Hubble images a part of the Universe - PowerPoint PPT Presentation

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Hubble images a part of the Universe

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One method parallax is only good for the very nearest stars ... For some stars, it has taken the light billions of years to reach Earth ... – PowerPoint PPT presentation

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Title: Hubble images a part of the Universe


1
Hubble images a part of the Universe
2
In the beginning
  • How did this all start?
  • When did it start?
  • Has it always been this way?
  • How is it changing?
  • What does it all mean?

3
A Quest for Answers
  • Observations of planets, stars, galaxies
  • Analysis of light from stars and galaxies
  • Thinking about these observations
  • Posing an hypothesis
  • Testing the hypothesis
  • Evidence/tests either support or refute
    hypothesis
  • Lets start with the observational evidence

4
The Electromagnetic Spectrum
  • Visible Light Range

5
The Electromagnetic Spectrum
6
Chemistry from Spectra
  • Emission Spectra

7
Chemistry from Spectra
  • Absorption Spectra

8
Analyzing Stellar Spectra
  • Chemistry of Stars
  • Predominantly Hydrogen (H)
  • Second most common Helium (He)
  • Other elements in minor quantities

9
Analyzing Stellar Spectra
  • Anomalies in positions of absorption bands
  • Normal Spectrum

10
Analyzing Stellar Spectra
  • Anomalies in positions of absorption bands
  • Shifted Spectrum

11
Comparison of Normal and Shifted Spectra
  • Normal Spectrum
  • Shifted Spectrum

12
What could cause shifted spectra?
13
Animation
  • http//lectureonline.cl.msu.edu/mmp/applist/doppl
    er/d.htm

14
Doppler Effect
  • Waves emitted from a moving source are shifted
    depending on direction of motion.
  • Sources moving toward observer show shift toward
    shorter wavelengths (i.e., toward blue end of
    spectrum)
  • Wavelength is compressed by motion of source.
  • Referred to as BLUE SHIFT

15
Doppler Effect
  • Waves emitted from a moving source are shifted
    depending on direction of motion.
  • Sources moving AWAY from observer show shift
    toward longer wavelengths (i.e., toward red end
    of spectrum)
  • Wavelength is stretched by motion of source.
  • Referred to as RED SHIFT

16
Hubbles Law
  • Nearly all galaxies in the Universe display RED
    SHIFT
  • The amount of RED SHIFT is related to the
    relative distance to the galaxy.
  • FARTHER galaxies show GREATER RED SHIFT

17
Example of Red Shift
  • Normal Spectrum
  • Shifted Spectrum

18
Hubbles Law What does it mean?
  • Is the Earth the center of the Universe after all
    and everything is moving away from us?
  • Does it depend on frame of reference?
  • Would Hubbles Law apply if we looked at the
    Universe from another location?
  • Why is everything moving away?

19
Hubbles Observation/Hubbles Insight
  • All galaxies appear to be moving away from the
    center of the Universe because the Universe is
    expanding.
  • The existence of RED SHIFT and the pattern that
    it shows (greater shift for farther galaxies) is
    consistent with a pattern produced by an
    explosion
  • THE BIG BANG!!

20
The Big Bang
  • Currently the best theory to explain the origin
    of the Universe
  • Supported by multiple lines of evidence

21
What was the Big Bang?
  • Prior to the Big Bang there was no Universe
  • A single super-massive object exploded
  • Explosion creates Universe
  • Matter, space and time are created
  • Explosion was approximately 15 billion years ago

22
  • The Big Bang 10-35 seconds
  • generates space time, as well as all the matter
    energy universe will ever hold
  • For small fraction of a sec., the universe is an
    infinitely dense, hot fireball

23
  • The Universe Takes Shape -- 10-6 sec.
  • universe continues to expand ? less dense
    cooler.
  • now basic forces in nature become distinct
  • Gravity strong force (holds nuclei of atoms
    together), followed by the weak electromagnetic
    forces.
  • By end of 1st second, universe consists of
    particles energy -- smash together ? form
    protons neutrons.

24
  • Formation of Basic Elements -- 3 sec.
  • nuclei of simple elements hydrogen, helium and
    lithium form
  • (will be another 300,000 yrs before electrons are
    captured into orbits around these nuclei to form
    stable atoms).

25
  • The Radiation Era -- 10,000 years
  • most of the energy left from the fireball is in
    the form of radiation --
  • different wavelengths of light, X rays, radio
    waves ultraviolet rays

26
  • Birth of Stars Galaxies -- 300 my after BB
  • (still 12 to 15 by before the present).
  • pockets of gas become more and more dense as a
    result of gravitational attraction.
  • Stars ignite within these pockets
  • groups of stars become the earliest galaxies.

27
  • Birth of the Sun -- 5 Billion Years Before
    Present (BP)
  • Sun forms w/in cloud of gas in spiral arm of
    Milky Way Galaxy.
  • vast disk of gas debris swirls around new star
    ? gives birth to planets, moons, asteroids .

28
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29
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30
Evidence in support ofBig Bang Theory
  • Hubbles Law and pattern of red shift
  • Cosmic Background Radiation
  • Mathematical models
  • Particle physics theory

31
New Insights into the Big Bang
  • Recent mapping of microwave and temperature
    variations suggest that the Universe may be flat
    not spherical!
  • Implications?

32
What about life elsewhere in the Universe and How
Big is the Universe?
33
Spiral Galaxy
34
Stars and Planets
  • Each galaxy has about 100 billion stars
  • There are billions of galaxies!
  • Even if only 1 of stars had planets,
  • And even if only 1 of those planets were like
    Earth,
  • There would still be hundreds of millions of
    planets that could have life on them!

35
How far are the stars? How big is the Universe?
  • We can measure distances to stars by two methods
  • One method parallax is only good for the very
    nearest stars
  • The other method comparison of magnitudes is
    more complex, but it can be used for even the
    farthest stars and galaxies.

36
Parallax
  • Classroom demonstration of parallax
  • Knowing one distance and one angle, we can
    calculate distance to star using trigonometry

37
Apparent vs. Actual Stellar Magnitude (brightness)
  • Compare how bright the star looks to how bright
    it would look at a known distance
  • You must first know actual magnitude (brightness)

38
How do we know actual magnitude?
  • Cepheid variable stars absolute magnitude is
    directly related to period of pulsation
  • Supernova fixed magnitude
  • Spectral analysis gives composition, which is
    related to size, which is related to brightness

39
How close is our nearest neighbor?
  • Proxima centauri is 4.27 light years from Earth

40
What is a light year?
  • The distance that light will travel in one year.
  • Since light travels at 186,000 miles per second,
  • A light year is approximately 6 trillion miles

41
Implications?
  • Distances are enormous!!
  • For some stars, it has taken the light billions
    of years to reach Earth
  • In some cases, this means that the star isnt
    even there anymore!
  • We see the light that left long ago, therefore

42
Looking at the night sky is literally looking
into the past!!
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