15.2 Distances of Galaxies - PowerPoint PPT Presentation

About This Presentation
Title:

15.2 Distances of Galaxies

Description:

Determine distances of stars out to a few hundred light-years using parallax ... radar ranging in our own solar system and parallax measurements of distances ... – PowerPoint PPT presentation

Number of Views:41
Avg rating:3.0/5.0
Slides: 37
Provided by: YOR46
Category:

less

Transcript and Presenter's Notes

Title: 15.2 Distances of Galaxies


1
15.2 Distances of Galaxies
  • Our Goals for Learning

How do we measure the distances to galaxies?
What is Hubbles Law? How do distance
measurements tell us the age of the universe?
2
How do we measure the distances to galaxies?
3
Step 1 Determine size of solar system using radar
4
Step 2 Determine distances of stars out to a few
hundred light-years using parallax
5
Brightness alone does not provide enough
information to measure distance
6
The relationship between apparent brightness
and luminosity depends on distance
Luminosity Brightness
4 pi x
(distance)2 We can determine a stars distance
if we know its luminosity and can measure its
apparent brightness
Luminosity Distance
4 pi x Brightness A standard
candle is an object whose luminosity we can
determine without measuring its distance. We can
use standard candles to measure distances.
7
Step 3 Apparent brightness of star clusters
main sequence tells us its distance
8
Which kind of stars are best for measuring large
distances?
  • High-luminosity stars
  • Medium-luminosity stars
  • Low-luminosity stars

9

Cepheid variable stars are very luminous
10
Cepheid variable stars with longer periods have
greater luminosities
11
Step 4 The period of a Cepheid variable star
tells us its luminosity. Its luminosity plus
its apparent brightness tells us its distance.
So we can use Cepheid variable stars as
standard candles to measure distances.
12
Edwin Hubble, using Cepheids as standard candles,
was the first to measure distances to other
galaxies
13
Measuring distances using Cepheids has been a key
mission of the Hubble Space Telescope
14
Hubbles extra-sharp vision allows us to observe
individual Cepheid variable stars in galaxies up
to 100 million light-years away
15
Clicker Question Youve found a Cepheid variable
star in Galaxy A with a period of 100 days.
You've also found a Cepheid variable star in
Galaxy B with a period of 10 days. Both Cepheids
have the same brightness as seen from Earth.
Which galaxy is farther away from us?
  • GET YOUR ANSWER READY
  • A) Galaxy A
  • B) Galaxy B
  • C) Both are the same distance

16
Which galaxy is farther away?
  • Galaxy A
  • Galaxy B
  • Both are the same distance

17
White-dwarf supernovae can also be used as
standard candles
18
Step 5 Apparent brightness of white-dwarf
supernova (another kind of standard candle) tells
us the distance to its galaxy (up to 10 billion
light-years)
Supernova
19
In summary, we measure galaxy distances using a
chain of techniques known as the distance ladder
20
What is Hubbles Law?
21
By measuring velocities and distances of
galaxies, Hubble found that a galaxys velocity
and distance are related in a special way
22
The spectral features of virtually all galaxies
are redshifted ? Theyre all moving away from us
23
(No Transcript)
24
Redshift of a galaxy tells us its distance
through Hubbles Law distance
25
Distances of farthest galaxies are measured from
redshifts
26
What have we learned?
  • How do we measure the distances to galaxies?
  • Our measurements of galaxy distances depend on a
    chain of methods. The chain begins with radar
    ranging in our own solar system and parallax
    measurements of distances

27
What have we learned?
  • What is Hubbles law?
  • Hubbles law tells us that more distant galaxies
    are moving away faster. It allows us to determine
    a galaxys distance from the speed at which it is
    moving away from us, which we can measure from
    its Doppler shift.

28
Activity 49, page 185-188
  • Page 186 has 3 photos of a flat (2-dimensional)
    universe of galaxies, taken at 3 different times.
  • Use it to answer the questions in Part I on page
    185.
  • Well do those as clicker questions, then do the
    same for Part II.

29
2. If you were in one of the other galaxies,
would the MW (Milky Way) galaxy appear to be
moving away from you?
  • Yes
  • No
  • It depends

30
4. Are any of the galaxies moving closer to each
other?
  • Yes
  • No
  • Maybe

31
5. If we measured radial velocities of other
galaxies, what would we see?
  • All galaxies redshifted
  • All galaxies blueshifted
  • Some galaxies redshifted, some galaxies
    blueshifted

32
6. If someone in another galaxy measured radial
velocities of galaxies besides their own, what
would they see?
  • All other galaxies redshifted
  • All other galaxies blueshifted
  • Some galaxies redshifted, some galaxies
    blueshifted

33
Part II, page 187 (instructions on page 186)
  • Using Figure 2, fill in the blank entries in the
    lower right of Table 1 youre measuring how far
    galaxies A and B moved between images II and III,
    divided by the time elapsed between images II and
    III.
  • Then, using the bottom row of Table 1 (which
    youve just filled in), in Figure 3 plot the
    velocities of galaxies A and B as a function of
    their distance.
  • Then answer questions 8D, 9, 10.

34
8D. Figure 3 shows that the farther away a galaxy
is, the ___ it is moving away from the reference
galaxy.
  • Faster
  • Slower
  • Neither speed is independent of distance

35
9. How long has galaxy B been travelling if it
started at the origin in Fig. 2, moved at
constant speed, and ended up at its position in
Image III?
  • 2 billion years
  • 4 billion years
  • 8 billion years

36
10. Who do you think is correct?
  • Sam
  • Samantha
Write a Comment
User Comments (0)
About PowerShow.com