| Explanation | Law/principle | % Correct |
|---|---|---|
| The upthrust experienced by an object is equal and opposite to the weight of the displaced fluid. | Archimedes Principle | 0%
|
| The total charge remains constant over time. | Conservation of Charge Principle | 0%
|
| Energy can't be created or destroyed, only transferred from one form to another. | Conservation of Energy Principle | 0%
|
| The vector sum of the moments of bodies in a system stays constant even if forces act between the bodies, provided there is no external resultant force. | Conservation of Momentum Principle | 0%
|
| The force between two point charges was proportional to the magnitude of the charges and inversely proportional to the square of the distance between them. | Coulomb's Law | 0%
|
| Current from a source is equal to the sum of the currents in the separate branches of a parallel circuit. | Current Law | 0%
|
| A quantity decreases at a rate proportional to its current value, resulting in a consistent percentage reduction over time rather than a fixed amount. | Exponential Law of Decay | 0%
|
| The emf induced is equal to the rate of change of flux linkage. | Faraday's Law | 0%
|
| Energy can't be created or destroyed, only converted between forms like heat, work and internal energy. | First Law of Thermodynamics | 0%
|
| Defines the direction of a force acting on a current carrying conductor in a magnetic field, thumb is force/motion, forefinger is magnetic field and second finger is current. | Fleming's Left Hand Rule | 0%
|
| Tension in a spring or wire is proportional to its extension from its natural length if the extension isn't too large | Hooke's Law | 0%
|
| The further away a galaxy is, the greater the redshift is. | Hubble's Law | 0%
|
| The intensity of radiation from a star is inversely proportional to the distance from the star squared. | Inverse Square Law | 0%
|
| Each planet moves in an ellipse with the sun at one focus. | Kepler's First Law of Thermodynamics | 0%
|
| The line joining a planet to the centre of the sun sweeps out equal areas in intervals of time. | Kepler's Second Law of Thermodynamics | 0%
|
| The direction of the current resulting from an induced emf is such as to oppose the change in flux linkage. | Lenz's Law | 0%
|
| The force between two masses is directly proportional to the product of the masses and inversely proportional to the square of the distance between them. | Newton's Law of Gravitation | 0%
|
| The rate of change of momentum of an object is proportional to the resultant force acting on it and takes place in the direction of that force. | Newton's Second Law | 0%
|
| If body A exerts a force on body B, then body B exerts an equal and opposite force on body A. | Newton's Third Law | 0%
|
| The sum of the anticlockwise moments about a point is equal to the sum of the clockwise moments about that same point. | Principle of Moments | 0%
|
| If waves from two sources occupy the same region, then the total displacement at any one point is the vector sum of their individual displacements at that point. | Principle of Superposition | 0%
|
| When light moves from a less dense to a denser medium, it bends toward the normal line. | Snell's Law | 0%
|
| The total energy radiated per unit surface area of a black body is directly proportional to the fourth power of its absolute (kelvin) temperature. | Stefan's Law | 0%
|
| Sum of the potential differences across the components in a series circuit is equal ti the potential difference across the supply. | Voltage Law | 0%
|
| The wavelength of peak emission from a black body is inversely proportional to the absolute (kelvin) temperature. | Wien's Law | 0%
|