cosmology part 1. local group picture the local group

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Cosmology Part 1

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Page 1: Cosmology Part 1. Local Group Picture The Local Group

Cosmology

Part 1

Page 2: Cosmology Part 1. Local Group Picture The Local Group

Local Group Picture

Page 3: Cosmology Part 1. Local Group Picture The Local Group

The Local Group

Page 4: Cosmology Part 1. Local Group Picture The Local Group

Virgo Cluster

Page 5: Cosmology Part 1. Local Group Picture The Local Group
Page 6: Cosmology Part 1. Local Group Picture The Local Group

Size and scale of the Universe: Reference Points

• Solar System – Sun, planets, asteroids, comets

• Galaxy – hundreds of billions of stars, gas and dust

• Clusters of galaxies – millions of galaxies

• Universe – everything!

Page 7: Cosmology Part 1. Local Group Picture The Local Group

What is the Universe?• Everything we can know about is part of the universe.• Everything we do know about is part of the universe.• Everything!

Page 8: Cosmology Part 1. Local Group Picture The Local Group

Galaxies are redshifted!

• In 1903 at Lowell Observatory in Flagstaff, Arizona, Vesto Slipher was the first to measure the redshift of a spiral nebula (now known as a galaxy).

• Slipher realized that the redshift of the spectrum of the spiral nebula (galaxy) meant that it was moving away from us at a very high speed.

Page 9: Cosmology Part 1. Local Group Picture The Local Group

Recall: The amount the lines in a spectrum are shifted indicates how fast the galaxy is moving.

Page 10: Cosmology Part 1. Local Group Picture The Local Group

ALL Galaxies have redshifts – farther from us greater redshifts!

• Many other scientists made observations similar to Slipher’s.

• In 1929, Edwin Hubble and Milton Humason put their observations together in a way that led to the first realization that the universe changes – in fact, the universe is expanding!

Addison Wesley IF20.18

Page 11: Cosmology Part 1. Local Group Picture The Local Group

ALL Galaxies have redshifts – farther from us greater redshifts!

• The units of the slope of the line in the Hubble Plot are Speed/Distance OR (Distance/Time) / Distance OR

• 1/Time SO the inverse of the slope is a unit of “Time”. What time is it? THE AGE OF THE UNIVERSE!!!!!!

Page 12: Cosmology Part 1. Local Group Picture The Local Group

• the more distant the object – the farther back in time we are seeing it– the faster it is moving away from us– and the bigger its redshift.

Page 13: Cosmology Part 1. Local Group Picture The Local Group

Does the Universe Change?

• Einstein published his theory in two steps:– special theory of relativity (1905)

…how space & time are interrelated

– general theory of relativity (1915)…relationship between gravity and space & time

Albert Einstein (1879 – 1955)

“Nature conceals her secrets because she is sublime, not because she is a trickster.”

Page 14: Cosmology Part 1. Local Group Picture The Local Group

Space and Time

Hermann Minkowski (1864 – 1909)German physicist

Henceforth space by itself, and time by itself, are doomed to fade away into mere shadows, and only a kind of union of the two will preserve an independent reality.

Page 15: Cosmology Part 1. Local Group Picture The Local Group

The Universe is four-dimensional

• A good way to think of the universe is to use Einstein’s description of space-time, the four dimensional fabric that makes up our universe.

• The universe has three spatial dimensions (length, width, height) and one

temporal (time) dimension

Page 16: Cosmology Part 1. Local Group Picture The Local Group

Space-time and Gravity• Albert Einstein stunned the scientific world in 1915…

with publication of his general theory of relativity it illustrates how space-time can be used to describe the behavior of

how mass and light interact - in a way its an explanation of how gravity works

• Isaac Newton saw gravity as a mysterious “force.” even Newton had problems accepting this concept of “action at a

distance” -- how the force of gravity is transmitted through space Einstein theorized that the “force” of gravity arises from distortions of

spacetime itself!

Page 17: Cosmology Part 1. Local Group Picture The Local Group

• Matter Warps spacetime like weights on a taut rubber sheet.• The greater the amount of mass, the greater the warping of

spacetime.

Matter Warps Spacetime

Page 18: Cosmology Part 1. Local Group Picture The Local Group

The Strength of Gravity• The greater the amount and concentration of

mass (density), the more that spacetime warps, the stronger gravity becomes.

• The distance away from the center that space-time will be curved is the same for all three objects.

• White dwarf causes steeper curvature at Sun’s former position.

