Chapter 20 Galaxies Determining Distance

17
Chapter 20 Galaxies Determining Distance

description

Chapter 20 Galaxies Determining Distance. Measuring distances to galaxies:. We measure galaxy distances using a chain of interdependent techniques. Step 1 Determine size of solar system using radar – because light travels at a constant speed in space. Step 2 - PowerPoint PPT Presentation

Transcript of Chapter 20 Galaxies Determining Distance

Page 1: Chapter 20 Galaxies  Determining Distance

Chapter 20Galaxies

Determining Distance

Page 2: Chapter 20 Galaxies  Determining Distance

Measuring distances to galaxies:

We measure galaxy distances using a chain of interdependent techniques

Page 3: Chapter 20 Galaxies  Determining Distance

Light travels at a constant speed in space of 3x108 m/s).

We send a signal to a planet and measure the time for the reflected signal.

Distance = speed x time

Step 1: Radar

Page 4: Chapter 20 Galaxies  Determining Distance

Determine the parallax angle.

Distance = 1/p

Use parallax to determine distance of nearby stars out to a few hundred light-years

Step 2: Parallax

Page 5: Chapter 20 Galaxies  Determining Distance

Find the distance to a nearby star cluster with parallax. Use the distance and apparent magnitude to find the luminosity of each type of star it. Plot these stars on an HR diagram. Use the diagram as a reference diagram.

Step 3: Main Sequence Fitting

Page 6: Chapter 20 Galaxies  Determining Distance

Step 3 – con’t

Calculate distance of more distant clusters by comparing their brightness to nearby clusters and use the distance- luminosity formula.

Page 7: Chapter 20 Galaxies  Determining Distance

The remaining steps use standard candles. A standard candle is an object whose luminosity we can determine without measuring its distance.

Image Credit: NASA

Visible UV X-Ray

Supernova 2005ke

Page 8: Chapter 20 Galaxies  Determining Distance

Cepheid variables are very luminous stars that have a period-luminosity relationship. We can use these stars as standard candles.Cepheid variable stars with longer periods have greater luminosities

Step 4: Cepheid Variables

Page 9: Chapter 20 Galaxies  Determining Distance

All WD have the same maximum mass limit of 1.4 Ms, therefore they all have the same luminosity.

Their apparent brightness tells us distance to galaxies up to 10 billion light-years

Step 5: Type 1a Supernovae

Page 10: Chapter 20 Galaxies  Determining Distance

Step 6 Tully-Fisher Relation

Use entire galaxies as standard candles because luminosity is related to rotation speed(both depend on mass)

Page 11: Chapter 20 Galaxies  Determining Distance

Lastly, use redshift.Hubble measured the distance to the Andromeda Galaxy using Cepheid variables as standard candles

Edwin Hubble

Hubble’s Law

Page 12: Chapter 20 Galaxies  Determining Distance

He measured redshift & distance to other galaxies

Page 13: Chapter 20 Galaxies  Determining Distance

Hubble’s Law: velocity = H0 x distance

Hubble found that redshift and distance are related in a special way

Page 14: Chapter 20 Galaxies  Determining Distance

More distant galaxies have greater redshift.

Page 15: Chapter 20 Galaxies  Determining Distance

Hubble’s constant tells us age of universe because it relates velocities and distances of all galaxies

Age =

~ 1 / H0

Distance

Velocity

Page 16: Chapter 20 Galaxies  Determining Distance

But distances between faraway galaxies change while light travels

Astronomers think in terms of lookback time rather than distance

distance?

Page 17: Chapter 20 Galaxies  Determining Distance

Expansion of the Universe