Unit Overview – Force and Motion
The big picture stuff:
Students have been exploring push/pull relationships, throughout their K-8 years, but in high school, students begin using the language of mathematics as evidence from experimentation to support concepts that have been developing for some time. Students go beyond, “will this keep moving” or “will this collide” to “why does this object keep moving and when will it stop?” Understanding Newton’s 3rd law, as relating forces to the motion of objects, helps students frame why some objects move and others don’t in given situations. The NGSS asks students to compare movement of objects as related to gravitational pull to magnetic and electrical forces. The exploration of electromagnetism will occur in a different unit.
Next Generation Science Standards – High School (NGSS-HS):
Core ideas: For any pair of interacting objects, the force exerted by the first object on the second object is equal in strength to the force that the second object exerts on the first, but in the opposite direction.
Examples: the impact of collisions between two cars, between a car and stationary objects, and between a meteor and a space vehicle; limited to vertical or horizontal interactions in one dimension
Core ideas: The motion of an object is determined by the sum of the forces acting on it; if the total force on the object is not zero, its motion will change. The greater the mass of the object, the greater the force needed to achieve the same change in motion. For any given object, a larger force causes a larger change in motion. All positions of objects and the directions of forces and motions must be described in an artibrarily chosen reference frame and arbitrarily chosen units of size.
Emphasize: balanced (Newton’s First Law) and unbalanced forces in a system, qualitative comparisons of forces, mass and changes in motion (Newton’s Second Law), frame of reference, and specification of units. Focus on forces and changes in motion in one-dimension in an inertial reference frame, and to change in one variable at a time.
Core Ideas: Gravitational forces are always attractive. There is a gravitational force between any two masses, but it is very small except when one or both of the objects have large mass (e.g., Earth and the sun)
Examples: data generated from simulations or digital tools; and charts displaying mass, strength of interaction, distance from the Sun, and orbital periods of objects within the solar system.
California Science Standards - Physics:
1a. Students know how to solve problems that involve constant speed and average speed.
1b. Students know that when forces are balanced, no acceleration occurs: thus an object continues to move at constant speed or stays at rest.
1c. Students know how to apply the law F=ma to solve one dimensional motion problems that involve constant forces.
1d. Students know that when one object exerts a force on a second object, the second object will always exert a force of equal magnitude and in the opposite direction.
1e. Students know the relationship between the universal law of gravitation and the effect of gravity on an object at the surface of the Earth
Investigation and Experimentation Standards:
a. Select and use appropriate tools and technology (such as computer-linked probes, spreadsheets, and graphing calculators) to perform tests, collect data, analyze relationships, and display data.
b. Identify and communicate sources of unavoidable experimental error.
c. Identify possible reasons for inconsistent results, such as sources of error or uncontrolled conditions.
d. Formulate explanations by using logic and evidence.
j. Recognize the issues of statistical variability and the need for controlled tests.