• Black hole creates infinitely deep hole in the fabric of space-time but still warps out to the same distance.

• Nothing can escape from within the event horizon of the Black hole.

Page 19: Cosmology Part 1. Local Group Picture The Local Group
Page 20: Cosmology Part 1. Local Group Picture The Local Group

Matter tells space-time how to curve.

Curved space-time tells light and matter how to move.

Page 21: Cosmology Part 1. Local Group Picture The Local Group

Mass and Spacetime• Orbits can now be explained in a

new way. an object will travel on as straight a

path as possible through spacetime

Page 22: Cosmology Part 1. Local Group Picture The Local Group

Warping of Space-time and Black Holes

• Black Holes, Light and Space time.– even though it has no mass, light will be

affected by warped space-time– its path through space will be bent– within the event horizon, it cannot climb

out of the hole

• Black Holes, Matter and Space time…– the tidal forces are tremendous– the object would be “stretched and

squeezed and time would slow down”

Page 23: Cosmology Part 1. Local Group Picture The Local Group

Evidence for Space Time and General Relativity - Gravitational Lensing

• Light will always travel at a constant velocity. therefore, it will follow the straightest possible path through space-time if spacetime is curved near a massive object, so will the trajectory of light

• During a Solar eclipse in 1919, two stars near the Sun… were observed to have a smaller angular separation than is usually

measured for them at night at other times of the year

• This observation verified Einstein’s theory… making him the baddest White Guy of them ALL!!! (quoting Ed Prather, who

refers to the old astronomers, like Gallileo, dead white guys)

Page 24: Cosmology Part 1. Local Group Picture The Local Group

Gravitational Lensing• Since that time, more examples of

gravitational lensing have been seen.

• They usually involve light paths from quasars & galaxies being bent by intervening galaxies & clusters.

Einstein’s Cross

an Einstein ringgalaxy directly behind a galaxy

Page 25: Cosmology Part 1. Local Group Picture The Local Group

Spacetime for All• The reality of spacetime is the same in all reference frames.

we cannot visualize the 4D spacetime since we can’t see through time

we perceive a 3D projection (view) of spacetime while spacetime is the same for all observers, their 3D

perceptions of it (e.g. space & time) can be very different

• By analogy… we can all agree on the shape

& size of this book in 3 dimensions

• But… the following 2D projections

(views) of the same book all look very different

Page 26: Cosmology Part 1. Local Group Picture The Local Group

SO WHAT IS THE POINT!!

What is Einstein's theory of what the universe is composed of and how does it explain gravity and how the

universe is changing?

Page 27: Cosmology Part 1. Local Group Picture The Local Group

Remember the Universe, composed of a fabric of space-time, is expanding.

Page 28: Cosmology Part 1. Local Group Picture The Local Group

1 – 2 – 3 – 4 Dimensions

• A point moved in one direction creates a line (1D).• A line moved in a direction 90º to itself creates a plane (2D).• A plane moved in a direction 90º to itself creates a space (3D).• A space moved in a direction 90º to itself creates a 4D space.

Unfortunately we can not perceive this 4-D hyperspace…any space > 3D

dimension… an independent direction of possible motion

Page 29: Cosmology Part 1. Local Group Picture The Local Group

The Rules of Geometry

flat (Euclidean) geometry

spherical (curved-in) geometry

saddle-shaped (curved-out) geometry

• The geometry you know is valid when drawn on a flat surface.• The rules change if the surface is not flat.

Page 30: Cosmology Part 1. Local Group Picture The Local Group

The Universe and Spacetime• Galaxies are moving

away from us.

• Galaxies that are further away are moving faster.

• The universe is expanding!

• The expansion of the Universe creates more space and time

Page 31: Cosmology Part 1. Local Group Picture The Local Group

Tutorial: Expansion of the Universe – pg. 133

• Work with a partner.• Read the instructions and questions carefully.• Talk to each other and discuss your answers with each

another.• Come to a consensus answer you both agree on• If you get stuck or are not sure of your answer ask

another group.• If you get really stuck or don’t understand what the

Lecture Tutorial is asking for then ask for help.

Page 32: Cosmology Part 1. Local Group Picture The Local Group

As the universe expands, is the solar system expanding

with it?A. Yes, if new spacetime is forming, then there

is more space between all objects than there used to be.

B. Yes, if new spacetime is forming, then all objects are being pushed apart.

C. No, since the solar system is held together with gravity, the objects within it cannot be moved further apart.

Page 33: Cosmology Part 1. Local Group Picture The Local Group

What about the galaxies - are they expanding as well?

