Exploring the Universe

1. Exploring the Universe

2. I.) Properties of Stars • Color and Temperature • A star’s color indicates that temperature of its surface • Hottest stars (surface temps above 30,000K) appear blue • Milder stars (surface temps between 5,000-6,000K) appear yellow • Relatively cool stars (surface temps ~3,000K) appear red

3. Hertzsprung-Russell Diagram: a graph of the surface temperature (or color) and absolute brightness of a sample of stars • H-R diagrams are used to estimate the sizes of stars and their distances, and to infer how stars change over time • Horizontal axis=surfacetemperature • Vertical axis=absolutebrightness

4. H-R Diagram

6. Main-Sequence Stars • Mainsequence: A line or sequence in an H-R diagram where most stars spend 90% of their life. • A diagonal band running from the bright, hot stars on the upperleft to the dim, cool stars on the lowerright • Example: The Sun lies in the main sequence

7. Giants and Dwarfs a. Very bright stars in upper right of H-R diagram are known as supergiants • Very large (100 to 1000 times the diameter of the sun) • Just below the supergiants are the giants • Below the main sequence are the whitedwarfs, which are the small, dense remains of a low- or medium-mass star

8. Energy From Stars • Energy moves through the layers of a star by combination of convection, conduction, and radiation • Convection: rising hot gas moves upward, away from the star’s center, and cooler, denser gas sinks toward the center

9. Brightness of a Star • The actual “brightness” of a star depends upon 3 things: actual size of the star, temperature, and distance from Earth

10. Radiation occurs when energy radiates out from the star in the form of light • Travels at the speed of light • Light from Sun takes 8 minutes to reach Earth • Light and heat both travel this way from a star

11. II.) Life Cycle of Stars • How Stars Form • Nebula: a large cloud of dust & gas in interstellar space • Composed of mainly hydrogen gas • Gravity pulls the small pieces of dust to clump together & form a protostar

14. Nuclear fusion begins to take control over the gravity and the star begins to stabilize • Fusion reactions in the core produce an outward force that balances the inward force of gravity

15. Adult Stars • Most stars spend 90% of their life in mainsequence • Once achieving nuclear fusion, stars radiate energy into space

16. The Death of a Star • When the hydrogen fuel has run out & fusion can no longer continue, the star collapses because the forces are no longer balanced • Core collapses because of its own gravity & then rebounds with a shock wave that violently blows the star’s outer layers away from the core

17. The path a star takes in its life cycle depends on its size/mass

18. LARGE MASS STARS : Results in huge, bright explosion called a supernova • Supernova produce heavier elements up to the element iron.

19. The path a star takes in its life cycle depends on its size/mass

20. http://www.youtube.com/watch?v=xsfie0Ly0Ic&NR=1&feature=fvwp

21. III.) Expanding Universe • Hubble’s Law • Edwin Hubble used observations of spectral lines from other galaxies to conclude that the universe is expanding • Lines shifted toward the red end of the visible light spectrum • http://www.youtube.com/watch?v=FhfnqboacV0 • http://www.youtube.com/watch?v=3kw4id0NvJ0&NR=1&feature=fvwp

22. Redshift: the apparent shift toward longer wavelengths of light caused when a luminous object moves away from the observer • Red shift showed that nearly all galaxies are getting fartheraway from Earth • Blueshift: an apparent shift toward shorter wavelengths of light caused when a luminous object moves towards the observer

23. Big Bang Theory • The Big Bang Theory states that all matter and energy in the universe was compressed into an extremely small volume that 10 to 20 billion years ago exploded and began expanding in all directions

24. What force is responsible for causing interstellar material to condense and form our sun? • GRAVITY

25. Evidence for the Bang • Redshift, and cosmicbackgroundradiation • Cosmicbackgroundradiation: steady, but very dim signals in the form of microwaves that are emitted all over the sky • Scientists believe that these microwaves are the remains of the radiation produced during the Big Bang

26. 4. What is the future of our universe? • It all depends on the mass of our universe • One of 3 things can happen: • Universe can continue to expand • Universe can stop expanding and remain constant • Universe can collapse in on itself (“Big Crunch”)

27. What causes the moon to “shine?” • It’s actually a reflection of the sun’s light off the surface, back to the earth.

28. IV.) Phases of the Moon & Eclipses • The different shapes of the moon visible from Earth are called phases • Moon’s phases are caused by changes in the relative positions of the moon and Earth as the moon revolves around the Earth [Fig 8, p.634] • http://aspire.cosmic-ray.org/labs/moon/lunar_phase3.swf

30. http://www.sumanasinc.com/webcontent/animations/content/moonphase.htmlhttp://www.sumanasinc.com/webcontent/animations/content/moonphase.html

31. Eclipse: an event in which the shadow of one celestial body falls on another [Fig 9, p.635] • Caused by the changes in relative positions of the moon, sun, and Earth—when all three are lined up in a certain order • Solar Eclipse: Moon blocks the sun • Lunar Eclipse: Earth’s shadow blocks the moon

32. Solar vs Lunar Eclipses

33. http://www.youtube.com/watch?v=XMyqPxFh5Zw

34. http://www.youtube.com/watch?v=nXseTWTZlks&feature=related • http://www.youtube.com/watch?v=wHxcWSiD_4E

35. Tides • Caused by the differences in the pull of the moon’s gravity on different areas of the Earth • Coastal areas have two high tides and two low tides each day • Times of the tides will vary because the moon is orbiting around the Earth

38. The Milky Way- our galaxy is a spiral galaxy