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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. In the Bohr model of the atom - the state in which an electron has the least energy and orbits closest to the nucleus.
Collision
Destructive interference
Reflection
Ground state
2. A transverse traveling wave created by the oscillations of an electric field and a magnetic field. Electromagnetic waves travel at the speed of light - m/s. Examples include microwaves - X rays - and visible light.
Coefficient of linear expansion
Radian
Electromagnetic wave
Pitch
3. The points of maximum negative displacement along a wave. They are the opposite of wave crests.
Trough
Inertial reference frame
Kepler's First Law
Mole
4. Life- The amount of time it takes for one-half of a radioactive sample to decay.
Isotope
Directly proportional
Half
Neutron
5. The straight line that runs through the focal point and the vertex of a mirror or lens.
Temperature
Moment of inertia
System
Principal axis
6. The angle between a reflected ray and the normal.
Angular displacement
Angle of reflection
Dynamics
Node
7. With spherical mirrors - the radius of the sphere of which the mirror is a part.
Radius of curvature
Kinetic friction
Force
Beta decay
8. Relates the angle of incidence to the angle of refraction: .
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9. The speed at which a wave crest or trough propagates. Note that this is not the speed at which the actual medium (like the stretched string or the air particles) moves.
Alpha decay
Potential energy
Pascals
Wave speed
10. When two waves of slightly different frequencies interfere with one another - they produce a "beating" interference pattern that alternates between constructive (in-phase) and destructive (out-of-phase). In the case of sound waves - this sort of inte
Translational kinetic energy
Celsius
Mass defect
Beats
11. Heat transfer via the mass movement of molecules.
Convection
Heat
Thermal energy
Reflection
12. The energy of the molecules that make up an object. It is related to heat - which is the amount of energy transferred from one object to another object that is a different temperature.
Transverse waves
Thermal energy
Free
Elastic collision
13. A measurement of a body's inertia - or resistance to being accelerated.
Mass
Kinetic theory of gases
Refracted ray
Wave speed
14. A logorithmic unit for measuring the volume of sound - which is the square of the amplitude of sound waves.
Angular displacement
Latent heat of vaporization
Beats
Decibel
15. A model for the atom developed in 1913 by Niels Bohr. According to this model - the electrons orbiting a nucleus can only orbit at certain particular radii. Excited electrons may jump to a more distant radii and then return to their ground state - em
Angular velocity
Center of mass
Diffraction
Bohr atomic model
16. The force between two surfaces moving relative to one another. The frictional force is parallel to the plane of contact between the two objects and in the opposite direction of the sliding object's motion.
Electromagnetic induction
Superposition
Boiling point
Kinetic friction
17. The particles and energy released by the fission or fusion of one atom may trigger the fission or fusion of further atoms. In a chain reaction - fission or fusion is rapidly transferred to a large number of atoms - releasing tremendous amounts of ene
Basis vector
Total internal reflection
Chain reaction
Uniform circular motion
18. The building blocks of all matter - quarks are the constituent parts of protons - neutrons - and mesons.
Quark
Phase change
Dispersion
Maxima
19. 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.
Law of reflection
Hypotenuse
Wave
Torque
20. The series of standing waves supported by a string with both ends tied down. The first member of the series - called the fundamental - has two nodes at the ends and one anti-node in the middle. The higher harmonics are generated by placing an integra
Thermal equilibrium
Harmonic series
Gravitational Potential Energy
Reflect
21. When dealing with reflection or refraction - the incident ray is the ray of light before it strikes the reflecting or refracting surface.
Frequency
Incident ray
Phase change
Cycle
22. If the net torque acting on a rigid body is zero - then the angular momentum of the body is constant or conserved.
Conservation of Angular Momentum
Frictional force
Convex lens
Magnetic flux
23. The mass difference between a nucleus and the sum of the masses of the constituent protons and neutrons.
Pulley
Coefficient of linear expansion
Mass defect
Kinetic energy
24. Body diagram- Illustrates the forces acting on an object - drawn as vectors originating from the center of the object.
Component
Free
Pitch
Weight
25. 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.
