1 / 12

The Moon

The Moon. Joel Tome Aaron Fujioka Pd. 3. The Moon. A roughly spherical and rocky body which orbits the Earth at an average distance of 382,942 km Moon diameter = ¼ Earth diameter Moon mass = 1/80 Earth mass. Rotation and Orbit. Rotates on axis every 29.5 days Axis tilted

carsyn
Télécharger la présentation

The Moon

An Image/Link below is provided (as is) to download presentation Download Policy: Content on the Website is provided to you AS IS for your information and personal use and may not be sold / licensed / shared on other websites without getting consent from its author. Content is provided to you AS IS for your information and personal use only. Download presentation by click this link. While downloading, if for some reason you are not able to download a presentation, the publisher may have deleted the file from their server. During download, if you can't get a presentation, the file might be deleted by the publisher.

E N D

Presentation Transcript


  1. The Moon Joel Tome Aaron Fujioka Pd. 3

  2. The Moon • A roughly spherical and rocky body which orbits the Earth at an average distance of 382,942 km • Moon diameter = ¼ Earth diameter • Moon mass = 1/80 Earth mass

  3. Rotation and Orbit • Rotates on axis every 29.5 days • Axis tilted • Craters near south pole always in shadows • Sidereal month: complete orbit of Earth • Synodic month: one lunar day, relative to sun

  4. Origin and Evolution • Collision known as “Giant Impact” or the “Big Whack” • Occurred 4.6 billion years ago between Earth and planet-sized object • Resulted in a cloud of vaporized rock which came from Earth’s surface

  5. Origin and Evolution cont. • Vaporized rock went into Earth’s orbit • Cloud cooled and condensed into a ring of small and solid bodies • Gathered together and formed the moon

  6. Origin and Evolution cont. • The quick joining together released lots of energy as heat • Creating an “ocean” of magma • It slowly cooled and solidified

  7. Origin and Evolution cont. • As the crust formed, asteroids continually hit the moon • One created the South Pole-Aitken Basin • One of the largest known impact craters in solar system

  8. Interior of the Moon • Crust- Average thickness is 43 miles • Mantle- Formed during period of global melting, low density minerals floated to the outer layers and dense minerals sank deeper • Core- Radius of 250 miles, consists mostly of iron and may contain large amounts of sulfur

  9. Surface Features • Craters: result from meteoroids, asteroids, comets • Basins: craters 190 mi or more in diameter, rings vary with size • Maria: dark areas on the surface of the moon (16% of SA)

  10. Surface Features cont. • Wrinkle ridges: blister-like humps across Maria • Rilies: snakelike depression across Maria • Volcanic features: dome/cone-shaped areas

  11. The moon’s volcanic past • Contained active volcanoes for billions of years • Large dark areas filling the moon’s craters indicate the largest volcanic flows • Almost exclusively on the near side

  12. Works Cited • Angelo, Joseph A., Jr. "Moon." Science Online. Facts On File, Inc. Web. 21 Jan. 2011. <http://www.fofweb.com/activelink2.asp?ItemID=WE40&SID=5&iPin=ESA1805&SingleRecord=True>. • Elkins-Tanton, Linda T. "Moon." Science Online. Facts On File, Inc. Web. 18 Jan. 2011. <http://www.fofweb.com/activelink2.asp?ItemID=WE40&SID=5&iPin=SSEM0007&SingleRecord=True>. • "Moon." Gale Encyclopedia of Science. Ed. K. Lee Lerner and Brenda Wilmoth Lerner. 4th ed. Detroit: Gale Group, 2008. Discovering Collection. Gale. Mid-Pacific Institute. 14 Jan. 2011 <http://find.galegroup.com/srcx/infomark.do?&contentSet=GSRC&type=retrieve&tabID=T001&prodId=DC&docId=EJ2644041517&source=gale&srcprod=DISC&userGroupName=mid&version=1.0>. • Spudis, Paul D. "Moon." World Book Advanced. World Book, 2011. Web.  18 Jan. 2011.

More Related