Download Circular motion

Survey
yes no Was this document useful for you?
   Thank you for your participation!

* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project

Document related concepts

Derivations of the Lorentz transformations wikipedia , lookup

Relativistic mechanics wikipedia , lookup

N-body problem wikipedia , lookup

Coriolis force wikipedia , lookup

Classical mechanics wikipedia , lookup

Center of mass wikipedia , lookup

Modified Newtonian dynamics wikipedia , lookup

Force wikipedia , lookup

Brownian motion wikipedia , lookup

Jerk (physics) wikipedia , lookup

Fictitious force wikipedia , lookup

Torque wikipedia , lookup

Mass versus weight wikipedia , lookup

Newton's theorem of revolving orbits wikipedia , lookup

Kinematics wikipedia , lookup

Centrifugal force wikipedia , lookup

Rotational spectroscopy wikipedia , lookup

Rigid body dynamics wikipedia , lookup

Classical central-force problem wikipedia , lookup

Hunting oscillation wikipedia , lookup

Equations of motion wikipedia , lookup

Seismometer wikipedia , lookup

Newton's laws of motion wikipedia , lookup

Inertia wikipedia , lookup

Centripetal force wikipedia , lookup

Transcript
CHAPTER III.
MOTIONS IN PLANE OR SPACE
- more frequent than one-dimensional motion
- two or three dimensional motions can be divided
into separate motions in each dimension  we can
apply the laws developed for one-dimension to
many common motions in space or plane
Circular motion
Examples: motion of planets, Moon around Earth,
motion of car around a circular track, a point on a
wheel etc…..
- two-dimensional motion (motion in a plane)
- a force is necessary to keep an object moving
along a circular path even when speed is constant
(different from the one dimensional case)
- this force acts on the body making the circular
motion and it is directed toward the center of the
circle
- called: centripetal force (center-seeking force)
- the presence of the centripetal force for circular
motion is in agreement both with the first and
second law of Newton!!!
-without centripetal force the motion would
be in a straight line
-although speed is constant the velocity
vector is not!
acceleration during
motion
 circular

- since F  0  a  0
 V V
-a
t t





- V  V , but V  V  a  0

- for t  t 0 a is pointing towards
the center of the circle


Difference of two
 vectors
  A and
 B
A  B  A  ( B)

(adding the inverse B )
f
i
f
f
i
f
i
f
i
i
Acceleration during circular motion: centripetal


F
acceleration: a  a ( F  F ) ; a 
;
m
2
Experiments suggest: Fc~v ; Fc~m ; Fc~1/r
(v the speed of the object, m the mass, and r the
radius of the circle)
mV
F 
r
V
a 
r
Centripetal forces when driving:
-must be present when taking a turn
-usually provided by static friction forces
-tilting or banking the road is another way
c
c
2
c
2
c
c
c
c
c
Projectile motion
- the motion of on object launched near the surface
of the Earth  free motion through the air under
the action of gravity alone
Examples: kicked footballs, speeding
bullets, flight of a golf ball,
athletes doing long or high jumps
- combination of two one-dimensional motions
- we ignore air resistance
vertical direction: free fall, motion with constant
acceleration ; a=g=9.81 m/s2 ; V  V sin( )
1
V V  gt ; y  V t  gt
2
horizontal direction: motion with no acceleration,
constant speed; a=0 ; V  V cos( )
V V ; x V t;
- the motions in horizontal and vertical directions
are independent from each other !
Y0
2
y
y0
y0
X0
X
Vy0
X0
V0
Vx0
y
x0
x
0
0
Motion of extended objects
(extendednot point-like)
- motion is a combination of translational and
rotational motions
important new concept: center of mass
- the point where the weight acts
- for a point-like object  the point characterizing
the object
- for a regularly shaped object the geometric
center of the object
- for an irregularly shaped object
-hang the object from different points
-construct the vertical lines starting from
the support point
-intersection of these lines  center of mass
- center of mass can be in a point where there is no
matter
- motion of bodies can be understood as a
combination of a translational motion of it’s center
of mass and a rotational motion around the center
of mass
- translational motion described as we did for pointlike bodies
- rotational motion ??
Rotational motion
- laws for rotational motion have many analogies
with translational motion
- distance traveled  angles rotated or revolutions
(units: degrees
or no units)
- speed  rotational speed:
1. angular rotations/time (units: degrees/s)
2. revolutions/time
units: rotations/s (rps) rotations/minute (rpm)
- acceleration  rotational acceleration
(measures the rate at which rotational speed
changes)
(units: degrees/s2 or rotations/s2)
- force  torque
-is governing how the rotational motion changes
-torque depends on the force acting + the
direction and location of the force relative to the
rotational axes : T  F  r  sin( )
(r: the distance from the axes,  the angle
between F and r)
-when F is perpendicular to r  T=F.r
-units for torque: N.m
-condition to change rotational speed is to have
an unbalanced torque!
-condition to have no rotation no net torque
- mass  rotational inertia
-characterizes the inertia against rotations
-depends on the chosen axes
-changing the arrangement of the matter around
the rotational axes result in different resistance
against rotation
-depends on the mass of the body, and on how
far this mass is situated relative to the rotational
axes
-as the distance of the matter relative to the
rotational axes increases, the rotational inertia
increases
-as the rotational inertia is bigger, changing the
rotational motion is harder
Home-work assignments:
71/1-6; 72/9-10; 72/15; 73/22-24; 73/26-28
76/1-8; 76/11-13; 76/15-16