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Earth Science

Earth Science. With Mr. Thomas. Stars. cont. Characteristics: Early Observations: - Constellations: Groups of stars that depict an object, often used for navigation. - Examples include the Big & Small Dippers, Orion, and Pegasus.

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Earth Science

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  1. Earth Science With Mr. Thomas

  2. Stars cont. • Characteristics: • Early Observations: • - Constellations: Groups of stars that depict an object, often used for navigation. • - Examples include the Big & Small Dippers, Orion, and Pegasus. • - The positions of the constellations change with the seasons.

  3. Stars cont. • Apparent Magnitude: • - A measure of how bright a star appears to an observer on earth. (The lower the magnitude number, the brighter the star!) • Distance: • - Since things in space are so far apart, to measure in km’s would result in astronomically sized #’s! So we use: Astronomical Units (AU)

  4. Stars cont. - One astronomical Unit is equal to the distance from Earth to the Sun: - The nearest star (Proxima Centauri) is about 260,000 AU away (or 40 trillion km), so even with astronomical units, the numbers are getting really big, so we can use: 1 AU = 150 million km Light Years

  5. Stars cont. • One light year is the distance that light travels in one year. • Since light travels at a speed of • This distance is 300,000 km/s 9.5 trillion km

  6. Stars cont. • Proxima Centauri is about 4.2 light years away, or in other words, light takes 4.2 years to travel from that star to Earth! • So if a star is 75,000 light years away, it took that light 75,000 years to reach Earth, so the light we see is • 75,000 years old!!

  7. Stars cont. • Parallax: • - A change in an object’s direction or location due to a change in the observer’s position.

  8. Stars cont. • Star Elements: • The most abundant elements in stars are hydrogen and helium. • Temperature, color, and luminosity are given in the ESRT’s pg. 15. • Luminosity is the actual brightness of a star as compared to our sun and is only dependant upon size and temperature.

  9. Stars cont. • Absolute Magnitude: • A measure of how bright a star would be if all stars were the same distance from the Earth.

  10. Life Cycle of Stars: • The stars in our universe are at different stages in their life cycles. • These stages are outlined with distinct groups in the • or Hertzsprung-Russell Diagram H-R Diagram

  11. The H-R Diagram

  12. Life Cycle of Stars: • Beginning: • Nebula – Gas cloud • 2nd Step: • A) Star like our sun • B) Red Supergiant

  13. Life Cycle of Stars: • End Result: • A) Black Hole • B) Neutron Star

  14. Galaxies • Defn.: Systems containing millions or billions of stars and orbiting planets. • Types of Galaxies: Spiral Irregular Elliptical

  15. Origin of the Universe • Big Bang Theory: • The entire universe was created after a large explosion. • Evidence: • Expanding Universe (Red Shift) • Cosmic Background Radiation

  16. That's it for Today!

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