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Announcements • Reading for next class: Chapter 20 • Cosmos Assignment 2, Due Wednesday, April 14 Angel Quiz
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Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14 Angel Quiz.

Dec 22, 2015

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Page 1: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Announcements• Reading for next class: Chapter 20• Cosmos Assignment 2,

Due Wednesday, April 14Angel Quiz

Page 2: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Questions:

• Black Holes

• Star-Gas-Star cycle

• Halo, halo stars, halo vs. bulge, halo vs disk

• Spiral arms

• Do dying stars come back as the same star?

• superbubbles

Page 3: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

QuickTime™ and aTIFF (Uncompressed) decompressor

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Halo Stars: 0.02-0.2% heavy elements (O, Fe, …) only old stars

Disk Stars: 2% heavy elements stars of all ages

Page 4: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

What do your classmates see?

To answer this need to know a little of Einstein’s theory of Motion and Gravity:

• Gravity is Motion in Warped Space - Time

• You can’t tell the difference between acceleration by gravity and any other constant acceleration

• E = mc2, energy and mass are same thing measured in different units

Page 5: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

QuickTime™ and aCinepak decompressor

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Mass warps Space - TimeWarped Space - Time tells

Mass how to Move

Forget time, think just about warped space

Page 6: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Orbits in Warped Space - Timec = circular, e = elliptical, u = unbounded

Page 7: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Elevator & Rocket

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Page 8: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Gravity = AccelerationLight Beam in an Elevator or Gravity

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Page 9: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Gravity Attracts LightLight generates Gravity

Reasonable since E = mc2

• Black Holes Gravity attracts light

• Light loses energy escaping from environs of a Black Hole. Convert radiation energy to gravitational potential energy.

• Escaping Light is redshifted to longer wavelengths and periods

Page 10: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Your classmates would see you slow down as you approached

the BH event horizon

• Can use period of light as a clock

• Redshifted light oscillates with a longer period

• Time appears to run slower near event horizon

• You would appear to stop and hover (& fade out) as you approached the Event Horizozn

Page 11: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

What would you notice as you passed the Event Horizon

Nothing special

• For you time does not slow down in a BH.

• You quickly crash into the previous matter inside the BH(But you couldn’t tell us about it)

Page 12: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

What can we know about Black Holes?• Nothing can escape from inside an Event

Horizon• Long range forces can exert influence

outside Event Horizon1. Gravity2. Electric Force

• Can determine: 1. Mass2. Charge3. Spin

Page 13: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Mini Black Holes can Evaporate

Mini BH produce strong tides (stellar BH don’t have strong enough tides)

Lose energy by work of tidal gravity on material outside the event horizon

Since energy = mass, they lose mass and get smaller

Evaporate

Page 14: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

The Milky Way,our galaxy

Beginning of Unit IV: Cosmology

Milky Way - chapter 19

Page 15: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

What does my building look like?

Page 16: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Milky Way

small portion from the

winter sky

Page 17: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

First Idea: Count stars in different directions,

more stars -> larger extent.What Assumption is made?

apteyn Model of Milky Way, 1922

Sun

Page 18: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Question 1:What Assumptions were made?

A. Stars are clustered in a disk

B. Stars are evenly distributed in space

C. Stars are clustered near the Sun

D. We see all the stars in the Milky Way

Page 19: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Question 1:What Assumptions were made?

A. Stars are clustered in a disk

B. Stars are evenly distributed in space

C. Stars are clustered near the Sun

D. We see all the stars in the Milky Way

Page 20: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

What was missing?

• We don’t see all the stars, because some are hidden by interstellar clouds of gas & dust

• The stars are not evenly distributed in space (but this is not as important)

Page 21: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

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All-Sky View

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Mosaic View, does give good idea of MW structure

Page 22: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Familiar Constellations

Page 23: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Dusty gas clouds obscure our view because they absorb visible light

This gas is the interstellar medium that makes new stars

Page 24: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Infrared light passes more easily through dusty gas clouds

This gas is the interstellar medium that makes new stars

Page 25: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Infrared Light

Page 26: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.
Page 27: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Milky Way has DISK shape

• Stars are concentrated into a disk, but some stars above and below the disk

• Neutral Hydrogen gas is concentrated in disk

Page 28: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

MilkyWay

Cartoon

Page 29: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Stars in the disk orbit in the same direction with a little bobbing up & down

Page 30: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Stars in the bulge &

halo have randomly oriented

orbits

Page 31: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.
Page 32: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Question 2:

Why do orbits of disk stars bob up and down?

