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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. Any vector can be expressed as the sum of two mutually perpendicular component vectors. Usually - but not always - these components are multiples of the basis vectors - and ; that is - vectors along the x-axis and y-axis. We define these two vectors
Focal point
Minima
Component
Radian
2. The separation of different color light via refraction.
Calorie
Node
Dispersion
Vector
3. The amount of error that's possible in a given measurement.
Margin of error
Heat transfer
Meson
Coefficient of linear expansion
4. For two given media - the smallest angle of incidence at which total internal reflection occurs.
Critical angle
Angular velocity
Diffraction grating
Inelastic collision
5. The number of hydrogen atoms in one gram of hydrogen - equal to . When counting the number of molecules in a gas - it is often convenient to count them in moles.
Latent heat of vaporization
Axis of rotation
Mole
Radioactivity
6. A vector quantity - - that reflects the change of angular displacement with time - and is typically given in units of rad/s. To find the direction of the angular velocity vector - take your right hand and curl your fingers along the particle or body
Beta decay
Angular velocity
Thermal equilibrium
Spring constant
7. To every action - there is an equal and opposite reaction. If an object A exerts a force on another object B - B will exert on A a force equal in magnitude and opposite in direction to the force exerted by A.
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8. Relates the angle of incidence to the angle of refraction: .
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9. A scale for measuring temperature - defined such that 0K is the lowest theoretical temperature a material can have. 273K = 0ºC.
Kelvin
Scalar
Work
Spring
10. The index of refraction n = c/v of a substance characterizes the speed of light in that substance - v. It also characterizes - by way of Snell's Law - the angle at which light refracts in that substance.
Displacement
Concave mirror
Index of refraction
Kinematic equations
11. A device that breaks incoming light down into spectral rays - so that one can see the exact wavelength constituents of the light.
Tail
Spectroscope
Weight
Loudness
12. An object cannot be cooled to absolute zero.
Third Law of Thermodynamics
Polarization
Pitch
Melting point
13. A coefficient that tells how much a material will expand or contract lengthwise when it is heated or cooled.
Coefficient of linear expansion
Deposition
Heat
Heat transfer
14. A unit vector is a vector with length 1.
De Broglie wavelength
Unit vector
Spring
Beta particle
15. The force transmitted along a rope or cable.
Critical angle
Meson
Reflected ray
Tension force
16. 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.
Nuclear fusion
Calorie
Rigid body
Alpha decay
17. The sum of a system's potential and kinetic energy. In many systems - including projectiles - pulleys - pendulums - and motion on frictionless surfaces - mechanical energy is conserved. One important type of problem in which mechanical energy is not
Neutron number
Mechanical energy
Spring constant
Constant of proportionality
18. The mass difference between a nucleus and the sum of the masses of the constituent protons and neutrons.
Mass defect
Wavelength
Incident ray
Spring constant
19. A vector quantity defined as the rate of change of the displacement vector with time. It is to be contrasted with speed - which is a scalar quantity for which no direction is specified.
Axis of rotation
Velocity
Thermal energy
Kepler's First Law
20. A form of radioactivity where an excited atom releases a photon of gamma radiation - thereby returning to a lower energy state. The atomic structure itself does not change in the course of gamma radiation.
Gamma decay
Convex lens
Fundamental
Specific heat
21. The distance between the focal point and the vertex of a mirror or lens. For concave mirrors and convex lenses - this number is positive. For convex mirrors and concave lenses - this number is negative.
Rigid body
Focal length
Electron
Alpha particle
22. A constant - - not to be confused with wavelength - that defines the speed at which a radioactive element undergoes decay. The greater is - the faster the element decays.
Decay constant
Work-energy theorem
Normal
Simple harmonic oscillator
23. The net change - - in a point's angular position - . It is a scalar quantity.
Equilibrium position
Angular displacement
Conservation of Angular Momentum
Entropy
24. The bending of light as it passes from one medium to another. Light refracts toward the normal when going from a less dense medium into a denser medium and away from the normal when going from a denser medium into a less dense medium.