A. It’s the same thing as with the solar system - gravity keeps the galaxies the same size.

B. Yes, there’s more spacetime between all of the objects in the universe. So there’s more empty space between the objects in a galaxy.

Page 34: Cosmology Part 1. Local Group Picture The Local Group

The Universe is expanding

• The redshifts of galaxies is evidence that the universe is expanding.

Page 35: Cosmology Part 1. Local Group Picture The Local Group

The Universe is expanding• If the universe is expanding, it must have

been smaller in the past.• If it was smaller in the past, then there must

have been a beginning for the universe • Working backwards, what would the universe

be like at the beginning?• Hot, dense, tiny

Page 36: Cosmology Part 1. Local Group Picture The Local Group

The Big Bang marks the time when the Universe began

• In the 1940s, based on Hubble’s Law, George Gamow proposed that the universe began in a colossal explosion

• In the 1950s, the term BIG BANG was coined by an unconvinced Sir Fred Hoyle

• The BIG BANG is the event that marks the time when the universe began.

Page 37: Cosmology Part 1. Local Group Picture The Local Group

• The BIG BANG is the event that marks the time when the universe began – the beginning of the expansion.

• But what did the universe look like at the beginning?

• All of the universe as we know it now, was once a single point-like location of infinite Temperature and Energy but was NOT composed of any Matter.

Page 38: Cosmology Part 1. Local Group Picture The Local Group

10-44sec 10-35sec 10-32sec 10-10sec 300 sec 3x105yr 1x109yr 15x109yrRadiation

EraGUTEra

InflationEra

Electro-weakEra

ParticleEra

RecombinationEra

Galaxy and StarFormation

PresentEra

What happened after the Big Bang?

Page 39: Cosmology Part 1. Local Group Picture The Local Group

What evidence is there to support the idea of a Big Bang?

• ~380,000 years after the event of the Big Bang, the Universe cooled to a temperature of 3,000 K, and light, which could not propagate until then, began to spread in all directions.

• Working backwards, we should be able to see some evidence of this signature of light (blackbody radiation) at the time of the early universe.

• The light released then, almost 14 billion years ago, can still be observed now. The 3,000 Kelvin temperature of the early Universe has dropped to a temperature today of 2.735 K (Blackbody peak in the microwave) - This is known as the Cosmic Microwave Background Radiation!!!

Page 40: Cosmology Part 1. Local Group Picture The Local Group

The cosmic microwave background radiation that fills all space is evidence for

the BIG BANG

Page 41: Cosmology Part 1. Local Group Picture The Local Group

The Blackbody spectrum of the

Cosmic Microwave

Background Radiation reveals a

temperature of 2.735K

Page 42: Cosmology Part 1. Local Group Picture The Local Group

The microwave background radiation is evidence to support the ideas that:

• The Universe was once much hotter, denser and smaller.

• There were times during the early universe when light could not freely travel through space.

• The Universe began during an event we call the Big Bang.

• The Universe is approximately 14 billion years old.

Page 43: Cosmology Part 1. Local Group Picture The Local Group

COBE

WMAP

Cosmic Microwave Background Radiation

Page 44: Cosmology Part 1. Local Group Picture The Local Group

So what does the WMAP (“the best baby picture of the Universe ever taken”) tell us?

• The first generation of stars in the Universe first ignited only 200 million years after the Big Bang, much earlier than many scientists had expected.

• The new microwave background observations precisely peg the age of the Universe at 13.7 billion years old, with a remarkably small one percent margin of error.

• The Universe includes 4% atoms (ordinary matter), 23% of an unknown type of dark matter, and 73% of a mysterious dark energy.

• The new measurements even shed light on the nature of the dark energy, which acts as a sort of an anti-gravity affecting the rate of expansion of the Universe. We might not only be expanding, but the expansion might be accelerating.

Page 45: Cosmology Part 1. Local Group Picture The Local Group
Page 46: Cosmology Part 1. Local Group Picture The Local Group

The Universe – Expansion and the Big Bang

• The observation that galaxies are moving away from us, tells us that the universe is expanding

• The observation of the Cosmic Microwave Background Radiation supports the idea that the Universe stated with an event called the The BIG BANG which marks the time when the universe began its expansion from a single point-like location of infinite Temperature and Energy but was NOT composed of any Matter.

• The Universe is a Blackbody and the Cosmic Microwave Background Radiation tells us that the current average temperature of the Universe is 2.73K. Which corresponds with an age of the universe of approximately 13.7 billion years.