Term
When a Type II Supernova explodes the Stellar core is left over depending on its mass it will either be a _______ or __________.
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Neutron Star or Black Hole |
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In a Type II Supernova the High Mass core collapsed and forced the electrons into the atomic nucleus (iron core) |
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If the core left behind has a mass between 1.4 and 3 Mo
it becomes a ________.
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Definition
big ball of neutrons with a mass of 1.4-3 Mo
radius: 10-15km (20 mile diameter) *About as big as Mobile is Wide
density extremely high
Sugar cube size of this stuff would weigh 200 billion lbs on Earth |
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Neutron Stars rotate rapidly, up to 30 times a second
Conservation of angular momentum. It must rotate rapidly due to its smaller size.
*Ice skater example - Ice skaters spin faster and faster as they bring their arms in - the smaller the angular momentum the faster they spin. |
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Neutron Stars have large magnetic fields.
The neutron star has the magnetic field of the original star - its smaller size concentrates the field, making the magnetic field trillions times larger.
Also - very very hot: 1 million K at surface, emits lots of X-Rays, heat due to contraction, low luminosity due to size. |
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Which of the following is not a fundamental property of a black hole? |
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The imaginary surface around a black hole where the escape velocity is the speed of light is called: |
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Definition
two of the following choicse are true
(has a large magnetic field)
(rotates rapidly) |
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The clock-like regularity of radio pulses from pulsars is the result of |
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The main reason for the observed slowdown of many pulsars is |
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Definition
loss of rotational energy by emission of radiation |
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In 1054 A.D., Chinese Astronomers observed the appearance of a "guest star" whose location is now occupied by |
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Definition
a supernova remnant called the Crab Nebula |
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The Schwartzchild radius of a black hole is |
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Definition
the distance from the singularity to the event horizon |
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Definition
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Lighthouse theory:
- spinning magnetic field acts like a generator, creates and electric field
- electric field rips charged particles off surface of neutron star
- particles accelerate outward along poles of magnet, emitting radiation
- looks like it flashes when beam of light passes your line of sight.
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Term
Not all neutron stars are pulsars
but
All pulsars are neutron stars
approx 500 known pulsars |
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Definition
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Pulsar Glitches!
Pulsars are slowing down
- period of rotation increases by a few billionths af a second each day
- Pulsar is losing energy
- Energy radiated outward is about equal to the energy lost by slowing rotation
- Estimate age of pulsar by how fast it rotates.
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Definition
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X-Ray Bursters
- Neutron star in a binary system
- Matter from companion falls onto neutron star
- forms an accretion disk
- slowly spirals to the surface
- as matter builds up on surface it gets hot, and very dense
- Hydrogen fusion begins over the entire surface
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X-Ray Bursters cont...
like a nova except:
with a Nova you have a white dwarf (H falling on white dwarf)
HERE you have X-Ray Burster: neutron star and H falling on it. |
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Gamma Ray Burster
Flash of Gamma Rays lasting only a few seconds.
Possibly from merging neutron stars |
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Black Hole
If the core of the supernova star has a mass greater than 3Mo, no known force can stop its collapse.
3Mo the "Chandraskhar Limit" for neutron stars.
- core collapes to zero radius
- density is infinite / gravity at its surface is infinite - Not even light can escape |
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Definition
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Black Hole escape velocity
do not need to know formula - but do know:
- R (size of object) = size of thing you are going to try to escape
- *as R gets bigger the Ve (escape velocity) will get smaller
- If R gets smaller than Ve gets bigger
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Term
Eventually R could be so small that Ve would exceed the speed of light.
**But nothing can travel faster than the speed of light - which means you cannot get away from the Black Hole |
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If Ve exceeds C (speed of light) you can't escape. It is a Black Hole.
