ASTRONOMY

1. There are 8 planets and a dwarf planet. The Sun is the center of our solar system: MERCURY; VENUS; EARTH; MARS; JUPITER; SATURN; URANUS; NEPTUNE; PLUTO My Very Excellent Mother Just Served Us Nine Pizzas ASTRONOMY SOLAR SYSTEM

2. MERCURY • Smallest and fastest planet • Orbit is 88 days • Surface is rocky and covered with craters • Has no moon

3. VENUS *Smaller than the Earth • *Wrapped in bright clouds (greenhouse effect) • Hottest Planet ; Temperatures 4640 C to 4800 C • Air is poisonous to humans; contains CO2 • High pressure • No moon • Composition: Mostly rock (Terrestrial)

4. EARTH • The Earth is 93 million miles (150 million km) • The different layers of the Earth are: Crust, Mantle, Core • Orbits the Sun in 365 days (= 1 year) • Rotates in 24 hours (= 1 day) • One moon

5. LUNATHE EARTH’S MOON • Dry, dusty land, flat plains, and craters • Earth’s gravity keeps the moon from going in a straight line • The light of the moon is the reflection of the sun’s light • The dark side of the moon is the Earth’s shadow

6. PHASES OF THE MOON • We always see the same side of the moon • Revolution (orbitaround the earth) is 27.3 days = 1 month • The positions of the moon, sun, and Earth determine the phases of the moon

7. ECLIPSES • A lunar eclipse happens when Earth comes between the sun and the moon and the shadow of Earth falls on the moon • A solar eclipse happens when the moon comes between Earth and the sun and the shadow of the moon falls on part of Earth

8. MARS • Rocky and shaped by running water • Looks red because the soil is rich in rust (iron oxide) • Same rotation as Earth (day) • Revolution is twice as long as Earth (687 earth days) • Has two small moons • Mons Olympus is a volcano, 16 miles high

9. JUPITER • A giant gas ball • The planet of storms • The Great Red Spot is a storm that never changes and it is as big as 3 Earths • Jupiter’s atmosphere consists of hydrogen, helium, some ammonia, methane, and H2O • Temperature of its interior can be 30,0000C • High winds (540 km/h) • Distance from sun 5,2 AU • Rotation: 9h, 55 min • Revolution: 11 years, 314 days

10. JUPITER’S MOONS • Europa, Ganymede, Callisto, and Io are Jupiter’s largest moons • Ganymede is the largest moon in the solar system List of all Jupiter Moons (63): 1. Metis  2. Adrastea  3. Amalthea  4. Thebe  6. Europa  7. Ganymede 8. Callisto  9. Themisto 10. Leda 11. Himalia 12. Lysithea   13. Elara 14. S/2000 15. Carpo 16. S/2003 17. Euporie 18. S/2003 19. S/2003 20. Thelxinoe 21. Euanthe 22. Helike 23. Orthosie 24. 25. S/2003 26. Ananke 27. Praxidike28. Harpalyke 29. Hermippe 30. Thyone 31. Mneme 32. S/2003 33. Aitne 34. Kale 35. Taygete 36. S/2003 37. Chaldene 38. S/2003 39. S/2003 40. S/2003 41. Erinome 42. Aoede43. Kallichore 44. Kalyke 45. Eurydome 46. S/2003 47. Pasithee 48. Cyllene 49. Eukelade 50. S/2003 51. Hegemone 52. Arche 53. Carme 54.Isonoe55. S/2003 56. S/2003 57. Pasiphae 58. Callirrhoe 59. Sinope 60. Sponde 61. Autonoe 62. Megaclite 63. S/2003

11. Major moons: Distance Radius Mass Satellite (000 km) (km) (kg) Discoverer Date --------- -------- ------ ------- ---------- ----- Pan 134 10 ? Showalter 1990 Atlas 138 14 ? Terrile 1980 Prometheus 139 46 2.70e17 Collins 1980 Pandora 142 46 2.20e17 Collins 1980 Epimetheus 151 57 5.60e17 Walker 1980 Janus 151 89 2.01e18 Dollfus 1966 Mimas 186 196 3.80e19 Herschel 1789 Enceladus 238 260 8.40e19 Herschel 1789 Tethys 295 530 7.55e20 Cassini 1684 Telesto 295 15 ? Reitsema 1980 Calypso 295 13 ? Pascu 1980 Dione 377 560 1.05e21 Cassini 1684 Helene 377 16 ? Laques 1980 Rhea 527 765 2.49e21 Cassini 1672 Titan 1222 2575 1.35e23 Huygens 1655 Hyperion 1481 143 1.77e19 Bond 1848 Iapetus 3561 730 1.88e21 Cassini 1671 Phoebe 12952 110 4.00e18 Pickering 1898 SATURN • 800 times bigger than the Earth • Many moons (more than 53) • Titan is the largest moon of Saturn • Has rings

12. SATURN’S MOONS • MAJOR MOONS (53 + 9): Pan 1990; Atlas 1980; Prometheus 1980; Pandora 1980; Epimetheus 1980; Janus 1966; Mimas 1789; Enceladus 1789; Tethys 1684; Telesto 1980; Calypso 1980; Dione 1684; Helene 1980; Rhea 1672; Titan 1655; Hyperion 1848; Iapetus 1671; Phoebe 1898 • RINGS: A-Ring, B, C, D, E, F, G.

