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Equivalence principle
Being in free fall is equivalent to being in a zero-gravity space (elevator example)
Evidence for Einstein’s theory of gravity
In Newton’s description of gravity, light shouldn’t bend due to gravity because it has no mass, but it does. Einstein’s theory says that objects with a lot of mass bend spacetime, and that’s why light bends near massive objects
Spacetime
There are three dimensions of space and one dimension of time, space and time are not separate like we think they are. Stronger gravity = slower pace of time
How Mercury supports Einstein’s theory
Mercury’s orbit is very eccentric and the orientation of the major axis changes (orbital procession). Astronomers used to think that there was another planet affecting its orbit named Vulcan, but that didn’t exist. Einstein’s theory was able to predict Mercury’s orbit using his theory of gravity
What prevents objects from collapsing
Earth - it’s hard to compress rocks
The Sun - pressure from nuclear explosions
White dwarfs - it’s hard to compress electrons together
Neutron stars - it’s hard to compress neutrons together
Black holes - no known force can fight gravity strong enough to create a black hole
Schwarzchild radius
Radius from which light cannot escape a black hole, also called an event horizon
R = 2GM/c², determines the radius of a black hole using its mass, can also be used to find the size of an object if it were a black hole
Gravitational lensing
Direction of light around a black hole changes and gets brighter, causes objects to appear brighter or in a different place
Photon sphere
Area around the black hole where light particles can remain in orbit
Spaghettification
Our best guess for what happens beyond the event horizon. Tidal forces are shallower at the surface of the black hole, so the bottom of the object is pulled in faster than the top and the object gets stretched out
Evidence for black holes
We can see weird motion of objects around them, we can see accretion disks around them, they create ripples in spacetime called gravitational waves, and also we have a picture now
Parts of the Milky Way galaxy
Halo - in the middle, contains almost entirely old, metal-poor stars from when the galaxy first formed
Disk - includes every kind of star
Spiral arms - part of the disk, formed because of differential rotation and because the arms had self-gravity
Galactic year
How long it takes the Sun to go around the galaxy - 225 million years
Weight of the galaxy
100 billion solar masses, estimate based on Kepler’s third law
Dark matter
A model that explains why everything in the galaxy is moving quickly. The stars furthest from the center should be moving slower than the stuff in the middle, but it’s not, so either our theory of gravity is wrong, or the galaxy is filled with matter we can’t detect
Sagittarius A* (Sgr A*)
The supermassive black hole at the center of the Milky Way galaxy, has a mass of 4 million Suns. One star orbits it at 124 AU
Why accretion disks around black holes are bright
The black holes pull matter in so fast that it lights up
Why accretion disks around black holes look like two circles
There’s only one accretion disk, but gravitational lensing makes it look like two
Population I stars
Bright blue stars in spiral arms of the galaxy (can also be yellow, red, and white, but blue stars are much more luminous), 0-12 billion years old, more heavy elements. Orbits are usually on the disk
Bright supergiants, main sequence stars, open clusters
Population II stars
Stars in halos, RR Lyrae stars, and globular clusters, but also found everywhere in the galaxy, 10-14 billion years old, not as many heavy elements. Orbits don’t have to be on the disk
Why young stars have more heavy elements than old stars
Old stars process the hydrogen and helium into heavier elements through fusion, and then they release it as supernovae or planetary nebulae. Young stars form from the enriched gas
Model of galaxy formation
Spherical blob of gas → starts collapsing → first stars form → forms a rotating disk → more stars form
Origin of the Big Bang Theory
Einstein’s theory of gravity predicts that the universe should either be expanding or contracting, but he didn’t believe it until Hubble discovered that it is actually expanding because he observed the redshift of the galaxies moving away from us. If we rewind expansion, everything had to be really close together at some point in the past, and that’s the Big Bang
Hubble’s constant
H = 70 km/s/Megaparsec (one million parsecs), used to estimate the age of the universe
How we know the expansion of the universe is accelerating
Astronomers used supernovae as standard candles and saw that they were accelerating away from us
Dark energy
A model that explains why the universe’s expansion is accelerating when it should be collapsing due to gravity. We have no idea where it comes from, what it is, or why it’s happening
Cosmological redshift
When wavelengths from everything get longer due to the expansion of the universe
Raisin bread model of the universe