Concave lens
Acceleration
Michelson-Morley experiment
Static friction
26. The standing wave with the lowest frequency that is supported by a string with both ends tied down is called the fundamental - or resonance - of the string. The wavelength of the fundamental is twice the length of the string - .
Absolute zero
Fundamental
Concave lens
Kinematics
27. The motion of a body in a circular path with constant speed.
Beta decay
Uniform circular motion
Potential energy
Deposition
28. An experiment by Ernest Rutherford that proved for the first time that atoms have nuclei.
Uniform circular motion
Gold foil experiment
Impulse
Significant digits
29. A quantity that possesses a magnitude but not a direction. Mass and length are common examples.
Scalar
Kepler's Third Law
Boyle's Law
Heat engine
30. 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
Magnification
Orbit
Law of conservation of energy
31. 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
Zeroth Law of Thermodynamics
Concave mirror
Focal point
Inversely proportional
32. A coefficient that tells how much a material will expand or contract lengthwise when it is heated or cooled.
Antinode
Wavelength
Angle of reflection
Coefficient of linear expansion
33. The experience of being in free fall. If you are in a satellite - elevator - or other free-falling object - then you have a weight of zero Newtons relative to that object.
Induced current
Significant digits
Weightlessness
Impulse
34. A nuclear reaction in which a high-energy neutron bombards a heavy - unstable atomic nucleus - causing it to split into two smaller nuclei - and releasing some neutrons and a vast amount of energy at the same time
Velocity
Latent heat of fusion
Convection
Nuclear fission
35. A process that aligns a wave of light to oscillate in one dimension rather than two.
Neutrino
Kinematic equations
Weber
Polarization
36. The amount of heat necessary to transform a liquid at a given temperature into a gas of the same temperature - or the amount of heat needed to be taken away from a gas of a given temperature to transform it into a liquid of the same temperature.
Torque
Polarization
Latent heat of vaporization
Legs
37. 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 -
Momentum
Transverse waves
Rarefaction
Index of refraction
38. The force involved in beta decay that changes a proton to a neutron and releases an electron and a neutrino.
Gravitational constant
Weak nuclear force
Center of mass
Total internal reflection
39. Linear momentum - p - commonly called "momentum" for short - is a vector quantity defined as the product of an object's mass - m - and its velocity - v.
Spectroscope
Thermal energy
Momentum
Spring constant
40. A wave with wave crests that propagate down the length of the medium - in contrast to stationary standing waves. The velocity at which a crest propagates is called the wave speed.
Traveling waves
Longitudinal waves
Newton's Third Law
Distance
41. The unit of magnetic flux - equal to one T · m2.
Spring constant
Law of reflection
Weber
Concave mirror
42. The number of digits that have been accurately measured. When combining several measurements in a formula - the resulting calculation can only have as many significant digits as the measurement that has the smallest number of significant digits.
Angle of reflection
Speed
Significant digits
Longitudinal waves
43. The number - N - of neutrons in an atomic nucleus.
Electron
Neutron number
Thermal equilibrium
Mass number
44. An area of high air pressure that acts as the wave crest for sound waves. The spacing between successive compressions is the wavelength of sound - and the number of successive areas of compression that arrive at the ear per second is the frequency -
Unit vector
Instantaneous velocity
Compression
Momentum
45. The position - of an object according to a co-ordinate system measured in s of the angle of the object from a certain origin axis. Conventionally - this origin axis is the positive x-axis.
Angular position
Deposition
Snell's Law
Centripetal acceleration
46. A vector quantity defined as the rate of change of the velocity vector with time.
Snell's Law
Meson
Centripetal force
Acceleration
47. The time - T - required for a rigid body to complete one revolution.
Instantaneous velocity
Angular period
Photoelectric effect
Kinetic energy
48. States that the net work done on an object is equal to the object's change in kinetic energy.
Work-energy theorem
Magnitude
Kinematic equations
Electromagnetic wave
49. The center of a mirror or lens.
Temperature
Vertex
Compression
Angular acceleration
50. For a heat engine - the ratio of work done by the engine to heat intake. Efficiency is never 100%.
Newton's Third Law
Efficiency
Hooke's Law
Incident ray