13. URANUS • 300 times bigger than the Earth • 84 Earth years to orbit the sun • Strange thing: Orbits the sun on its side • Has rings

14. NEPTUNE • 300 times larger than the Earth • Two moons • Jupiter, Saturn, Uranus, Neptune are called OUTER PLANETS and GAS GIANTS

15. PLUTO • Dwarf planet in Kueper Zone • Rock and ice • Charon is Pluto’s moon • Charon is the COLDEST place on the entire solar system

16. ASTEROID BELT • Between the INNER PLANETS and the OUTER PLANETS is the Asteroid Belt • Full of asteroids that orbit the SUN • ASTEROIDS are made of chunks of rock and some ice and orbit the sun

17. GALAXIES • Galaxies are identified based on their shape • Clusters of billions of stars with different shapes: spiral, elliptical, irregular • Galaxies are composed of stars, star clusters, nebulas, and planetary systems • Classified by shape and by rate of star formation • Spiral galaxies have a bulge at the center and spiral arms.

18. The Milky Way • Our galaxy is a spiral shape and is called the Milky Way • Consists of about 200 billion stars • The sun is located about 2/3 of the way between the center of the galaxy and the galaxy’s edge

19. ELLIPTICAL GALAXIES • Elliptical Galaxies are round or oval (cosmic snowballs) • They have stopped making new stars more than 10 billion years ago. • They are the largest galaxies in the universe • Contain up to 5 trillion stars • They form by the merging of smaller galaxies

20. IRREGULAR GALAXIES • Irregular galaxies are galaxies that have no definite shape • Smallest ones have only about 10 million stars • Form new stars slowly • Some form when galaxies • collide • The Milky Way is consuming a pair of nearby irregular galaxies

21. CONTENTS OF GALAXIES • Galaxies contain stars, planetary systems, gas clouds and star clusters • Gas Clouds are called nebulas and they are large clouds of gas and dust where stars are born • Some nebulas glow, other types absorb light and hide stars, and others reflect starlight

22. STAR CLUSTERS • A globular cluster is a highly concentrated group of stars that looks like a ball • May have up to 1 million stars • Open clusters are groups of 100 to 1,000 stars that are close together relative to other stars

23. QUASARS • Quasars are among the most distant objects in the universe • Star like sources of energy that are located in the centers of galaxies • They generate energy at a high rate and are among the most powerful energy sources in the universe • May be caused by massive black holes in the cores of galaxies • The quasar known as PKS 0637-752 radiates with the power of 10 trillion suns

24. ORIGIN OF GALAXIES • Scientists investigate the early universe by observing objects that are extremely far away in space • Because light takes time to travel through space, looking through a telescope is like looking back in time • Looking at distant galaxies reveals what early galaxies looked like

25. FORMATION OF THE UNIVERSE The Big Bang Theory • Most galaxies are moving away from each other and the universe is expanding • About 14 billion years ago, all of the contents of the universe were compressed under tremendous pressure, at high temperature and high density, into an extremely small volume • The universe was contracting and all matter squeezed together in one small volume • Then expanded and cooled • Galaxy formation

26. FORMATION OF THE SOLAR SYSTEM • The collision of particles formed bodies the size of boulders and asteroids • As the mass of particles increased, gravity increased • Matter in the solar nebula was pulled together by gravity into spheres

27. FORMATION OF THE SOLAR SYSTEM • The solar nebula collapsed, rotated • Becomes hot and dense in its center • The gas and dust forms a disk • The disk begins to cool enough for dust particles to form • Particles begin to collide and form larger particles

28. GRAVITY AND THE UNIVERSE • Gravitational attraction pulls objects toward one another • All objects experience gravity • After the big bang, gravitational attraction caused the matter distributed throughout the universe to form galaxies • The mutual attraction between galaxies caused galaxies to cluster • Even though the distances between galaxy clusters are very large, gravity still acts between them • Because gravity acts over such great distances, gravity controls the size and shape of the universe

29. HOW OLD IS THE UNIVERSE? • Astronomers can estimate the age of the universe by studying whitedwarfs, the oldest stars in the Milky Way • White dwarfs are the burned-out cores of stars that started out with masses that were less than 8 times the mass of the sun • These stars have cores of carbon and oxygen at the end of the red giant phase • They lose their atmospheres in the planetary nebula stage • The planetary nebula stage is a stage in which the hot central region of a star drives off the star’s cooler atmosphere over a period of a few thousand years.

