SOLAR SYSTEM LESSON4-5-6

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Across
  1. 6. When the earth crosses the tail of comet,swarms of meteors are seen.
  2. 8. are stony meteorites which do not
  3. 10. The body that reaches the earth is called.
  4. 11. meteorites, as their name suggests,
  5. 15. Which appear after nearly every 76 year. It was seen in 1986.
  6. 20. They are believed to have condensed directly out of the solar nebula, making them the most ‘pristine’ material in the Solar System.
  7. 23. is the fireball seen in the sky when a meteoroid collides with the Earth’s atmosphere.
  8. 27. He predicted that the Sun released a steady stream of charged particles with speeds of a few 100 km/s.
  9. 28. man-made satellite
  10. 31. is a piece of rocky space debris orbiting the Sun at typically 20 - 40 km/s,some of which are on a collision course with the Earth.
  11. 32. are composed of about 50% silicates and 50% iron, and make up only about 1% the of meteorite falls.
Down
  1. 1. are small Solar System bodies.
  2. 2. is the remnant of a meteoroid which has survived the fireball to impact on the Earth’s surface.
  3. 3. lead to suggest in the early 1600s that cometary tails were effected by the pressure of sunlight.
  4. 4. an explosion was felt hundreds of kilometers away and felled trees over an area of 2000 square kilometers.
  5. 5. are small spherical pebbles, generally 0.1 mm to 10 mm in size, found in the primitive chondrites.
  6. 6. As comets burn out*, dust and rock fragments form a compact which for many years continues to circle the Sun in the orbit of the parent comet.
  7. 7. make up the remaining 95% of meteorite falls, and are divided into three types: chondrites, achondrites & carbonaceous.
  8. 9. chondrules or volatiles and have far less iron than chondrites.
  9. 10. it is generally known as "shooting star" or "falling star".
  10. 12. a stream of ionised gas emanating from the Sun, was discovered ten years later in 1962.
  11. 13. There is large gap in between the orbit of Mars & Jupiter.
  12. 14. Crater would have had a diameter between 50 and 100 meters.
  13. 16. bodies that have been chemically sorted.
  14. 17. some larger meteoroids can actually explode in the air before they hit the ground.
  15. 18. are composed of silicate rock & rounded bits of glassy rock.
  16. 19. trace amounts of gas that resembles the atmosphere of Mars, which is trapped within microscopic pockets of the rocks.
  17. 21. tails of comets, point in a slightly different direction though still away from the Sun.
  18. 22. meteorites are extremely rare - less that 0.1% of all meteorites are of lunar origin.
  19. 24. carbon and some complex organic material. They can also contain as much as 20% water and other volatile compounds.
  20. 25. Earth are typically 10-20 times as large as the diameter of the meteorite which causes it.
  21. 26. formed when large meteorites strike
  22. 29. meteors are dust particles from the Temple-Tuttle comet.
  23. 30. meteorites are composed of about 90% iron and 10% nickel. They make up about 4% of the Earth’s meteorites.