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3.1 Cosmic Distance Ladder

3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

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Page 1: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

3.1 Cosmic Distance Ladder

Page 2: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

From these methods: Determine distance (see p 615 including Fig 20.16)

Page 3: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

From these methods: Determine distance (see p 626 including Fig 20.16)

Page 4: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

From these methods: Determine distance (see p 626 including Fig 20.16)

Page 5: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

Given luminosity infer distance (see p 626 including Fig 20.16)

Use surface temperature of “main sequence stars” to infer Luminosity.

Page 6: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

Use pulsation period of variable starts (“Cepheids”) to infer luminosity

Given luminosity infer distance (see p 626 including Fig 20.16)

Page 7: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

Given luminosity infer distance (see p 626 including Fig 20.16)

Use “Tully-Fisher relation” to infer galaxy luminosity from rotation speed

Page 8: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

Given luminosity infer distance (see p 626 including Fig 20.16)

Use “Tully-Fisher relation” to infer galaxy luminosity from rotation speed

Page 9: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

From these methods: Determine distance (see p 641)

Page 10: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

3.2 The Redshift

Page 11: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

Fig 20.15A redshifted galaxy spectrum

observed rest

rest

z

Redshift:

For small z v c z

Page 12: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

3.3 The Hubble law

Page 13: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

Putting together info about speed v and distance d reveals

remarkably simple behavior:

0v H d

0 65H Km/Sec/Megaparsec

1 Megaparsec = 3.3 million lightyears

Page 14: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

Special feature of the Hubble law: It looks the same from any position:

Page 15: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)

The Big Bang

Page 16: 3.1 Cosmic Distance Ladder. From these methods: Determine distance (see p 615 including Fig 20.16)