Definitions of everything Flashcards
Includes most (not all) definitions in boxes.
random error vs systematic error
random error: when the measured readings are scattered about the true reading with no fixed pattern
systematic error: when the measured readings are consistently larger or consistently smaller than the true reading
accuracy vs precision
accuracy: how close the measured reading is to the true value
precision of a set of readings (diff from precision of instrument): how close the measured readings are to each other
Newton’s Third Law of Motion
when body A exerts a force on body B, body B exerts on body A a force of the same type that is equal in magnitude and opposite in direction.
Newton’s First Law of Motion
an object continues at rest or with constant velocity unless acted upon by a resultant force
The mass of a body
property of a body which resists change in motion
The weight of a body
force acting on the body due to a gravitational field
Newton’s Second Law of Motion
rate of change of momentum of a body is
[magnitude] directly proportional to the resultant force acting on it and
[direction] in the direction of the resultant force
The Principle of Conservation of Linear Momentum states that the
total linear momentum of an isolated system of interacting bodies before and after collision remains constant if no net external force acts on the system
The centre of gravity
the single point where the weight of a body may be considered to act
Hooke’s Law states that
the change in length of a material is directly proportional to the force applied on it when the limit of proportionality is not exceeded.
Upthrust is
equal in magnitude and opposite in direction to the weight of fluid displaced by submerged or floating object
Explain the origin of upthrust
pressure exerted by water increases with depth
pressure on bottom surface area of cylinder
greater than pressure on top surface area of cylinder
upwards force on bottom surface larger
than downwards force on top surface
net upwards force is upthrust
Principle of moments
For a body in rotational equilibrium, sum of clockwise moments about any point is equal to sum of anti-clockwise moments about the same point
a body is in rotational equilibrium when there is:
a body is in translational equilibrium when there is:
a body is in equilibrium when:
body is in translational equilibrium when there is
[magnitude] no resultant force
[direction] in any direction
a body is in rotational equilibrium
when there is
[magnitude] no resultant torque
[direction] about any point
a body is in equilibrium when
there is no resultant force in any direction and
there is no resultant torque about any point
work done by a force is
the product of the force and the displacement in the direction of the force
one radian is the
angle subtended at the centre of a circle by an arc length that is equal to the radius
angular velocity ω (NOT THE SAME AS ANGULAR FREQUENCY IN OSCILLATIONS) is
the rate of angular displacement swept out by radius
a gravitational field is
a region of space where a mass experiences a gravitational force
Newton’s law of gravitation states that the
[type of force] gravitational force of attraction between two point masses
[magnitude] is directly proportional to the product of the masses and
inversely proportional to the square of separation between the masses
Advantage of geostationary satellites? What are they used for?
Geostationary satellites allow transmission of signals between two regions at all times because the satellite will remain within “line-of-sight” of ground-based transmission and reception equipment.
They are useful for constant monitoring of weather especially in the equatorial region.
a geostationary satellite must:
have a period of 24 hour
be in circular orbit at a particular radius
orbit directly above Equator
move from west to east along same orbital axis as Earth’s rotation
gravitational field strength g at a point in the field is the
[type of force] gravitational force of attraction
[ratio] per unit mass
[specifics] by a small test mass
placed at that point
gravitational potential φ at a point in the field is the
[process] work done
[ratio] per unit mass
[specifics] in bringing a small test mass
from infinity to that point
an oscillation is
a complete to-and-fro motion between two limits
free oscillations are
oscillations with constant amplitude without energy loss or gain as there is no external force acting on the system