1 / 0

Newtons First Law Newtons Second Law Newtons Third Law F=ma F= μmg F= μma F NET = F 1 + F 2 + F 3 … F fr F drag F

Newtons First Law Newtons Second Law Newtons Third Law F=ma F= μmg F= μma F NET = F 1 + F 2 + F 3 … F fr F drag F app Force Tension Gravity Acceleration Coefficient of Drag/Friction. Gravitation & Kepler’s Laws. Kepler’s Laws.

rosie
Download Presentation

Newtons First Law Newtons Second Law Newtons Third Law F=ma F= μmg F= μma F NET = F 1 + F 2 + F 3 … F fr F drag F

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. Newtons First Law Newtons Second Law NewtonsThird Law F=ma F=μmg F= μma FNET = F1 + F2 + F3… Ffr Fdrag Fapp Force Tension Gravity Acceleration Coefficient of Drag/Friction
  2. Gravitation & Kepler’s Laws

  3. Kepler’s Laws Kepler’s First Law: Planets orbit in Ellipses Kepler’s Second Law: Planets travel distances that cover equal amounts of area in the ellipse per month.
  4. Kepler’s Laws Kepler’s Third Law: The ratio of two planets periods (squared) is equal to the ratios of distances of the two planets to the sun (cubed). (TA/TB)2 = (rA/rB)3 T = period (time for one trip around the sun) r = distance to sun
  5. Newton’s Law of Universal Gravitation Gravitational Force is a field force that is based on an amount of mass two objects have which make them attract to each other. FGravitation = G (m1m2/r2) G = 6.67E-11 Nm2/kg2 M1 or M2 = mass of objects one and two R = distance between two centers of the two masses
  6. Orbits Period of a Planet Orbiting the Sun or Satellite orbiting the earth: T = 2π√(r3/Gm) G = 6.67E-11 Nm2/kg2 M= mass of the sun for a planet orbiting the sun or mass of earth for a satellite orbiting the earth R = orbiting radius
More Related