The bread = space and the raisins = galaxies. The bread is getting bigger and the raisins are staying the same size but getting further apart
Models of the universe
No expansion, decelerating expansion (U shape), constant expansion (V shape), accelerating expansion (Y shape)
Big freeze
Aka “heat death”, everything separates and no stars form
Big rip
Expansion is stronger than nuclear forces that hold nucleons and electrons together, so atoms split apart
Big crunch
Everything clumps together, space gets tighter, atoms and subatomic particles crunch together
Big bounce
Big crunch and big bang cycle repeats over and over again
Critical density
Density needed for the universe to expand forever and not contract
3H² / 8𝜋G
Matter = 30%, dark energy and dark matter = about 70% (estimate)
Models for ages of galaxies
Light from far galaxies has to travel further, so it’s redshifted more and we can use a model to estimate its age. 0 redshift = now, higher redshift = older
Primeval fusion model (or Big Bang nucleosynthesis)
No fission but a period of nuclear fusion. Started with about 75% hydrogen, 25% helium, and a little bit of lithium
Deuterium
Isotope of hydrogen with a proton and a neutron instead of just a proton, heavier than hydrogen
Timeline of the beginning of the universe
T = 0.01 seconds: soup of matter and radiation, particles collided all the time, temperature was hot enough to turn light into an electron when photons collided
T = 3 minutes: atomic nuclei formed because high energy photons stopped breaking up nuclei
T = 300,000 years: universe was no longer ionized and electrons could bind to protons, universe became transparent
T = 400 million years: first stars form
Cosmic microwave background
Microwave radiation from all directions, redshifted because it’s from the Big Bang. Insanely uniform (2.73 Kelvin, 2 mm photons in every direction and 1 part in 100,000 is different from those measurements). Good confirmation that the universe evolved from a hot initial state, matches perfectly with predictions
Fluctuations in CMB
Seeds of galaxies. If there were no fluctuations, the atoms would be evenly spaced throughout the whole universe
Standard model of cosmology
Universe age = 13.8 billion years
Hubble constant and fractions of visible matter and dark energy/matter are also included
Universe contents that we know of
Luminous matter = 1%
Hydrogen, helium, ISM = 4%
Dark matter = 27%
Dark energy = 68%
WIMPs
Weakly interacting massive particles, a model for dark matter
Cosmological inflation
Attempt at explaining why the universe is flat, homogenous, and close to the critical density, says that the universe had a phase of very rapid expansion at 10^-35 seconds
Anthropic principle
Physical laws must allow for the existence of humans because humans have to be around to document the physical laws
Copernican principle
There is nothing special about our place in the universe
Fermi’s paradox
If alien life is common, we should expect to see evidence of them
Possible explanations for Fermi’s paradox
Life is not common
Life is common, but intelligent life is rare
Intelligent life is common, but we can’t detect their signals
Intelligent life is common, but they’re leaving us alone on purpose
Maybe intelligent life always self-destructs
We have detected intelligent life, but the government is hiding it from us
Miller-Urey experiment from 1952
Produced biotic materials from abiotic materials by putting building blocks of life in sealed vials, experiment was more successful than they originally thought
Habitable zone
Area of temperature around a star where the water on the planets is neither vaporized nor frozen, varies based on type of star and greenhouse gases on planets
Extremophiles
Some microorganisms can survive in extreme temperatures (-25 degrees C to 122 degrees C). Life can survive throughout the acid-base range and through varied salt contents
Europa
One of Jupiter’s moons, has a salty ocean beneath the crust
Titan
Largest moon of Saturn, has lakes and rivers of methane so it could have a different kind of life
Enceladus
6th largest moon of Saturn, has subsurface oceans and water vapor with minerals and organic compounds come out of plumes. Further away from Earth and gravity there is 98.8% weaker than Earth’s so it’s hard to land a probe there
Biosignatures
One of the ways to detect whether conditions on a planet are good for life or not, transmission spectrum on the atmosphere to tell the composition. We can’t detect these yet but we might be able to soon
The Drake equation
N = R* x fp x ne x fl x fi x fc x L
N = number of civilizations in the Milky Way that we might be able to communicate with
R* = rate of formation of stars in the galaxy
fp = fraction of the stars with planetary systems
ne = number of planets per system with habitable environments
fl = fraction of habitable planets on which life appears
fi = fraction of habitable planets on which intelligent life appears
fc = fraction of habitable planets on which intelligent life develops interstellar communication
L = length of time the civilizations release detectable signals into space
This equation has to be true, but we don’t know these numbers, so it’s not that helpful