Http:// Journey Through the Expanding Universe Month, Day, Year Location Journey Through the...

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http://www.universeforum.org/ einstein/ Journey Through the Expanding Universe Month, Day, Year Location Journey Through the Expanding Universe

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Page 1: Http:// Journey Through the Expanding Universe Month, Day, Year Location Journey Through the Expanding Universe.

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Journey Through the Expanding Universe

Month, Day, Year

Location

Journey Through the Expanding Universe

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Journey Through the Expanding Universe

Roger Smith, CTIO

Home Sweet Universe, 1905

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Journey Through the Expanding Universe

GMOS-S Commissioning Team, Gemini Observatory

Home Sweet Universe, 2005

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Journey Through the Expanding Universe

NASA, the Hubble Heritage Team and A.Riess (STScI)

A Couple of Gals

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Post Cards From The Universe

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Smithsonian Astrophysical Observatory

Good Morning, Sunshine!

All light shines with a certain amount of energy.

Lower energy light includes: Radio waves Microwaves Infrared

Higher energy light includes: Ultraviolet X-rays Gamma rays

Less energy = Red

More energy = Blue

Our eyes detect only visible light

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Elementary My Dear Einstein

Hydrogen

Every element has a characteristic “fingerprint” in the form of a “spectrum”

“one line, two line, red line, blue line”

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Smithsonian Astrophysical Observatory

In a Galaxy, Far, Far, Away

A galaxy:

Billions of stars

Light from the galaxy:

Lots of hydrogen

European Southern Observatory

“one line, two line, red line, blue line”

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NASA, ESA, STScI and the HUDF Team

It’s Not Easy Being Red

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NASA/JPL-Caltech

NASA’s Spitzer Infrared Space Telescope

NASA/JPL-Caltech/M.Urry (Yale)

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Journey Through the Expanding Universe

Our Expanding Universe

S. Beckwith & the HUDF Working Group (STScI), HST, ESA, NASA

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Journey Through the Expanding Universe

Milky Way: Roger Smith, CTIO

HCG 87: The GMOS-S Commissioning Team, Gemini Observatory

Galaxies: NASA, the Hubble Heritage Team and A. Riess (STScI)

Trifid Nebula: © Jean-Charles Cuillandre (CFHT), Hawaiian Starlight, CFHT

Electromagnetic Spectrum: SAO

Spectrum Images: SAO, Virtual Spectroscope, Emilio Falco (CfA)

NGC 300: European Southern Observatory

Distant galaxies: NASA, ESA, STScI, and the HUDF Team

Spitzer: NASA/JPL-Caltech, J. Urry (Yale)

Special thanks to the Museum of Science, Boston

Historical images: Rocky Kolb (Fermilab)

Historical images: Robert Kirshner (CfA)

Historical image: Barbara J. Becker (UC-Irvine)

Historical image: Eric Shaver (U. Toronto)

Historical image: Paul Eskridge (Minnesota State)

Andromeda Galaxy: Palomar, P. Challis (CfA)

Ultra Deep Field: S. Beckwith & the HUDF Working Group (STScI), HST, ESA, NASA

Stars in Leo: © Phillippe Durville

Sun SOHO (ESA & NASA)

Orion Nebula: © ESO

ALBERT EINSTEIN and related rights ™/© of The Hebrew University of Jerusalem, used under license. Represented by the Roger Richman Agency, Inc., www.albert-einstein.net

URL or program name here

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Credits

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There’s No Place Like Home

A view of the universe, circa 1905

Composition: Stars, stars, and more stars

Arrangement: A disc with our solar system near the center

Age: Eternal

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Journey Through the Expanding Universe

Cornelius Easton

A Nebulous Question

The Milky Way Star System, 1900

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Palomar Observatory, P.Challis (CfA)

The Universe of 2005

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S. Beckwith & the HUDF Working Group (STScI), HST, ESA, NASA

How Far Are the Stars and Galaxies?

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© Philippe Durville

How Far Are the Stars?

Denebola

Zosma

Chertan

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Einstein won the Nobel Prize for his discovery of

The Photoelectric Effect

Electric = Charged particles

A Nobel Idea

Photo + Electric = Light + Atoms

The interaction of light and matter

Photo = Light

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Hubble, Hubble, Toil and Trouble

Edwin Hubble showed that the Milky Way was not the whole Universe.

He showed we live in a universe of galaxies, each equivalent to the Milky Way.

And most surprisingly of all…

Galaxies in the universe are moving away from us!

The Huntington LibrarySan Marino, California

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Smithsonian Astrophysical Observatory

Messages from Space

The Sun: Absorption (Dark Line) Spectrum

Orion Nebula:Emission (Bright Line) Spectrum

Smithsonian Astrophysical Observatory

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Pattern-ity Test

Low energy(long wavelength)

High energy(short wavelength)

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Preserving the Static Quo

Introduced to maintain a static, unchanging universe.

There was NO evidence to support it!

Einstein’s cosmological constant

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Return of the Cosmological Constant

With the discovery of Dark Energy at the end of the 20th Century, Einstein’s “biggest blunder” was back on the table.

The universe is not just expanding, it’s also accelerating!