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Published byGervase Barrett Modified over 9 years ago
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The Universe Chapter 16
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Our Universe Only one that exists Includes everything –Stars, planets, galaxies, etc. Commonly accepted to be created by the Big Bang –A giant explosion of a very tiny dot of matter –Happened 15 billion years ago
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Evidence of Big Bang Theory Red shift –As objects move away, wavelength gets longer –Appears red or moves to the red end of the spectrum – When observing objects over time, their wavelengths are getting longer
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Evidence of Big Bang Theory Cosmic Background Radiation –Faint energy waves coming from every direction in the universe –Leftover from the Big Bang
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What Will Happen? Fate of the Universe depends on the mass
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Within the Universe….. Many galaxies grouped together in clusters –Held near each other by gravity
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Galaxies Three main types –Spiral –Elliptical –Irregular Classified by shape and age of stars Made of interstellar matter –Dust, gasses, stars, masses of rock
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Spiral Galaxy 30% of all galaxies in the universe Have stars of all ages
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Elliptical Galaxy 60% of all galaxies in the universe Have mostly old stars
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Irregular Galaxy Only 10% of all galaxies in the universe All young stars
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Our Galaxy - Milky Way A spiral galaxy
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Within the Milky Way….. All stars we see are in our galaxy Appear to make patterns in our sky –We call these constellations –Patterns don’t really exist –Really are light years apart Light year measures distance 1 light year = 9.5 x 10 15 m
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Stars Brightness in the sky depends on…. –Size Larger = brighter –Distance for Earth Closer = brighter –Temperature Hotter = brighter
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Stars Use color of stars to study them –Color tells us make up of stars Mostly hydrogen and helium –Color can tell us temperature Hot = blue Cool = red
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Stars Powered by nuclear fusion –Burn at a temperature of 15 million K –Energy takes 8 minutes to reach Earth Have a life cycle like living organisms –How long a star lives depends on its mass
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Star Life Cycle Start as a nebula –Cloud of dust and gas
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Star Life Cycle Nebula comes together in a large mass –Forms a protostar Nuclear fusion starts –Becomes a main sequence star –This is the true star –Lives most of its life here
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Star Life Cycle Death of star depends on mass –Very small stars become white dwarf –Medium mass stars become a red giant, then planetary nebula, then white dwarf –Large stars become a supergiant, then a supernova, then a black hole or neutron star
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Planetary Nebula
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SupernovaSupernova
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Our Star - The Sun A typical, average, medium mass star –Right now is a main sequence star –Is in the middle of its life Like most of the stars in the Milky Way Next closest star is 4.3 light years away
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Our Solar System Formed when a nebula started to spin –Pieces of rock and dust came together to form planets Our sun and everything that orbits around it –Nine planets, Asteroids, Comets, Meteors
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Our Solar System We can see some –Reflect the light of the sun –Appear to wonder across the sky because they are orbiting We can see 5 planets –Mercury, Venus, Mars, Jupiter, and Saturn –Besides the sun and moon, Venus is the the brightest in our sky
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Division of Solar System Inner Planets –Mercury, Venus, Earth, Mars –Small and mostly rock Asteroid belt –Asteroid = small rocky object that orbits the sun –Usually found in this belt Outer Planets –Jupiter, Saturn, Uranus, Neptune –Very large and mostly thick gas atmosphere
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Our Moon Rock that orbits Earth Reflects light of the Sun so we see it in the night sky –Depending on where it is, different amounts of sunlight hit the moon –Makes phases of the moon
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Phases of the Moon One cycle takes 4 weeks
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Eclipses When a shadow is cast over the sun or the moon Don’t happen all the time because moon’s orbit is at an angle
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Solar Eclipse You can only see a total solar eclipse when in the umbra. Total solar eclipses are very rare. These can only occur in the new moon phase.
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Lunar Eclipse You can only see a total lunar eclipse when in the umbra. Total lunar eclipses are the most likely to be seen. These can only occur in the full moon phase.
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