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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. The constant of proportionality in Newton's Law of Gravitation. It reflects the proportion of the gravitational force and - the product of two particles' masses divided by the square of the bodies' separation. N · m2/kg2.
Rutherford nuclear model
Gravitational constant
Mass number
Coefficient of static friction
2. There are a few versions of this law. One is that heat flows spontaneously from hot to cold - but not in the reverse direction. Another is that there is no such thing as a 100% efficient heat engine. A third states that the entropy - or disorder - of
Sublimation
Activity
Second Law of Thermodynamics
Cosine
3. For a heat engine - the ratio of work done by the engine to heat intake. Efficiency is never 100%.
Kepler's Third Law
Normal
Efficiency
Kinetic energy
4. 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.
Michelson-Morley experiment
Elastic collision
Charles's Law
Gamma decay
5. 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
Incident ray
Electromagnetic induction
Efficiency
6. Life- The amount of time it takes for one-half of a radioactive sample to decay.
Faraday's Law
Half
Mole
Reflected ray
7. An image created by a mirror or lens in such a way that light does actually come from where the image appears to be. If you place a screen in front of a real image - the image will be projected onto the screen.
Directly proportional
Real image
Normal force
Angular displacement
8. A vector quantity - L - that is the rotational analogue of linear momentum. For a single particle - the angular momentum is the cross product of the particle's displacement from the axis of rotation and the particle's linear momentum - . For a rigid
Internal energy
Electromagnetic induction
Angular momentum
Medium
9. The building blocks of all matter - atoms are made up of a nucleus consisting of protons and neutrons - and a number of electrons that orbit the nucleus. An electrically neutral atom has as many protons as it has electrons.
Coefficient of volume expansion
Kinetic friction
Atom
Angular acceleration
10. The time - T - required for a rigid body to complete one revolution.
Instantaneous velocity
Mass defect
Centripetal acceleration
Angular period
11. 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.
Instantaneous velocity
Angular frequency
Radius of curvature
Inelastic collision
12. 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.
Heat engine
Power
Translational kinetic energy
Rotational kinetic energy
13. The longest side of a right triangle - opposite to the right angle.
Magnification
Hypotenuse
Dynamics
Frictional force
14. The temperature at which a material will change phase from liquid to gas or gas to liquid.
Angular position
Weightlessness
Boiling point
Radiation
15. F = ma. The net force - F - acting on an object causes the object to accelerate - a. The magnitude of the acceleration is directly proportional to the net force on the object and inversely proportional to the mass - m - of the object.
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16. A logorithmic unit for measuring the volume of sound - which is the square of the amplitude of sound waves.
Medium
Decay constant
Decibel
Destructive interference
17. Kinematics is the study and description of the motion of objects.
Kinematics
Magnification
Angular acceleration
Activity
18. 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
Harmonic series
Photon
Concave mirror
Isotope
19. The state of a nonrotating object upon whom the net torque acting is zero.
Equilibrium
Hertz (Hz)
Absolute zero
Transverse waves
20. The amount of heat needed to raise the temperature of one gram of water by one degree Celsius. 1 cal = 4.19 J.
Radiation
Inertia
Calorie
Newton's Third Law
21. Relates the angle of incidence to the angle of refraction: .
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22. A vector quantity - commonly denoted by the vector s - which reflects an object's change in spatial position. The displacement vector points from the object's starting position to the object's current position in space. If an object is moved from poi
Antinode
Radian
Displacement
Newton's Third Law
23. The separation of different color light via refraction.
Transverse waves
Reflect
Dispersion
Lenz's Law
24. The amount heat necessary to cause a substance to undergo a phase transition.
Gamma decay
Latent heat of transformation
Motional emf
Amplitude
25. A coefficient that tells how much the volume of a solid will change when it is heated or cooled.
Rarefaction
Oscillation
Coefficient of volume expansion
Longitudinal waves
26. The amount of heat necessary for a material undergoing sublimation to make a phase change from gas to solid or solid to gas - without a change in temperature.
Radiation
Latent heat of sublimation
Vertex
Sound
27. States that the current induced in a circuit by a change in magnetic flux is in the direction that will oppose that change in flux. Using the right-hand rule - point your thumb in the opposite direction of the change in magnetic flux. The direction y
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28. Waves in which the medium moves in the direction perpendicular to the propagation of the wave. Waves on a stretched string - water waves - and electromagnetic waves are all examples of transverse waves.
Transverse waves
Rigid body
Pascals
Trough
29. The principle by which the displacements from different waves traveling in the same medium add up. Superposition is the basis for interference.
Dynamics
Rarefaction
Superposition
Hooke's Law
30. 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.
Nucleus
Atomic number
Focal length
Radian
31. If a line is drawn from the sun to the planet - then the area swept out by this line in a given time interval is constant.
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32. 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.
Reflect
Convection
Photoelectric effect
Angular position
33. 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 -
Wave speed
Thermal equilibrium
Mass defect
Energy
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
Conservation of Angular Momentum
Directly proportional
Beta particle
Focal length
35. Another word for the frequency of a sound wave.
Fundamental
Pitch
Simple harmonic oscillator
Law of reflection
36. The temperature at which a material will change phase from solid to liquid or liquid to solid.
Melting point
Atomic number
Universal gas constant
Reflect
37. 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.
Spectroscope
Coefficient of static friction
Reflected ray
Magnification
38. In the graphical representation of vectors - the tip of the arrow is the pointy end.
Kepler's Second Law
Lenz's Law
Tip
Inversely proportional
39. The ray of light that is refracted through a surface into a different medium.
Refracted ray
Mass defect
Mass
Virtual image
40. 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 -
Compression
Transformer
Latent heat of vaporization
Wave speed
41. 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.
Magnetic flux
Newton's First Law
Mass defect
Uncertainty principle
42. 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.
Momentum
Cross product
Newton
Pendulum
43. The phenomenon of light bouncing off a surface - such as a mirror.
Heat transfer
Neutron number
Coefficient of linear expansion
Reflection
44. A scalar quantity. If an object is moved from point A to point B in space along path AB - the distance that the object has traveled is the length of the path AB. Distance is to be contrasted with displacement - which is simply a measure of the distan
Newton's First Law
Magnetic flux
Impulse
Distance
45. A wedge or a slide. The dynamics of objects sliding down inclined planes is a popular topic on SAT II Physics.
Newton's Law of Universal Gravitation
Inclined plane
Mole
Beats
46. A force caused by the roughness of two materials in contact - deformations in the materials - and a molecular attraction between the materials. Frictional forces are always parallel to the plane of contact between two surfaces and opposite the direct
Law of conservation of energy
Frictional force
Kepler's Second Law
Restoring force
47. 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
Gravitational Potential Energy
Direction
Nuclear fission
Internal energy
48. 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
Melting point
Virtual image
Beats
Activity
49. The energy associated with the configuration of bodies attracted to each other by the gravitational force. It is a measure of the amount of work necessary to get the two bodies from a chosen point of reference to their present position. This point of
Gravitational Potential Energy
Coefficient of volume expansion
Decay constant
Transverse waves
50. 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.
Absolute zero
Atom
Latent heat of vaporization
Mutual Induction