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Distance from black hole where Ve = C |
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Definition
The imaginary sphere around a black hole where radius = Schwarzchild radius
**If you cross the event horizon, you cannot escape - nothing can escape
**Any event inside the event horizon can never be communicated to the universe.
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Finding a Black Hole
Black holes are in a binary system
black holes strip mass off its companion
forms an accretion disk
as mass falls into the hole, it is heated and emits x-rays.
bipolar jets formed by companions mass
*a black hole ingesting mass can release a huge amount of radiation due to mass being heated as it falls |
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Three Characteristics of Black Holes |
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Definition
- mass
- charge
- angular momentum
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A Swarzchild Black Hole has NO angular momentum
A Kerr Black Hole has angualr momentum
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Term
William and Caroline Herschel (brother and sister)
studied: |
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Definition
shape of Milky Way using star counts
*They thought the Milky Way was shaped like an alligator head. |
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Milky Way
can be confused with a cloud
Galileo discovered the Milky Way was stars |
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Definition
noted globular clusters mostly on one side of the sky
measured their distance using RR Lyrae Varibles
generated a 3D map (locations of clusters)
- He believed that the center of distribution must be the center of the galaxy (because of the effects of gravity).
- Shapely estomated the size of the galaxy at 100,000 parsecs with us at one edge.
- He believed that the galaxy was the entire universe, there was nothing else. |
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Milky Way
Earth is about 25,000 ly from the center of the galaxy
*we are indeed off to one side like Shapely thought
Overall shape similar to a fried egg earth is off in the white of the egg |
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Definition
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Milky Way components
Disk Component
- stars
- open clusters
- almost all gas and dust
Nuclear Bulge (galactic bulge)
- crowded with stars
- cool low main sequence stars (K & M stars) |
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Milky Way Componenet cont..
Halo
- thin scattering of stars, same type as in nucleus
- globular clusters
- no gas and dust |
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Definition
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Milky Way rotates
-stars would fall into center of galaxy without rotation
-stars are orbiting the inner galaxy
Sun moves at 220 km/s toward Hercules
-orbit radius = 8500 pc
-orbit period = 240 million yrs (20 orbits since we were first formed)
Use Keplers 3 law to estimate mass of galaxy
-2 X 1011 Mo |
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Definition
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Term
Extra mass apparently Dark Mass - we don't see it
Theories for dark matter:
- black hole (unlikely)
- brown dwarfs (possible)
- low mass white dwarfs (possible)
- exotic matter (?) |
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Term
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Definition
General Theory of relativity that says the path of light can be changed by gravity - Thus "gravitational lensing".
*Dim white dwarfs may have been detected using gravitational lensing |
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Term
Stars in galaxy can be divided into two general classes or Stellar Populations
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Definition
Polulation I and Population II |
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Term
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Definition
- located in galactic disk
- metal rich (203% atoms heavier then He)
- relatively young
- circular orbits in plane of galactic disk
*Sun is population I
Metal content defines whether Pop i or Pop II
Population I stars get metal from previous generations of stars |
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Term
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Definition
- located in Halo and nuclear bulge
- metallic poor
- old stars
- elliptical orbits, randomly tilted
*Globular cluster stars are Population II stars.
Population II stars are older & were formed before metal were created.
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Term
Spiral Arms
- Milky way apparently has a spiral patterned shape
- Many other galaxies also
- Spiral arms are regions of high gas density and young hot stars
- Spiral arms defines by presence of gas, dust, and O & B stars.
