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Test your basic knowledge |
SAT Subject Test: hysics
Start Test
Study First
Subjects
:
sat
,
science
,
physics
Instructions:
Answer 50 questions in 15 minutes.
If you are not ready to take this test, you can
study here
.
Match each statement with the correct term.
Don't refresh. All questions and answers are randomly picked and ordered every time you load a test.
This is a study tool. The 3 wrong answers for each question are randomly chosen from answers to other questions. So, you might find at times the answers obvious, but you will see it re-enforces your understanding as you take the test each time.
1. Done when energy is transferred by a force. The work done by a force F in displacing an object by s is W = F · s.
Weak nuclear force
Radioactivity
Work
Electromagnetic wave
2. The process by which unstable nuclei spontaneously release particles and/or energy so as to come to a more stable arrangement. The most common forms of radioactive decay are alpha decay - beta decay - and gamma decay.
Motional emf
Radioactive decay
Threshold frequency
Alpha decay
3. A collision in which both kinetic energy and momentum are conserved.
Reflect
Boyle's Law
Real image
Elastic collision
4. The cancellation of one wave by another wave that is exactly out of phase with the first. Despite the dramatic name of this phenomenon - nothing is "destroyed" by this interference—the two waves emerge intact once they have passed each other.
Work function
Oscillation
Destructive interference
Mass number
5. A collision in which momentum is conserved but kinetic energy is not.
Heat transfer
Scalar
Third Law of Thermodynamics
Inelastic collision
6. An image created by a mirror or lens in such a way that light does not actually come from where the image appears to be.
Zeroth Law of Thermodynamics
Virtual image
Weak nuclear force
Fundamental
7. A neutrally charged particle that - along with protons - constitutes the nucleus of an atom.
Weight
Neutron
Energy
Pendulum
8. The number of cycles executed by a system in one second. Frequency is the inverse of period - f = 1/T. Frequency is measured in hertz - Hz.
Frequency
Medium
Free
Sound
9. The temperature at which a material will change phase from solid to liquid or liquid to solid.
Angular momentum
Boiling point
Antinode
Melting point
10. The point of a mirror or lens where all light that runs parallel to the principal axis will be focused. Concave mirrors and convex lenses are designed to focus light into the focal point. Convex mirrors and concave lenses focus light away from the fo
Focal point
Latent heat of fusion
Energy
Amplitude
11. In an interference or diffraction pattern - the places where there is the least light.
Legs
Minima
Scalar
Atom
12. A conserved scalar quantity associated with the state or condition of an object or system of objects. We can roughly define energy as the capacity for an object or system to do work. There are many different types of energy - such as kinetic energy -
Translational kinetic energy
Threshold frequency
Lenz's Law
Energy
13. Energy associated with the state of motion. The translational kinetic energy of an object is given by the equation .
Acceleration
Traveling waves
Coefficient of kinetic friction
Kinetic energy
14. For a reflected light ray - . In other words - a ray of light reflects of a surface in the same plane as the incident ray and the normal - and at an angle to the normal that is equal to the angle between the incident ray and the normal.
Dispersion
Simple harmonic oscillator
Law of reflection
Phase change
15. Heat transfer by molecular collisions.
Mechanical energy
Pulley
Conduction
Motional emf
16. A unit of measurement for energy on atomic levels. 1 eV = J.
Equilibrium
Pendulum
Threshold frequency
Electronvolt
17. The disorder of a system.
Gamma ray
Ideal gas law
Decibel
Entropy
18. For a gas held at a constant temperature - pressure and volume are inversely proportional.
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19. The amount of energy that metal must absorb before it can release a photoelectron from the metal.
Work function
Work
Motional emf
Energy
20. The force necessary to maintain a body in uniform circular motion. This force is always directed radially toward the center of the circle.
Spectroscope
Force
Free
Centripetal force
21. A pulley is a simple machine that consists of a rope that slides around a disk or block.
Tail
Reflect
Nucleus
Pulley
22. If two systems - A and B - are in thermal equilibrium and if B and C are also in thermal equilibrium - then systems A and C are necessarily in thermal equilibrium.
Kepler's First Law
Zeroth Law of Thermodynamics
De Broglie wavelength
Tension force
23. In an interference or diffraction pattern - the places where there is the most light.
Maxima
Latent heat of fusion
Dynamics
Principal axis
24. When objects collide - each object feels a force for a short amount of time. This force imparts an impulse - or changes the momentum of each of the colliding objects. The momentum of a system is conserved in all kinds of collisions. Kinetic energy is
Critical angle
Collision
Lenz's Law
Electromagnetic spectrum
25. The ratio of the size of the image produced by a mirror or lens to the size of the original object. This number is negative if the image is upside-down.
