modern telescopes and ancient skies new views of the universe an iu lifelong learning class...

54
Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Upload: susan-leonard

Post on 23-Dec-2015

219 views

Category:

Documents


0 download

TRANSCRIPT

Page 1: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Modern Telescopes and Ancient

SkiesNew Views of the Universe

An IU Lifelong Learning ClassTuesdays, May 10, 17, 24

Page 2: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24
Page 3: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Size and Scale Surveying

the Universefrom the Earth to the farthest reaches of the visible Universe

Page 4: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Galileo Galilei's "The Phases of the Moon"Image courtesy of Biblioteca Nazionale Florence, Italy

Our closest neighbor

Page 5: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Visualizing the Earth from Space

• What do you see?– Earth

– Moon

– Sun

– Stars

Copyright 1980 by DC Comics Inc.

Page 7: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

EarthRadius: 6400 kmDistance from Sun: 150,000,000 km

1 AU, 8 light minutes

Moon

Radius: ¼ Earth’s radiusDistance from Earth:

384,000 km

Page 8: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Solar System

Sizes of planets NOT to scale

Distance to Pluto: about 40 AU(about 320 light minutes)

Page 9: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The Nearest

Stars

The closest star to our Sun is Proxima Centauri, about 4 light years distant.

Page 10: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Most of the stars we see in the sky are within

250 light years

Page 11: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Our Sector of the Galaxy

The Sun lies along one of our Galaxy’s spiral arms, known as the Orion Arm

Page 12: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

View of theMilky Way Galaxy

Our Milky Way galaxy contains two hundred billion stars.

The Sun is about 26,000

light years from the center.

Page 13: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Our Milky Way Galaxy is part of a small cluster of galaxies.

Page 14: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Virgo Supercluster

Our Local Group of galaxies is part of a larger supercluster of galaxy groups.

Page 15: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Galaxies and clusters of galaxies collect into vast streams, sheets and walls of galaxies.

Page 16: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The Visible Universe

On the largest scales, the universe seems to be more or less uniform

Page 17: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

With thanks to Bill Watterson, 1990

Page 18: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

What will we cover?????

How telescopes work

Modern telescopes

Sky viewing

Space telescopesSpace telescopes

Kirkwood Obs

Visiting the Gemini Observatory

Future telescopes

Page 19: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Beginnings…

This sketch of a telescope was included in a letter

written by Giovanpattista della Porta in August 1609

Page 20: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Thomas Harriet’s Drawings of the

Moon and Sun

Page 22: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Technology moves forward…

Page 23: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The 3.5-meter WIYN telescope Kitt Peak, Arizona

Page 24: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

New Telescope Technology

“Fast” mirror Lightweight mirror

Mirror shape controlled Mechanically simpler

mount Temperature control

Page 25: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Casting the WIYN Mirror

Page 26: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Polishing the WIYN Mirror

Page 27: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The WIYN New Technology “Dome”

Compact telescope chamber Open for ventilation Insulated to keep cool Heated spaces kept separate

Page 28: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Breaking the “cost curve”

New technology provides better performance at lower cost

WIYN

Page 29: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

in 6-8 meter telescopes

WIYN TECHNOLOGY

Page 30: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

text

The importance of image quality

typical ground-based image

Hubble image

WIYN image

The Ring Nebula

Page 31: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Connecting the First Nanoseconds to the Origin of Life

Page 32: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

How is the Universe put together? The Wilkinson Microwave Anisotropy

Probe tells us about the state of the Universe 400,000 years after the Big Bang.

How did the UniverseHow did the Universeevolve from this…evolve from this…

Page 33: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

…to this?

Page 34: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The cosmic web of intergalactic gas and galaxies in a young universe

Intergalacticgas

Clumpsconcentratedby darkmatter lead to galaxies

Observing the assembly of galaxies

Galaxy building blocks

observed withHubble

Simulation

Page 35: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

WMAP also providesevidence of the first stars

Tiny fluctuations in polarization

About 200 million years after the Big Bang

Page 36: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

We can almost see the first stars

Simulation

What we might see with a 30-meter telescope(Barton et al., 2004)

4 million LY

hydrogen emission from hot stars

Green=hot gas yellow=stars

Page 37: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The composition of stars and gas:

everythingelse

90% hydrogen atoms

10% helium atoms

Less than 1% everything else

What is the Universe made of?

Page 38: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

But ordinary matter is only part of the story…

96% of the Universe is something else

Page 39: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Galaxy interactions require more mass than we can see

Antennae Galaxy (HST)

Computersimulation

The real thing

Page 40: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Dark Matter The universe contains additional matter

we cannot see Dark matter interacts with normal

matter through gravity Dark matter does NOT interact with light

the way the normal matter does The Universe contains 5 or 6 times

MORE dark matter than normal matterAll galaxies are embedded in clouds of

dark matter We do not know what it is!

Page 41: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

“Redshift” of Galaxies

The spectra of galaxies are shifted to the red: galaxies are moving away from us.

The farther away a galaxy is, the faster it recedes from us!

Page 42: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Hubble’s Law

Distance - Velocity Relation

0

1000

2000

3000

0 20000 40000

Velocity (km/sec)

Dis

tan

ce (

LY

)

Page 43: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The speeds of very distant galaxies tell us the Universe

is expanding faster today than in the past

The brightness of stellar explosions tells

us how far away galaxies are

Page 44: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

The universe is expanding faster today than it did in early times

This expansion cannot be caused by ordinary or dark matter, which slows expansion.

The acceleration suggests a new repulsive force (anti-gravity) acting on very large scales

The Universe is speeding up!

Page 45: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Dark energy accounts for 73% of the content of the universe

Dark matter accounts for 23%The content we’re familiar with is only 4%

The New Force Is Called “Dark Energy”

Page 46: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

We don’t know

What is Dark Energy?

Identifying what dark energy is requires bigger

telescopes and new techniques

Page 47: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Connecting the First Nanoseconds to the Origin of Life

Page 48: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Kirkwood Observatory ViewingTuesday evenings, weather permitting

Page 49: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Night Sky Viewing

• Scheduled nights–Tuesday, May 17

–Tuesday, May 24

• Roof of Swain West

Page 50: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Next Week• Telescopes in Space,

including the Hubble Space Telescope

• New Views of the Universe – Planets around other Suns

• Kirkwood Obs and Rooftop, weather permitting

Page 51: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Is there life elsewhere?

Artist’s conception of 55 Cancri’s planetary system

More than 150 planets found around other stars

Most are vastly different fromour Solar System

Page 52: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

detecting planets directly is hardplanets are small and dimplanets are near much brighter stars

detecting planets directly requires large telescopes (30-meters) and/or special instruments

Detecting Planets

Page 53: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

Imaging planets around other stars

“Brown Dwarf” orbiting a star

at the same distance as

Saturn from our Sun

Gemini/Keck AO detectionby Michael Liu (IfA), 2002

Page 54: Modern Telescopes and Ancient Skies New Views of the Universe An IU Lifelong Learning Class Tuesdays, May 10, 17, 24

With a 30-metertelescope we canobtain the spectraof planets aroundother stars to searchfor the signatures of life

Simulation by Sudarskyet al. 2003

Simulation of the spectra of 55 Cancri’s planets