galaxies read your textbook: foundations of astronomy –chapter 16, 17 homework problems chapter 16...

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Galaxies • Read Your Textbook: Foundations of Astronomy Chapter 16, 17 • Homework Problems Chapter 16 – Review Questions: 1, 2, 5-7, 10 Review Problems: 1, 5, 9, 10 – Web Inquiries: • Homework Problems Chapter 17 Review Questions: 2, 4, 7, 8-10 Review Problems: 1, 5, 9, 10 – Web Inquiries:

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Page 1: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxies• Read Your Textbook: Foundations of Astronomy

– Chapter 16, 17

• Homework Problems Chapter 16– Review Questions: 1, 2, 5-7, 10– Review Problems: 1, 5, 9, 10– Web Inquiries:

• Homework Problems Chapter 17– Review Questions: 2, 4, 7, 8-10– Review Problems: 1, 5, 9, 10– Web Inquiries:

Page 2: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy Types• Ellipticals (Triaxial ellipsoids)• Lacking significant star formation

Page 3: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

E0 through E9

E0 more spherical,

E9 more elliptical (cigar)

Ellipticals

Page 4: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy Types• Spirals (Disks)• Significant star formation, gas, dust

Page 5: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

S0 through S9

S0 spiral arms not well defined

S9 spiral arms very well defined

Spiral Galaxies

Page 6: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Sa, Sb, Sc

Sa tightly wound spiral arms

Sb less so

Sc barely wrapped spiral arms

Spiral Galaxies

Page 7: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

• Barred Spirals

Barred Galaxies

Page 8: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Barred GalaxiesSBa, SBb, SBc

(Spiral Arm winding)

Page 9: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Barred Galaxies• Barred Spirals

Page 10: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy Types• Irregulars (includes those that are interacting)• Lots of star formation, gas and dust

Page 11: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Interacting• Interacting (Irregular)• Mergers

Page 12: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Hubble “Tuning Fork” Classification

Page 13: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Our view from within our own galaxy home.

Milky Way Map

Page 14: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Hydrogen 21-cm Radio Image

Page 15: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Picture (c): Home of a supermassive black hole?

The Galactic Center

Page 16: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

You Are Here

Page 17: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Disk and Halo Stars

Page 18: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

• Population II Stars (Halo objects): – Older stars

– “First or Second” generation

– Metal poor chemical composition (Anything else but H, He)

– Large space velocities relative to the sun

– High inclination orbits

• Population I Stars (Disk objects):– Younger stars (solar-type)

– “> Second” generation

– Metal rich chemical composition (Formed from enriched ISM)

– Small space velocities relative to the sun

– Low inclination orbits

Population I and II Stars

Page 19: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Population II stars:

formed first

spherically distributed

globular clusters

Population I stars:

formed later

disk distribution

open clusters

Galaxy Formation

Page 20: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy Schematic

Page 21: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Solar Galactic Orbit

Page 22: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Spiral structure

viewed as the

precession of

elliptical galactic

orbits creating

density waves.

Spiral Arm Structure

Page 23: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Spiral Density Waves

Page 24: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy RotationInvariably, it is found that the stellar rotational velocities remain

constant, or "flat", with increasing distance away from the

galactic center.

This result is highly counterintuitive since, based on

Newton's law of gravity, the rotational velocity would steadily decrease

for stars further away from the galactic center. Analogously, inner

planets within the Solar System travel more quickly about the Sun than

do the outer planets (e.g. the Earth travels around the sun at about

100,000 km/hr while Saturn, which is further out, travels at only one

third this speed). Kepler’s Third Law: P 2 ~ a3

One way to speed up the outer planets would be to

add more mass to the solar system, between the planets.

Page 25: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galactic Rotation Curve

Page 26: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy Rotation Curves

Page 27: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

• There is a LOT of non-luminous matter.

• Gravitationally, our observations show that the universe is almost 90% non-luminous matter!

• 90% of the universe is made up of stuff we can not see!

• Solar System Mass to Light Ratio ~ 1– The Sun has 99.85% of the mass and 100% of the light

• This changes to ~100 on galactic and extra-galactic scales– There is a LOT of mass inferred by gravity, but not much light

Dark Matter

Page 28: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

• What is this stuff? Normal Stuff (protons, neutrons)– very small faint objects

• brown dwarfs (large “jupiter” planets, star duds)• gas and dust

– stellar remnants • white dwarfs• neutron stars• black holes

– known or exotic yet undiscovered particles with mass• nutrinos

Dark Matter

Page 29: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy Red Shifts

Page 30: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

“Redshift”• Hubble wanted to know the distance to the faint nebulosities

• He took galaxy spectra to obtain their radial velocities.

• Armed with distance determinations to local galaxies utilizing pulsating Cepheid stars, Hubble discovered that galaxies were in general moving away from the Milky Way.

• The recessional velocity of galaxies increases with increasing distance. (Redshift-Distance relation, a.k.a. the Hubble Law)

Page 31: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Hubble’s Redshift-Distance Relation

Page 32: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Hubble Law

Vr = H0D

Vr = radial velocity (a.k.a. redshift,doppler shift)

D = Distance

H0 = Constant (a.k.a. Hubble constant)

Vr

D

Page 33: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Hubble Flow

• Galaxies A, B, and C separated by distance d• After some time (t) this distance has doubled (2d)• Distance between A,B and B,C is now 2d, and A,C is 4d• Recession velocity of B from A is v = d/t,

and B from C from A is v = 2d/t• The farther away you are, the faster you appear to recede!

Page 34: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Local Group Galaxies

Page 35: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Hubble Law

Page 36: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Galaxy Clusters

Page 37: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Hubble Constant

Vr = H0D

H0 = Hubble constant

= 60-80 km/s/Mpc

Units for 1/H0 = seconds

This is an age estimate for our universe.

The true age should be less than this

maximum age estimate because matter has

surely caused some amount of deceleration.

Page 38: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

Age Estimation

H0 = 60-80 km/s/Mpc

1/H0 ago, all matter was piled up onto each other

if there has been no acceleration or deceleration.

1/H0 ~ 10-20 Billion years (Gigayears)

Page 39: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

H = H(t)Has expansion remained constant throughout time?

Has expansion been slowing down due to the matter in the

universe gravitationally attracting?

OR

Is the universe accelerating?

Therefore, H0 = H(tnow)

The Hubble constant is not a fundamental constant,

it is variable with time.

Page 40: Galaxies Read Your Textbook: Foundations of Astronomy –Chapter 16, 17 Homework Problems Chapter 16 –Review Questions: 1, 2, 5-7, 10 –Review Problems: 1,

How Far?