- lots of emission and dark nebula in the spiral arm |
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Definition
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Milky way spiral arms found by
- plot position of O and B stars
- plot density of neutral hydrogen
-21 cm radiation (photon)
-transparent dust particles
*The Sun is in Orian Arm of spiral |
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Definition
-spiral arms are stable regions of compression
-coiled wave of high density
-squeezes gas, triggers star formation
*like cars in a traffic jam |
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Center of the Milky Way is in Sagitarius
50,000 stars per cubic parsec
powerful radio source, Sag A
rapidly moving gases
cosmic rays
Gamma Rays emitting from galaxy center
E of gamma rays = mass of electron
gamma rays created by pair annihilation
- electrons and anti-electrons meeting, emit 2 gamma rays |
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Definition
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Term
Giant Black Hole in galactic core
Sag A is radio emission from the suspected black hole at the galaxy center. |
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Definition
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Measuring Galaxies:
- several methods for measuring distance, depending on the distance
*Cepheid Variables
- period proportional to avg luminosity
- must resolve individual stars
- ***The best method***
- Hubble gets us to 25 Mpc
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Definition
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Term
Tully Fisher Relation
- Rotation Speed of galaxy is proportional to its luminosity
*bigger galaxies rotate faster
*big galaxies are brighter (more stars)
-Rotation speed from Doppler Shift
- Measure apparent magnitude
- calculate distance
- good to 200 Mpc
***Only true for Spiral galaxies - not elliptical |
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Definition
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Term
Supernovae (Type I)
-Assume Supernovae reach same absolute magnitude
- measure apparent magnitude
- good to about 1000 Mpc
-18.9 or 19. |
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Definition
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Velocity
Radial Velocity
- speed directly towards or away from us
- measure using Doppler Shift
- blue shift - moving towards us
- red shift - moving away from us
**only a few display blue shift |
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Definition
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Velocity cont..
Transverse Velocity
- recall this is speed across our line of sight
- must measure distance
- must measure proper motion
**Cannot be done (galaxies too far away) |
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Definition
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Edwin Hubble and Melton Humason
- measured radial speeds of many galaxies and their distance
- made a graph of distance on X axis and radial speed on Y axis.
Hubbles Law = more distant the galaxy, the greater the recessional speed. |
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Definition
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Hubbles Law comes from the diagram
recessional velocity = H x distance
- H is Hubbles Constant
- H corresponds to the slope of line in diagram
- we now know Hubbles constant within 5%
*Hubbles law is now the way to measure galactic distance
V=HxD D=V/H answer in Mpc |
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Definition
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Galaxy Types
Edwin Hubble noted 3 types of galaxies
the normal ones - do not put out alot of energy
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Definition
- Spiral
- Elliptical
- irregular
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Term
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Definition
- Medium to large
- Central bulge, flattened disk, spiral arms, gas, dust, & young stars
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Spiral Classes
SO
-very large core
-disk has no apparent spiral
- very little gas and dust
SA
- large core
- tightly wound arms
- little gas and dust |
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Definition
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Term
SB
- medium core
- medium wound spiral arms
- medium gas and dust
SC
- Small Core
- loosely wound arms
-lots of gas and dust - dust indicates that these are relatively young |
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Definition
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Term
Barred Spiral Galaxies
- Elongated structure, flattened disk, spiral arm, gas, dust, young stars
- These galaxies have a strabge bar extending from their core.
Class same as for spirals w/added letter B
SBo, SBa, SBc.. |
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Definition
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Elliptical Galaxies
- Round, no disk, very little gas, very little dust, old stars
- These have an elliptical shape
- Classed E0, E1...E7
- O Spherical Shape
- 7 Cigar Shape
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Definition
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Irrengular galaxies
Asymetric often with gas, dust, young stars
- No obvious pattern
- generally pretty small
- generally lots of gas and dust
Milky way has two gravitationall bound to it:
Large Magellanic Cloud and Small Magellanic Cloud |
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Definition
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Term
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Definition
Collection of galaxies held together by their mutual gravitation attraction.
- the Milky Way is in the local group. - about 50 galaxies within 1 Mpc.
- only 3 spirals, the rest are dwarf irregulars and dwarf ellipticals
*The Virgo cluster is about 17 Mpc from the Milky Way and has 2500 galaxies in volume 3 Mpc across |
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Irregular Galaxies
-Because galaxies occur in close clusters they often interact gravitationally.
- Cause of many Irregular Galaxies.
Many astronomers believe that the SMC used to be a barge spiral but gravitational forces within the Milky Way ruined the galaxies shape.