Uniform circular motion
Calorie
Refraction
Component
25. A pendulum consists of a bob connected to a rod or rope. At small angles - a pendulum's motion approximates simple harmonic motion as it swings back and forth without friction.
Atomic number
Beta decay
Pendulum
Induced current
26. A collision in which the colliding particles stick together.
Completely inelastic collision
Component
Calorie
Focal length
27. The tendency of an object to remain at a constant velocity - or its resistance to being accelerated. Newton's First Law is alternatively called the Law of Inertia because it describes this tendency.
Inertia
Weber
Kepler's First Law
Thermal equilibrium
28. 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
Angular acceleration
Nuclear fission
Elastic collision
Static friction
29. 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.
Latent heat of vaporization
Cross product
Velocity
Diffraction
30. When a light ray strikes a surface - the angle of incidence is the angle between the incident ray and the normal.
Component
Magnitude
Angle of incidence
Amplitude
31. Light such that all of the associated waves have the same wavelength and are in phase.
Transverse waves
Coherent light
Right-hand rule
Diffraction grating
32. The motion of a body in a circular path with constant speed.
Uniform circular motion
Angular period
Maxima
Simple harmonic oscillator
33. A transfer of thermal energy. We don't speak about systems "having" heat - but about their "transferring" heat - much in the way that dynamical systems don't "have" work - but rather "do" work.
Heat
Kinetic friction
Planck's constant
Harmonic series
34. The property of a vector that distinguishes it from a scalar: while scalars have only a magnitude - vectors have both a magnitude and a direction. When graphing vectors in the xy-coordinate space - direction is usually given by the angle measured cou
Melting point
Dispersion
Direction
Inversely proportional
35. A property of a metal - the minimum frequency of electromagnetic radiation that is necessary to release photoelectrons from that metal.
Static friction
Radioactive decay
Pendulum
Threshold frequency
36. The stable position of a system where the net force acting on the object is zero.
Gravitational constant
Virtual image
Electronvolt
Equilibrium position
37. 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.
Pendulum
Rutherford nuclear model
Thermal energy
Law of reflection
38. An almost massless particle of neutral charge that is released along with a beta particle in beta decay.
Kepler's First Law
Magnitude
Neutrino
Destructive interference
39. The emf created by the motion of a charge through a magnetic field.
Rarefaction
Motional emf
Wavelength
Isotope
40. Heat transfer by molecular collisions.
Conduction
Impulse
Moment of inertia
Hooke's Law
41. 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.
Weightlessness
Mass
Amplitude
Motional emf
42. A frequency - f - defined as the number of revolutions a rigid body makes in a given time interval. It is a scalar quantity commonly denoted in units of Hertz (Hz) or s-1.
Kepler's Third Law
Angular frequency
Elastic collision
Mass defect
43. In an interference or diffraction pattern - the places where there is the most light.
Maxima
Newton's Second Law
Doppler shift
Conduction
44. A transfer of thermal energy from one system to another.
Kinetic theory of gases
Universal gas constant
Heat transfer
Coherent light
45. An electromagnetic wave of very high frequency.
Gamma ray
Neutrino
Newton's Second Law
Specific heat
46. 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.
Vertex
Reflect
Elastic collision
Uncertainty principle
47. The square of the amplitude of a sound wave is called the sound's loudness - or volume.
Normal force
Ideal gas law
Loudness
Atomic number
48. A form of radioactive decay where a heavy element emits an alpha particle and some energy - thus transforming into a lighter - more stable - element.
Inertial reference frame
Electron
Weak nuclear force
Alpha decay
49. 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.
Polarization
Weight
Instantaneous velocity
Strong nuclear force
50. The path of each planet around the sun is an ellipse with the sun at one focus.
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