Node
Center of mass
Refracted ray
Magnification
26. Energy cannot be made or destroyed; energy can only be changed from one place to another or from one form to another.
Kepler's Second Law
Gamma decay
Law of conservation of energy
Pressure
27. The points midway between nodes on a standing wave - where the oscillations are largest.
Antinode
Legs
Tangent
Destructive interference
28. A back-and-forth movement about an equilibrium position. Springs - pendulums - and other oscillators experience harmonic motion.
Diffraction
Oscillation
Convection
Neutrino
29. A form of vector multiplication - where two vectors are multiplied to produce a third vector. The cross product of two vectors - A and B - separated by an angle - - is - where is a unit vector perpendicular to both A and B. To deine which direction
Gravitational constant
Normal
Cross product
Phase
30. A quantity that possesses a magnitude but not a direction. Mass and length are common examples.
Electromagnetic wave
Wave
Tension force
Scalar
31. The time - T - required for a rigid body to complete one revolution.
Angular period
Mechanical energy
Universal gas constant
Energy
32. The net change - - in a point's angular position - . It is a scalar quantity.
Longitudinal waves
Decay constant
Angular displacement
Uncertainty principle
33. Essentially a restatement of energy conservation - it states that the change in the internal energy of a system is equal to the heat added plus the work done on the system.
First Law of Thermodynamics
Pressure
Photon
Longitudinal waves
34. Two quantities are directly proportional if an increase in one results in a proportional increase in the other - and a decrease in one results in a proportional decrease in the other. In a formula defining a certain quantity - those quantities to whi
Michelson-Morley experiment
Compression
Gamma decay
Directly proportional
35. The state of a nonrotating object upon whom the net torque acting is zero.
Node
Basis vector
Equilibrium
Potential energy
36. The center of an atom - where the protons and neutrons reside. Electrons then orbit this nucleus.
Sine
Nucleus
Elastic collision
Kepler's Third Law
37. The effect of force on rotational motion.
Velocity
Torque
Faraday's Law
Coefficient of kinetic friction
38. An object that retains its overall shape - meaning that the particles that make up the rigid body stay in the same position relative to one another.
Rigid body
Weight
Mass defect
Dynamics
39. Another word for the frequency of a sound wave.
Electric generator
Electromagnetic induction
Pitch
Angle of refraction
40. The process by which a solid turns directly into gas - because it cannot exist as a liquid at a certain pressure.
Pendulum
Kelvin
Electronvolt
Sublimation
41. The velocity at any given instant in time. To be contrasted with average velocity - which is a measure of the change in displacement over a given time interval.
Scalar
Instantaneous velocity
Neutrino
Calorie
42. An experiment in 1879 that showed that the speed of light is constant to all observers. Einstein used the results of this experiment as support for his theory of special relativity.
Scalar
Dynamics
Heat engine
Michelson-Morley experiment
43. An area of high air pressure that acts as the wave trough for sound waves. The spacing between successive rarefactions is the wavelength of sound - and the number of successive areas of rarefaction that arrive at the ear per second is the frequency -
Rarefaction
Latent heat of vaporization
Planck's constant
Traveling waves
44. Two quantities are inversely proportional if an increase in one results in a proportional decrease in the other - and a decrease in one results in a proportional increase in the other. In a formula defining a certain quantity - those quantities to wh
Inversely proportional
Photon
Amplitude
Alpha decay
45. Life- The amount of time it takes for one-half of a radioactive sample to decay.
Cross product
Sound
Work-energy theorem
Half
46. The unit for measuring pressure. One Pascal is equal to one Newton per meter squared - 1 Pa = 1 N/m2.
Pascals
Pulley
Equilibrium position
Ideal gas law
47. A device that breaks incoming light down into spectral rays - so that one can see the exact wavelength constituents of the light.
Electronvolt
Spectroscope
Pulley
Deposition
48. A principle derived by Werner Heisenberg in 1927 that tells us that we can never know both the position and the momentum of a particle at any given time.
Beta particle
Translational kinetic energy
Basis vector
Uncertainty principle
49. The coefficient of kinetic friction - - for two materials is the constant of proportionality between the normal force and the force of kinetic friction. It is always a number between zero and one.
Reflect
Coefficient of kinetic friction
Fundamental
Index of refraction
50. The energy of a particle moving in space. It is defined in s of a particle's mass - m - and velocity - v - as (1/2)mv2.
Spring
Translational kinetic energy
Law of conservation of energy
Axis of rotation