Theoretical material for the lesson, definitions for concepts
quantity |
definition |
Mechanics |
|
displacement, s [m] |
displacement of a particle is the length and direction of a line drawn to the particle from the origin |
velocity, v [m s-1] |
rate of change of position with time |
speed, v [m s-1] |
rate of distance travelled along a path |
acceleration, a [m s-2] |
rate of change of velocity with time |
change in velocity / rate of change of velocity; per unit time / with time; |
|
(translational) equilibrium |
a body in equilibrium has zero resultant force acting on it and therefore has zero acceleration |
sum of the (net) forces acting is zero; |
|
weight, W [N] |
the weight of an object is the gravitational attraction of a massive body (eg Earth) for that object |
conserved |
any quantity which is conserved maintains a constant total value
|
conservation of energy |
appropriate statement of principle of conservation of energy; e.g. “Energy can not be created or destroyed, it just changes form.” |
Newton’s 1st law |
a body will remain at constant velocity unless a net force acts on it |
Newton’s 2nd law |
the rate of change of momentum of a body is proportional to the net force acting on it This simplifies to |
Newton’s 3rd law |
when two bodies A and B interact the force that A exerts on B is equal and opposite to the force that B exerts on A; or when a force acts on a body, an equal an opposite force acts on another body somewhere in the universe; |
linear momentum, p [kg m s-1] |
the product of a body’s mass and its velocity (therefore momentum is a vector with the same direction as the velocity) |
momentum is mass x velocity; allow an equation, with symbols explained. |
|
momentum is mass × velocity; |
|
impulse, Δp [kg m s-1] or [N s] |
the change in momentum of a body, |
impulse is force x time or change in momentum; |
|
(impulse =) force x time for which force acts; |
|
impulse is force × time / change in momentum; |
|
law of conservation of momentum |
if the total external force acting upon a system is zero / for an isolated system; the momentum of the system is constant; |
(vector) sum/total of momenta is constant; for isolated system; |
|
if the net external force acting on a system is zero; then the total momentum of the system is constant (or in any one direction, is constant); |
|
if the total (or net) external force acting on a system is zero / for an isolated system; the momentum of the system is constant/momentum before collision equals momentum after collision; |
|
if the net external force acting on a system is zero / for an isolated system of interacting particles; the momentum of the system is constant / momentum before collision equals momentum after collision; |
|
for isolated/closed system; total momentum remains constant; |
|
the momentum of a system (of interacting particles) is constant; if no external force acts on system / net force on system is zero / isolated system; |
|
work, W [J] |
force × distance (moved) in the direction of the force |
power |
the rate of working / work time; If equation is given, then symbols must be defined. |
the
rate of working / Ratio or rate must be clear. |
|
kinetic energy, EK [J] |
the energy associated with a body because of its motion |
potential energy, EP [J] |
the energy possessed by a system due to the relative positions of its component parts (ie due to the forces between the component parts) |
elastic collision |
a collision in which the total KE is conserved |
(a collision in which) kinetic energy is not lost / kinetic energy is conserved; |
|
inelastic collision |
a collision in which some kinetic energy is transferred to other forms (eg internal energy, sound), therefore the total KE is less after the collision than before |
gravitational field strength g [N kg-1] |
force exerted per unit mass; on a small / point mass; |
the force exerted per unit mass; on a point mass; |
|
the force per unit mass; exerted on a point/small mass; |
|
test mass |
a small mass which has a negligible effect on the gravitational field in which it is placed |
gravitational potential energy |
the work done to move a body from infinity to a point in a gravitational field |
gravitational potential U [J kg-1] |
the work done per kilogram to move a body from infinity to a point in a gravitational field |
the work done per unit mass; in bringing a small/point mass; from infinity to the point (in the gravitational field); |
|
the work done per unit mass; in bringing a small/point mass from infinity to a point (in the gravitational field); |
|
escape speed |
speed of object at Earth’s surface; so that it will escape from the gravitational field / travel to infinity; |
speed (of object) at surface (of planet) / specified starting point; so that object may move to infinity / escape gravitational field of planet; |
Additional guidelines for organizing a lesson
Students can deduce topic of the lessen and objectives, for clarification you can show topic and the learning objectives on the presentation.
Then Subject-specific vocabulary & terminology will be presented to the students and their activities during the research work will be explained.
Then teacher will give the worksheet on the concepts studied previously. Students attempt the questions in groups as they engage in discussion. The teacher helps the learners with difficulties in answering the questions.
Reinforce the LO’s: answer any questions students may have/clarify understanding. Students reflect on their learning.
At the end of the lesson teacher will give homework.
Additional multilevel (on differentiation) tasks
Each chapter has extra tasks which you would use for high level students.
Recommendations for formative assessment
1) Use the answers provided to assess students’ understanding and the manner of application of the all terms concept knowledge
2) Provide a general feedback for every given point (pay attention to give a fully explained feedback to the points that were not given)
3) You can change the numbers in calculations according to the student’s ability
Answers, criteria for assignments, additional materials for the lesson
Kinematics:
1 a. A, B, C, E, G, I, J 2b. B,C,I,G 2c. NONE 2d. H, 2e. 0.33 m/s 2f. 5 m/s 2g. -5.0 m/s (west)
2h.
Dynamics:
Answers:
1. The hammer will not fall to the Earth. The astronaut, shuttle, and hammer are all in free fall around the Earth (in an orbit), so the hammer has the same acceleration as the astronaut and does not move away from him.
2. The acceleration due to
gravity is With
and
3.
The gravitational
potential energy is negative because we choose to place the zero point of
potential energy at infinity With this
choice, the gravitational potential energy is negative because the conservative
force of gravity is attractive. The two masses will gain kinetic energy as they
approach each other.
Momentum:
1. (c) 10 rad/s
2. (e) 800 kg × m2/s
3. It points into the paper.
Mechanics of liquids and gases:
P2 = 0
Материалы на данной страницы взяты из открытых источников либо размещены пользователем в соответствии с договором-офертой сайта. Вы можете сообщить о нарушении.