Chapter 14: Measuring Galaxies - - PowerPoint PPT Presentation

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Chapter 14: Measuring Galaxies - - PowerPoint PPT Presentation

Chapter 14: Measuring Galaxies https://www.spacetelescope.org/news/heic1919/ https://apod.nasa.gov/apod/ap170510.html ASTR/PHYS 1060: The Universe Fall 2019: Chapter 14 1 Now on to Galaxies! ASTR/PHYS 1060: The Universe Fall 2019: Chapter


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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Chapter 14: Measuring Galaxies

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https://apod.nasa.gov/apod/ap170510.html https://www.spacetelescope.org/news/heic1919/

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe 2

Now on to Galaxies!

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Classifying Galaxies

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  • Groups of 2-4, one sheet per group
  • One person from each group raise your hand (so TAs can

efficiently pass out dead tree shavings)

  • First step: Once I display the 8 galaxies onscreen, begin!

What is the overall shape of the galaxy? Is it smooth or mottled? What else do you find notable about it?

  • When finished with Questions 1-4, display your ABCD

card so I know when you’re done.

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ASTR/PHYS 1060: The Universe Fall 2019: Chapter 14 4

M110 NGC 1300 M81 M87

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ASTR/PHYS 1060: The Universe Fall 2019: Chapter 14 5

NGC 4449 NGC 1232 Sombrero NGC 3628

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

How did you classify the galaxies?

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M110 NGC 1300 M81 M87 NGC 4449 NGC 1232 Sombrero NGC 3628

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ASTR/PHYS 1060: The Universe Fall 2019: Chapter 14 7

Cen A NGC 4731

Question 5: Try to incorporate these into your classification. Where would they go?

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

How did you classify the galaxies?

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M110 NGC 1300 M81 M87 NGC 4449 NGC 1232 Sombrero NGC 3628

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Hubble’s Classification Scheme: Tuning Fork Diagram

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe 10

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe 11

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Appearance depends on orientation…

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

…and the motions of stars

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Bulges and Ellipticals

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ASTR/PHYS 1060: The Universe Fall 2019: Chapter 14 14

Disk and Spiral Galaxies Which type of galaxy (Disk or Elliptical) is our galaxy, the Milky Way? Why do you think so?

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Color vs stellar age

A) Older stars have bluer colors B) Older stars have redder colors C) Stellar colors do not depend on age

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Which galaxy is oldest?

A B C

Which galaxy is prettiest?

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Why is there a connection between shape & stellar age?

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Hint: it’s analogous to planets in star systems Stars form from gas — gas settles into a disk due to angular momentum conservation!

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Spiral arms are density waves (like sound waves)

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Galaxies are not isolated

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ASTR/PHYS 1060: The Universe Fall 2019: Chapter 14 21

https://www.youtube.com/watch?v=52k-VryS1hs

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Active Galactic Nuclei (AGN) <—> Supermassive Black Holes (SMBHs)

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more or less all galaxies have an SMBH, and its mass is proportional to the mass of its bulge Cygnus A Galaxy (optical) Jets from its AGN (radio) M87 Centaurus A

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Fall 2018: Chapter 5 ASTR/PHYS 1060: The Universe

But how are galaxies moving?

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Doppler Shift of Light

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λobserved − λemitted λemitted = ∨ c

Which spectrum is moving away from us the fastest?

A B C D

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Almost all galaxies are moving away from us.

λobserved − λemitted λemitted = ∨ c

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We live in an expanding “balloon universe”

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

What are the spiral nebulae?

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Harlow Shapley Herber Curtis The great debate of 1920

MW is whole Universe

  • Sun is in outer part of the MW
  • M31 would have to be at an insane

distance to be similar

  • we can see rotation in the Pinwheel
  • this one nova in M31 would have

been impossibly bright MW is one of many galaxies

  • Sun is at the center of MW
  • M31 has too many novae to be just

a galactic nebula

  • we see dust lanes in other nebulae,

like the MW’s

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

Edwin Hubble settles the debate

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M31: Andromeda Galaxy

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Hubble’s Law

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Distance Ladder

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Parallax Spectroscopic Parallax Cepheid Variables Type Ia SNe

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A) Total Mass B) Age of stars C) Environment D) All of the above

What is the dominant factor that determines a galaxies appearance?

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What are galaxies mostly made of?

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A) Stars B) Stellar Remnants C) Gas D) Who knows?

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What are galaxies mostly made of?

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Can estimate the mass of elliptical galaxies from its hot, X-ray emitting gas

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Fall 2019: Chapter 14 ASTR/PHYS 1060: The Universe

What is dark matter?

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  • Most likely a new kind of matter

(but possibly a modification to general relativity)

  • Does not absorb or emit light
  • Interacts very weakly, except

through its gravity

  • WIMP or MACHO? Axion or

sterile neutrino?