1 / 17

Tuesday, Sept. 10: 17:20 – 19:10 Wednesday, Sept. 10: 17:20 – 19:10

Evening Classes (Chap. 1 and 2). Tuesday, Sept. 10: 17:20 – 19:10 Wednesday, Sept. 10: 17:20 – 19:10 Thursday, Sept. 10: 17:20 – 19:10 Building 6, Room 125 (For students of Dr. Al Ramadan). General Physics (PHYS101). Coordinate systems, vectors and scalars Lecture 05 (Chap. 3).

aira
Télécharger la présentation

Tuesday, Sept. 10: 17:20 – 19:10 Wednesday, Sept. 10: 17:20 – 19:10

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. Evening Classes (Chap. 1 and 2) Tuesday, Sept. 10: 17:20 – 19:10 Wednesday, Sept. 10: 17:20 – 19:10 Thursday, Sept. 10: 17:20 – 19:10 Building 6, Room 125 (For students of Dr. Al Ramadan)

  2. General Physics (PHYS101) Coordinate systems, vectors and scalars Lecture 05 (Chap. 3) www.cmt.ua.ac.be/golib/PHYS101

  3. 2 4 5 1 3 Coordinate Systems • Coordinate systems are used to describe the position of an object in space • Coordinate system (frame) consists of: • a fixed reference point called the origin • specific axes with scales and labels • instructions on how to label a point relative to the origin and the axes 0 x (cm)

  4. 2D Coordinate Systems • Cartesian (rectangular) • Polar (plane)

  5. y (cm) x (cm) Cartesian Coordinate Systems • x- and y- axes • points are labeled (x,y)

  6. Polar Coordinate Systems • the origin and the reference line • point is distance r from the origin in the direction of angle , from the reference line • points are labeled (r, )

  7. Coordinate conversions • from polar coordinate to Cartesian coordinate • from Cartesian coordinate to polar coordinate

  8. Trigonometric functions • Pythagorean Theorem • c2=a2+b2

  9. height=dist. tan =(tan 39.0o)(46.0 m)=37.3 m Trigonometric functions Example: how high is the building? Known: angle and one side Find: another side

  10. x Scalar and Vector Quantities • Scalar quantities are completely described by magnitude only (temperature, mass, time, length ...) • Vector quantities need both magnitude (size) and direction to completely describe them (force, displacement, velocity ...) • Represented by an arrow, the length of the arrow is proportional to the magnitude of the vector • Head of the arrow represents the direction

  11. Vector Notation • When handwritten, use an arrow: • When printed, will be in bold print: • A normal letter is used for its magnitude:

  12. Properties of Vectors • Two vectors are equal if they have the same magnitude and the same direction • Two vectors are negative if they have the same magnitude but are 180o apart (opposite direction) • The resultant vector is the sum of a given set of vectors

  13. y • Rotation is not allowed!!! x Properties of Vectors • Any vector can be moved parallel to itself without being affected

  14. Division and multiplication by a Scalar • The result of the multiplication and division is a vector • The magnitude of the vector is multiplied or divided by the scalar. • If the scalar is positive, the direction of the result vector if the same as of the original vector • If the scalar is negative, the direction of the result vector if the opposite as of the original vector

  15. Division and multiplication by a Scalar

  16. displacement distance Examples: Distance or Displacement? • Distance may be, but is not necessarily, the magnitude of the displacement. • Distance - scalar quantity. • Displacement - vector quantity.

More Related