A. They’re stuck to the interstellar mediumB. Gravity of disk stars pulls toward diskC. Halo stars knock them back into disk

Page 33: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Question 2:

Why do orbits of disk stars bob up and down?

A. They’re stuck to the interstellar mediumB. Gravity of disk stars pulls toward diskC. Halo stars knock them back into disk

Page 34: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Life of a Galaxy:Gas -> Star -> Gas cycle

Gas clumps together by gravity -> stars Stars produce heavy elements by fusion Stars die and return processed gas to space Enriched gas clumps together by gravity New stars

Page 35: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Life of a Galaxy:Gas -> Star -> Gas cycle

Hot, ionized gas - one million K

Warm neutral gas - 10,000 K (most is here)

Cool neutral gas - 100 K

Molecular clouds - 30 K

Molecular cores - 6 KSTAR FORMATION

Gas

Coo

ls

Page 36: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

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X-ray map of sky shows hot gas high above and far below galactic disk

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Page 37: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

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Hot gas eventually cools to form atomic hydrogen and settles into disk

X-ray map of sky shows hot gas high above and far below galactic disk

Page 38: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

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Hot gas eventually cools to form atomic hydrogen and settles into disk

Additional cooling makes the gas cold enough to form moleculesQuickTime™ and a

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Page 39: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Darkest regions of Milky Way correspond to these dense clouds.

Additional cooling makes the gas cold enough to form moleculesQuickTime™ and a

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Page 40: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Hot, Blue, Massive MS starsheat and ionize the gas around them

Page 41: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Massive, hot, blue MS stars ionize the gas around them

Produce ionization nebula

Page 42: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Recycling Stellar

Material-Low mass stars blow

off winds & eject

envelopes

Page 43: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Recycling stellar

Material -High mass

stars explode as supernova

Page 44: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Recycling Stellar Material

Stellar Winds and Supernova return stellar material, as hot gas, to the Interstellar Medium (gas between the stars) ENRICHED in Heavy Elementsproduced during nuclear fusion & supernova explosions

Page 45: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Gas -> Star -> Gas cycle

Page 46: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

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Disk: ionization nebula & blue stars = star formationHalo: no ionization nebula or blue stars = no star formation

Page 47: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

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Halo Stars: 0.02-0.2% heavy elements (O, Fe, …) only old stars

Disk Stars: 2% heavy elements stars of all ages

Page 48: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Much of star formation in disk happens in spiral arms

Whirlpool Galaxy

Where do stars form?

Page 49: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Question 3: How can we study the Center of the Milky Way?

A. By observing it in x-rays

B. By observing it in ultraviolet light

C. By observing it in visible light

D. By observing it in infrared light

E. By observing it in radio light

Choose all that apply

Page 50: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Question 3: How can we study the Center of the Milky Way?

A. By observing it in (very energetic) x-rays

B. By observing it in ultraviolet light

C. By observing it in visible light

D. By observing it in infrared light

E. By observing it in radio light

Choose all that apply

Page 51: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Center of the Milky Way

Page 52: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Question 4: Will stars move faster closer to the

center or farther away from it?

A. Closer

B. Farther

C. The same at all distances

Page 53: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

What happens

in the Solar

System?

Page 54: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Star Motions near the Center of the Milky Way

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Page 55: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

Star Motions near the Center of the Milky Way

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Page 56: Announcements Reading for next class: Chapter 20 Cosmos Assignment 2, Due Wednesday, April 14  Angel Quiz.

What did we observe?

• Stars moved fastest closest to the center• Similar Solar System• Speed decreases as 1/DPoint mass at Center of Galaxy• From velocity & distance

can determine the MassM (inside distance D) = V2 D / G

Supermassive Black Hole, M ~3-4x106 Msun