30. HOW OLD IS THE UNIVERSE? • Once the star’s atmosphere is lost, all that is left is the carbon-oxygen core- a white dwarf-which is tiny, hot, and dense • The oldest white dwarfs are 12 billion to 13 billion years old • Because it took about 1 billion years after the big bang for the first white • dwarfs to form from the first stars, the universe must be approximately 14 billion years old

31. THE LIFE CYCLE OF STARS • Stars can exist for billions of years • Scientists study stars at different stages to understand how they develop • Stars are classified by mass,size, brightness, color, temperature, composition, and age • Stars are different as they age • The fast-expanding gas clouds in the picture show a dying star

32. LIFE CYCLE OF SUNLIKE STARS PROTOSTARS -1st Stage • A star begins its life as a ball of gas and dust • Gravity pulls the gas and dust into a sphere • As the sphere becomes denser it gets hotter and hotter to 10,000,0000 Cin its center • Hydrogen nuclei combine to become helium • This is called nuclearfusion • Causes energy to be released

33. LIFE CYCLE OF SUNLIKE STARS MAIN-SEQUENCE STARS • After it is formed, it enters the main sequence • Second and longest stage of its life cycle • Energy is generated in the core of the star as hydrogen atoms fuse into helium atoms. • Size changes very little

34. LIFE CYCLE OF SUNLIKE STARS GIANTS AND SUPERGIANTS • When a main-sequence star uses all of the hydrogen in its core, helium begins to fuse • The center of the star shrinks • The atmosphere of the star grows very large and cools • The star may become a red giant or red supergiantex. Betelgeuse

35. LIFE CYCLE OF SUNLIKE STARS WHITE DWARFS • In the final stage of its life cycle, a sunlike star becomes a white dwarf • Small, hot, and dim star that is the leftover center of a red giant • No longer generates energy by nuclear fusion • Slowly cools and becomes smaller • A white dwarf can shine for billions of years

36. H-R DIAGRAM The Sun *Middle age *5 billion years old Blue= Hot Yellow= MediumRed = Cool

37. THE AGING OF MASSIVE STARS • Massive stars use their hydrogen much faster than stars like the sun do • More energy and they are very hot! • Shorter lives SUPERNOVAS • At the end, a massive star may explode in a large, bright flash called supernova • A supernova is a gigantic explosion in which a massive star collapses and its outer layers are blasted into space

38. THE AGING OF MASSIVE STARS PULSARS -If a neutron star is spinning, it is called a pulsar • Pulsars send out beams of radiation that sweep across space like a lighthouse over the ocean • Detected by radio telescopes as pulses

39. THE AGING OF MASSIVE STARS NEUTRON STARS • The center of the supernova (collapsed star) may contract into a very small but very dense ball of neutrons • This ball of neutrons is called Neutron Star • One teaspoon of matter from a neutron star would weigh 100 million metric tons of Earth • A lot of energy (100,000 suns)

40. THE AGING OF MASSIVE STARS BLACK HOLES • An object so dense and massive that light cannot escape its gravity • If the center of a collapsed star has a mass several times the mass of the sun, the star may contract more because of too much gravity • The force of the contraction crushes the dense center of the star and leaves a black hole

41. BLACK HOLES

42. BLACK HOLES

43. BLACK HOLES • Black holes do not give off light • Locating them is difficult • If a star is nearby, some gas or dust from the star will spiral into the black hole and give off X rays • These X rays allow astronomers to detect the presence of black holes • The sun will never become a Black Hole • Stars with 10 -100 million times the mass of the sun • Stellar- Mass Black Hole & Supermassive Black Hole

44. INTERPLANETARY DISTANCES • Astronomical Unit (AU) is the average distance between the sun and Earth (150,000,000 km) • Light minute or light hour • 1s = 300,000 km • 1 min = 18,000,000 km (light minute) • 1 AU = 8.3 light minutes • Used to measure distances within the SOLAR SYSTEM Example: between planets or the sun and a planet • Light Year: used to measure outside the solar system =9.5 trillion km Example: between galaxies and stars

45. Comets • Small, loosely packed bodies of ice, rock, and cosmic dust • The core is rock, metals, and water ice • The coma surrounds the nucleus and is made of gas and dust • Comet tails—sunlight causes the comet’s ice to change to gas thus forming the tails • One tail is made of ionized gas (no electrons) and points away from the sun • The other is made of dust and gas

46. Comets • Comets are found in the Kuiper belt (flat ring of objects located beyond Neptune’s orbit) • Oort cloud--spherical cloud of dust and ice that surrounds the solar system far beyond Pluto’s orbit

47. ASTEROIDS--Asteroid Beltpg502 • Asteroid Belt is made of asteroids between Mars and Jupiter • Located betweenthe Inner Solar System and the Outer Solar System • Asteroids are small (1,000 km) rockyand some metal bodies • Revolve around the sun

48. Meteoroids • Dust and debris from asteroids and comets within our solar system • When enter Earth’s atmosphere reach speeds of 35,000-250,000 km/h • Friction heats the meteoroids to thousands of degrees Celsius • Glow brightly

49. Meteors • The glowing trails that result when meteoroids burn up in Earth’s atmosphere

50. Meteorites • Larger bodies that pass through Earth’s atmosphere without burning up and strike Earth • Three types: Stony, metallic, Stony-iron meteorites