosmological principle
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idea where galaxies in space are distributed similarly everywhere
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homogeneous
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idea where the universe looks the same to all observers regardless of the direction in which they are looking
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isotropic
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a gravitationally bound large collection of stars, gas, and dust
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galaxy
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spirals, ellipticals, irregulars
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types of galaxies
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___ galaxy shape: flattened and thin
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spiral
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___ galaxy shape: oval or football-shaped
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elliptical
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galaxy classification with bright center, tight arms
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Sa/SBa
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small center, open arms
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Sc/SBc
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galaxy classification: cross between S and E, disk with no arms
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S0
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area of a spiral galaxy where stars orbit in all directions
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central bulge
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___ galaxy features: little gas, mostly hot, no star formation, golden color
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elliptical
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___ galaxy features: abundant gas, mostly cold, star formation is ongoing, blue color
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spiral
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___ galaxy features: lots of gas, ongoing star formation
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irregular
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___ galaxy size: dwarf or giant
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elliptical and irregular
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___ galaxy size: giant
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spiral
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location of young, hot, bright stars
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spiral arms
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this is located in the spiral arms
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concentrated gas and dust
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cannot produce all the gravity observed in a galaxy
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luminous matter
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an additional source of gravity that does not make light
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dark matter
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do not decrease as a function of radius
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rotation speeds
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this percentage of mass is dark matter
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95%
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located around the galaxy (completely surrounding it)
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dark matter halo
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allows astronomers to look for mass that is not visible
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gravitational lensing
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massive compact halo objects
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MACHOs
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weakly interacting massive particles
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WIMPs
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a compact region at the center of a galaxy that has a much higher than normal luminosity
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AGN (active galactic nuclei)
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quasi-stellar radio source; center of violent activity in the hearts of large galaxies
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quasar
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low-luminosity cousins of quasars
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Seyfert galaxies and radio galaxies
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central supermassive black hole with an accretion disk
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AGN model
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masses of thousands to tens of billions of solar masses
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supermassive
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material in the accretion disk fuels ___
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AGN
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provide evidence that galaxies are moving away
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redshifts
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states that the recession velocity of a galaxy is proportional to the distance of that galaxy
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Hubble's Law
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constant of proportionality
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Hubble constant (H0)
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the Hubble constant determines ___
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the age of the universe
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these are used as luminous standard candles
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Type 1a supernovae
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70 km/s/Mpc
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H0
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dusty gas clouds that obscure our view
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interstellar medium
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result when interstellar dust blocks shorter wavelengths more efficiently
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interstellar reddening
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emits radio waves =21 cm
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neutral hygrogen
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example of barred spiral galaxy with elongated bulge
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Milky Way
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tightly gravitationally bound collections of up to a million stars
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globular clusters
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location of globular clusters
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spherical halo
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___ star sizes: RR Lyrae and Cepheid variable stars
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globular cluster
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___are found by looking at globular clusters
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distances
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distance from Solar System to the center
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27,000 ly
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distance across the whole Milky Way
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100,000 ly
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Milky Way + halo
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300,000 ly
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the age of globular clusters
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13 billion years old
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loosely bound collections of dozens to thousands of stars in the disk of a spiral galaxy
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open clusters
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younger
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open clusters are ___ than globular clusters
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first
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stars in the halo formed
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heavier
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younger stars have ___ elements
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process where gas is ejected from the disk by hot young stars and supernovae and then falls back onto the disk
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galactic fountain model
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high-energy, charged particles moving near the speed of light
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cosmic rays
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extend 25,000 ly above and below the galactic plane
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gamma ray bubbles
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Milky Way plus a few large and dwarf galaxies
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Local Group
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takes time for light from distant object to reach us
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look-back time
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the term for the time when separation between galaxies was zero
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Hubble time
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hot and dense
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early universe was
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energy that cooled into matter as the universe cooled
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beginning of the universe had
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evidence that everything is expanding
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cosmological redshift
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this explains why space glows in microwaves at 3 K
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CMB (cosmic microwave background) radiation
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temperature of the universe cooled enough for H atoms to form; like a fog being lifted
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recombination
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smoothness of the universe (CMB variations) has ___ over time
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decreased
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ratio of the critical density
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Ωmass = p/pc
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density equals the critical density; universe slows to stop at infinite time
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Ωmass = 1
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formula where expansion will stop and universe will contract
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Ωmass > 1
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formula where expansion will go on forever, slowing but never stopping
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Ωmass < 1
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0.3
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Ωmass (including stars, galaxies, and dark matter)
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energy that allows expansion to speed up
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dark energy
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Λ; associated with dark energy
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cosmological constant
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photons, particles, anti-particles
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early universe composition
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electromagnetic force
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QED
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gravity, electromagnetic, weak nuclear, strong nuclear
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four forces of the universe
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QED + weak
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electroweak
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combination of the ideas in QCD (strong) and electroweak
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standard model
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strong force + electroweak force; predicts proton decay
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grand unified theory (GUT)
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GUT + gravity
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theory of everything (TOE)
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name for other universes
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multiverse
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gravitationally bound collections of hundreds of thousands of galaxies
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galaxy clusters
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bunches of galaxy clusters
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superclusters
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clusters are bright in ___
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x-rays (rich in hot gas)
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formed via gravitational lenses; able to see the distorted images of background galaxies
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visible arcs
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universe is homogenous and isotropic
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large-scale structure
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process where small objects formed first, then grouped together
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hierarchical clustering
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process where collisions between protons (hydrogen nuclei) in the early universe formed low-mass nuclei (deuterium and isotopes of helium, lithium, beryllium, and boron)
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Big Bang nucleosynthesis
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all elements more massive than ___ formed in stars
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boron
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slow speeds compared to C; unknown elementary particles
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cold dark matter
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moving rapidly; neutrinos from Big Bang
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hot dark matter
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location of the formation of the first stars
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dark matter mini-halos
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size of the first stars
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very massive
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these build up to make larger galaxies
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protogalaxies
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the merging of many small galaxies triggers a ___
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supermassive black hole
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___ galaxy evolution: the merging of spiral galaxies
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elliptical
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this event heats up gas and emits x-rays
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merging of galaxy clusters
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complex biochemical process that draws energy from its environment to survive and reproduce
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life
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scientists who created molecules with an experiment similar to the primordial Earth
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Miller and Urey
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lightning, hydrothermal vents, UV radiation
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possible energy sources
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when life began
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3.5 billion years ago
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dating process where one infers that the deeper layers formed earlier
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relative ages
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radiometric dating
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absolute ages
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these release oxygen via photosynthesis
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cyanobacteria
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540-500 million years ago; explosion of new species due to climate change and increase in genetic diversity
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Cambrian Explosion
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composition of all terrestrial life
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carbon, hydrogen, oxygen, and nitrogen (CHON)
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the three necessities for life
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nutrient source, energy, liquid water
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region around a star that provides a range of temperatures in which liquid water can exist
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habitable zone
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hotter stars have ___ habitable zones
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larger
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multiply the number of stars in our galaxy, fraction of stars with planets, average number of planets per star, fraction of planets with life, fraction that develop advanced technology
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Drake equation
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surveys as many as a million stars per year to search for life
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ATA (Allen Telescope Array)
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states that civilizations should be common; even 1 in 1 million stars = 100,000 civilizations; but we still haven't detected them
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Fermi's Paradox
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