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Term
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Definition
giant galaxies absorbing smaller galaxies |
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Term
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Definition
- unusually bright tiny core
- 1000s times brighter than the Milky Way Core
- most energy in IR region and radio region which is indication that it is a Non-Stellar region (stars do not emit IR or radio)
-Spiral Galaxy
- Spectrum contains very broad emission lines, indicates gases rapidly rotating around a central object
*brightness varies over period of months, indicates source is light months across |
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Term
Quasar
aka Quasi Stellar Object
QSOs |
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Definition
-star like appearance
-show a large red shift
-wavelength 5 times longer than normal indiicates large distance (billion parsecs or more)
**Quasars are the central core of a very distant galaxy
quasars sometimes appear to be double or quadrouple - due to gravitational lensing
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Quasars are the core of very young galaxies
- every galaxy could have been a quasar |
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Definition
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Every galaxy could have been a Quasar:
-when young, many stars evolve into black holes
-black holes sink to the middle of the galaxy and merge
-lots of mass falls into the black hole, lots of radiation emitted
As galaxy ages, less mass available to fall into a central black hole
Galaxy becomes a Seyfert Galaxy or BL Loc galaxy (like Seyfert but elliptical) - bright tiny core is mass falling into black hole at reduced rate.
when galaxy matures, very little mass left to fall into central black hole
now a "normal" galaxy like the Milky Way |
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Term
The Big Bang
Three Basic Observations in Cosmology |
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Definition
- Homogeneity
- Isotropy
- Universality
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Term
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Definition
Matter is uniformly spread throughout the universe |
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The Universe looks the same in all directions |
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Term
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Definition
Laws of physics do not change with time or position |
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Homogeneity, Isotropy, and Universality are embodied in the Cosmoligical Principle
-any observer in the universe sees the same general features, no matter what his location or in what direction he looks.
-the Universe can have neither edge not center
Isotropy and Homogeneity would be violated otherwise |
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Definition
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Sloan Digital Survey
survey if 67,000 galaxies to a distance of a billion parsecs. -Galactic clusters, filaments, and voids can be seen but on a scale larger than 300Mpc the distance is constant
*all galaxies are moving away from us |
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Definition
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George LaMaitre, a Belgiam Priest and physics professor is credited with discovering the Big Bang Theory
"Some creation event started the universes expansion"
He derived Hubles Law 2 years before Hubble discovered it
*Consider Hubbles Law: V-HD: to everyones surprise, measurements indicated that the expansion of the universe is accelerating. |
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Definition
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The accelerating Universe
- There must be some energy source that is causing the expansion to accelerate.
-Most stuff in the universe is dark energy
-matter as we know it is rare
-Universe is 5% "normal matter"
-25% dark matter
-70% dark energy
**we do not understand the Nature of 95% of the Universe. |
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Definition
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Term
Big Bang Timeline
Time t = 0 to t = .0001 second
-universe is filled with high energy gamma rays
- radiation dominated
Time t = .0001 second to 3 minutes
- gamma rays have insufficient energy to form baryon anti-baryon pairs
**All matter in the universe formed in the first 3 minutes
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Definition
Time t = 3 minutes to 30 minutes
-Age of Nucleosynthesis
- He forms, trace of Li, nothing else
- Universe is virtually all H and He
Time t = 30 min to 50,000 yrs Time t = 50,000-100 Million yr
-Nucleosynthesis ceases -age of recombination
-75% H and 25% He -Universe cool enough to allow
-Universe is opague e's to combine with nuclei to form neutral atom.
*Universe now transparent. It is impossible to see any photons, to see anything before this era! Universe begins the "matter era"
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Term
Cosmic Microwave Background
Story of Arno Penzios & Robert Wilson
- Built a "horn" antennea to be ultra quiet -picked up interference everywhere in equal directions
- freq of noise correspondes to black body w/temp 2.7K
-They detected photons from the Big Bang
-photons traveling the universe for 14 billion years |
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Definition
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Term
Three pieces of evidence for the Big Bang Theory
- Virtually all galaxies getting farther away from us
- the universe is expanding
- Cosmic Microwave Background
-from photons present when universe became transparent
- Detailed Structure of the Cosmic Microwave Background.
*Big Bang Theory predicts size of temp blackbodys which match observations
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Definition
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