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Why are Cepheid variable stars useful in determining distances?. They all have the same distance.Their luminosity can be determined from their pulsation period.They all have the same luminosity.They all have the same radius.. How big is the Universe?. Spiral nebulae were identified not long after
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1. Galaxies How big is the Universe?
2. Why are Cepheid variable stars useful in determining distances? They all have the same distance.
Their luminosity can be determined from their pulsation period.
They all have the same luminosity.
They all have the same radius.
3. How big is the Universe? Spiral nebulae were identified not long after development of the telescope around 1600
In the 1600s, it was suggested that spiral nebula are separate galaxies so far away that the stars blur together, but most people thought they were clouds of gas
The question wasnt resolved until 1923.
4. Are there different types of objects here?
5. Great debate Two astronomers held a great debate in 1920
Harlow Shapley argued the Milky Way was the whole Universe
Heber Curtis argued the Milky Way was just one of many galaxies island universes
Held in the Smithsonian's Museum of Natural History the auditorium still looks the same
6. Distance to the Andromeda spiral nebula In 1923, Edwin Hubble found Cepheid variables in the Andromeda nebula and showed that the nebula was at a great distance, much larger than the size of the Milky Way.
7. A Cepheid is found with an oscillation period of 30 days. It is 700,000 times dimmer than another Cepheid with a period of 30 days at a known distance of 1000 pc. How far away is the dimmer Cepheid?
8. Flux and Luminosity Flux decreases as we get farther from the star like 1/distance2
Mathematically, if we have two stars A and B
9. Standard Candles
10. Standard Candles
11. How big is the Universe? Greeks (up about 100 B.C.)
Earth at Center
Universe extends to sphere of Saturn, largest measured distance is from Earth to Sun at several million miles
Renaissance (1500-1650)
Sun at Center
Universe extends to `distant stars with inferred distance of about 100 billion miles, largest measured distance is from Sun to Saturn at about 1 billion miles
12. How big is the Universe? Parallax to stars
First parallax measured in 1838 to star 61 Cygni of 0.3 arcseconds for a distance of 11 ly = 7×1013 miles.
Distance to center of Milky Way
from star counts 5000-10,000 ly (1785-1810)
from globular clusters 50,000 ly (1915)
Distance to Andromeda nebula
from Cepheids 2,000,000 ly (1923)
(really 2,500,000 ly)
13. What evidence do we have that there is hidden mass in the galaxy? cool clouds of hydrogen
RR Lyrae variable stars in globular clusters
flat rotation curve at large radii
dusty regions in the plane
14. Galaxies Types of galaxies
Elliptical
Spiral
Irregular
15. M100
16. NGC 1365
17. M87
18. NGC 3377
19. NGC 4449
20. Classifying Galaxies
21. Elliptical galaxies
22. Elliptical galaxies
23. Often occur in clusters
24. Spiral galaxies
25. Spirals vary in prominence of bulge, tightness of arms, presence of bar
26. Irregular galaxies have asymmetric shapes and usually lots of young stars They are often found near other galaxies
27. In which type of galaxy are stars orbits distributed in random directions? elliptical galaxies
spiral galaxies
barred spiral galaxies
blue galaxies
28. Our Galaxy is a member of a small cluster called the Local Group
29. MW eating neighbors
30. Review Questions What was the definitive evidence showing that spiral nebulae are actually entire galaxies outside of the the Milky Way?
What are the types of galaxies?
How do the rotation patterns of stars differ in elliptical versus spiral galaxies?
What is the Local Group?
31. Cosmic Distances How to measure distances
Primary distance indicators
Secondary and tertiary distance indicators
Recession of galaxies
Expansion of the Universe
32. Stellar Parallax
33. Stellar Parallax
34. Standard Candles
35. Distances to galaxies Standard candles, such as Cepheid variables, the most luminous supergiants, globular clusters, H II regions, and supernovae in a galaxy, are used in estimating intergalactic distances.
36. Each stage in the ladder overlaps the previous and next
Cepheid distances are critical
Tully-Fisher, fundamental plane apply to whole galaxies
Supernova are now the best estimators at large distances The Distance Ladder
37. Doppler effect for light
38. Light from distant galaxies is redshifted
39. Distances and velocities of galaxies If you measure the distances to a large set of galaxies and also measure the speed of the galaxies using the redshift, what do you find?
40. Hubble expansion v = H0d
41. Expansion of the Universe
42. Motion at constant velocity
43. Receding galaxy
44. Hubble expansion v = H0d
45. An observer at a distance of 3 billion light years from us looking in our general direction would see most of the galaxies approaching her.
the same Hubbles law that we see.
about equal numbers of red and blue shifted galaxies.
everything rushing away from a point near the Milky Way galaxy.
46. Expansion of the Universe Blow up the balloon to about a 3 inch diameter. Twist the neck and hold it closed so that no air escapes, but do NOT make a knot because you will need to blow it up some more. Make SIX dots on its surface to represent galaxies and label them A-F.
Measure and record the distances from cluster A to each of the other 5 clusters.
Measure and record the distances from cluster D to each of the other 5 clusters.
Blow up the balloon up more, to a diameter of about 6 inches. Measure the distances between the same clusters again and record them.
47. Expansion of the Universe Are all the other clusters moving away from cluster A?
Are all the other clusters moving away from cluster D?
Is there a cluster that could be considered to be at the center of the universe as represented by the surface of the balloon?
48. Formation of Galaxies Spiral versus elliptical
Young Universe
Collisions and Interactions
Starbursts
Elliptical galaxies
49. Formation of a Spiral Galaxy
50. Formation of an Elliptical Galaxy
51. Stellar Birthrate in Galaxies
52. Formation of Galaxies This picture of galaxy formation is incomplete
Mergers, collisions, and interactions between galaxies are very important in their formation, particularly in the early stages of the Universe (why?)
53. Expansion of the Universe The Universe is expanding
This means that the Universe used to be smaller
In the early stages of the Universe
there were more galaxies
they were closer together
therefore, they interacted more
54. Young Universe
55. Young Universe
56. Young Universe
57. Young Universe
58. Colliding galaxies
59. The Mice
60. Cartwheel galaxy
61. Seyferts Sextet
62. Interacting galaxies
63. Interacting galaxies
64. Starburst galaxy M82
65. M82 in X-rays
66. Colliding galaxies
67. Galaxy interactions Interactions can rip stars out of galaxies, producing tidal tails
Interactions can disturb gas in and between galaxies, producing starbursts
Collisions can randomize stellar orbits leading to the formation of elliptical galaxies
68. Formation of an Elliptical Galaxy Movie
69. Galaxy growth via interactions Galaxies initially form from mergers of several gas clouds
Galaxies then are changed by interactions
Galaxies grow gradually by galactic cannibalism
Interactions disturb gas leading to starbursts
Collisions can randomize stellar orbits leading to the formation of elliptical galaxies
70. Review Questions How are elliptical versus spiral versus irregular galaxies formed?
How do the star formation histories of elliptical versus spiral galaxies differ?
Why do galaxy interactions tend to cause star formation?
Was the population of galaxies different in the past?