1 / 15

Office Hours

Office Hours. Tue: 12:30 PM to 2:30 PM Wed: 9:00 AM to 10:30 AM & 12:00 PM to 2:00 PM Thr : 9:00 AM to 10:30 AM Course Syllabus can be found at: http://www.wx4sno.com/portfolio/BSU/Fall_2011 / This lecture will be posted AFTER class at:

ian-fulton
Download Presentation

Office Hours

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. Office Hours Tue: 12:30 PM to 2:30 PM Wed: 9:00 AM to 10:30 AM & 12:00 PM to 2:00 PM Thr: 9:00 AM to 10:30 AM Course Syllabus can be found at: http://www.wx4sno.com/portfolio/BSU/Fall_2011/ This lecture will be posted AFTER class at: http://www.wx4sno.com/portfolio/BSU/Fall_2011/Lectures/

  2. Lesson 10 Earth-Sun Relationships Hess, McKnight’s Physical Geography, 10 ed. 15-21 pp.

  3. Terms to Know • Rotation: Earth completes one rotation every 24 hours giving us day and night.

  4. Terms, cont. • Revolution: Earth completes one revolution around the sun every 365 ¼ days.

  5. Terms, cont. • Revolution is not a perfect circle, more of an elliptic. • When revolution brings earth closest to sun: perihelion • When revolution takes earth furthest from sun: aphelion Point 1: Earth at aphelion Point 2: Earth at perihelion Point 3: Sun

  6. Perihelion and Aphelion, cont.

  7. Terms, cont. • Ecliptic plane: This is the level, or plane, of Earth’s orbit around the sun…Earth’s orbital path. • Astronomically, this is the primary plane referred to when discussing the revolution of other planets around the sun

  8. Terms, cont. • Inclination: Relative to the ecliptic plane, Earth is tilted 23.5° from vertical at all times.

  9. Terms, cont. • Polarity: Because Earth is always tilted 23.5°, it’s axis is always pointed in the same direction…towards the star Polaris. • Because of this regular tilt, when the Earth revolves around the sun, the North pole is either tilted towards the sun (June) or tilted away from the sun (December) • DO NOT confuse this with Earth’s magnetic field!

  10. Earth’s Equinoxes • Equinox: Earth is positioned so that its is neither towards nor away from the sun…giving the entire planet equal amounts of day and night. • Occurs twice each year, around March 20 and September 22.

  11. Earth’s Solstices • Solstice: Earth is positioned where its tilt is either towards or away from the sun. • Occurs twice a year, just like the Equinoxes, around June 21 and December 21. • The direct rays from the sun hit the earth at 23.5°N on June 21, while the tangent rays hit the earth around 66.5°N and 66.5°S.

  12. Sun’s Rays during Equinoxes

  13. Sun’s Rays during Summer Solstice

  14. Sun’s Rays during Winter Solstice

  15. Video on Seasons • http://www.youtube.com/watch?v=taHTA7S_JGk • Powers of ten: • http://youtu.be/vRjGarICal4 • http://youtu.be/0fKBhvDjuy0

More Related