SUBJECTS
|
BROWSE
|
CAREER CENTER
|
POPULAR
|
JOIN
|
LOGIN
Business Skills
|
Soft Skills
|
Basic Literacy
|
Certifications
About
|
Help
|
Privacy
|
Terms
|
Email
Search
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. Waves produced by a source that is moving with respect to the observer will seem to have a higher frequency and smaller wavelength if the motion is towards the observer - and a lower frequency and longer wavelength if the motion is away from the obse
Doppler shift
Normal
Velocity
Kinetic energy
2. A property common to both vectors and scalars. In the graphical representation of a vector - the vector's magnitude is equal to the length of the arrow.
Dispersion
Cross product
Distance
Magnitude
3. The amount of heat necessary to transform a solid at a given temperature into a liquid of the same temperature - or the amount of heat needed to be removed from a liquid of a given temperature to transform it into a solid of the same temperature.
Photon
Translational motion
Latent heat of fusion
Moment of inertia
4. 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 acceleration
Bohr atomic model
Efficiency
Convection
5. A unit of force: 1 N is equivalent to a 1 kg · m/s2.
Real image
Newton
Entropy
Center of mass
6. 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.
Radioactive decay
Photoelectric effect
Strong nuclear force
Isolated system
7. A device that converts mechanical energy to electrical energy by rotating a coil in a magnetic field; sometimes called a "dynamo."
Heat
Electric generator
Reflection
Work function
8. 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
Newton's Third Law
Directly proportional
Potential energy
Electromagnetic spectrum
9. 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.
Coefficient of static friction
Rigid body
Electromagnetic spectrum
Kinetic friction
10. 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
Spring constant
Second Law of Thermodynamics
De Broglie wavelength
Fundamental
11. A unit vector is a vector with length 1.
Unit vector
Displacement
Free
Crest
12. A vector quantity - or vector - is an object possessing - and fully described by - a magnitude and a direction. Graphically a vector is depicted as an arrow with its magnitude given by the length of the arrow and its direction given by where the arro
Zeroth Law of Thermodynamics
Mole
Angular acceleration
Vector
13. The temperature at which a material will change phase from solid to liquid or liquid to solid.
Sine
Work function
Instantaneous velocity
Melting point
14. The cosine of an angle in a right triangle is equal to the length of the side adjacent to the angle divided by the length of the hypotenuse.
Simple harmonic oscillator
Rutherford nuclear model
Celsius
Cosine
15. The emf created by the motion of a charge through a magnetic field.
Tail
Tip
Motional emf
Pendulum
16. 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.
Thermal equilibrium
Index of refraction
Angular displacement
Magnetic flux
17. A collision in which both kinetic energy and momentum are conserved.
Uncertainty principle
Elastic collision
Latent heat of transformation
Threshold frequency
18. 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
Heat engine
Pendulum
Angular frequency
Collision
19. Also called a diverging lens - a lens that is thinner in the middle than at the edges. Concave lenses refract light away from a focal point.
Decay constant
Concave lens
Right-hand rule
Significant digits
20. For an oscillating spring - the restoring force exerted by the spring is directly proportional to the displacement. That is - the more the spring is displaced - the stronger the force that will pull toward the equilibrium position. This law is expres
21. 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.
Pascals
Thermal equilibrium
Joule
Significant digits
22. 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.
Uncertainty principle
Coefficient of kinetic friction
Photon
Weightlessness
23. The bending of light at the corners of objects or as it passes through narrow slits or apertures.
Transformer
Center of mass
Diffraction
Kepler's First Law
24. The time it takes a system to pass through one cycle of its repetitive motion. The period - T - is the inverse of the motion's frequency - f = 1/T.
Scalar
Principal axis
Period
Real image
25. Relates the angle of incidence to the angle of refraction: .
26. A back-and-forth movement about an equilibrium position. Springs - pendulums - and other oscillators experience harmonic motion.
Sublimation
Snell's Law
Momentum
Oscillation
27. Energy cannot be made or destroyed; energy can only be changed from one place to another or from one form to another.
Work function
Real image
Law of conservation of energy
Inertia
28. The amount of energy that metal must absorb before it can release a photoelectron from the metal.
Work function
Equilibrium
Inelastic collision
Ideal gas law
29. A sheet - film - or screen with a pattern of equally spaced slits. Typically the width of the slits and space between them is chosen to generate a particular diffraction pattern.
Nuclear fission
Diffraction grating
Frictional force
Threshold frequency
30. The amplification of one wave by another - identical wave of the same sign. Two constructively interfering waves are said to be "in phase."
Convection
Planck's constant
Constructive interference
Torque
31. The points of maximum negative displacement along a wave. They are the opposite of wave crests.
Angular momentum
Trough
Distance
Latent heat of sublimation
32. 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.
Destructive interference
Gamma ray
Spring
Rotational motion
33. 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.
Tangent
Thermal energy
Convection
Conduction
34. 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.
Angular acceleration
Magnification
Radian
Coefficient of volume expansion
35. Occurs when every point in the rigid body moves in a circular path around a line called the axis of rotation.
Rotational motion
Inelastic collision
Antinode
Third Law of Thermodynamics
36. 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
Virtual image
Temperature
Angular momentum
Angular period
37. A particle - identical to an electron. Beta particles are ejected from an atom in the process of beta decay.
Total internal reflection
Weak nuclear force
Photoelectric effect
Beta particle
38. A device that breaks incoming light down into spectral rays - so that one can see the exact wavelength constituents of the light.
Oscillation
Real image
Proton
Spectroscope
39. A coefficient that tells how much a material will expand or contract lengthwise when it is heated or cooled.
Latent heat of transformation
Cycle
Concave mirror
Coefficient of linear expansion
40. 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.
Incident ray
Pressure
First Law of Thermodynamics
Nuclear fusion
41. The amount of heat of a material required to raise the temperature of either one kilogram or one gram of that material by one degree Celsius. Different units may be used depending on whether specific heat is measured in s of grams or kilograms - and
Specific heat
Force
Hypotenuse
Translational motion
42. The process by which a gas turns directly into a solid because it cannot exist as a liquid at certain pressures.
Angular frequency
Crest
Virtual image
Deposition
43. The unit for measuring pressure. One Pascal is equal to one Newton per meter squared - 1 Pa = 1 N/m2.
Kepler's Second Law
Angle of refraction
Strong nuclear force
Pascals
44. Light such that all of the associated waves have the same wavelength and are in phase.
Gravitational constant
Coherent light
Maxima
Kinematic equations
45. The ray of light that is refracted through a surface into a different medium.
Electron
Refracted ray
Second Law of Thermodynamics
Pendulum
46. The ray of light that is reflected from a mirror or other reflecting surface.
Weightlessness
Elastic collision
Reflected ray
Boiling point
47. 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
Strong nuclear force
Tangent
Chain reaction
Activity
48. A unit for measuring angles; also called a "rad." 2p rad = 360º.
Radian
Newton's Law of Universal Gravitation
Real image
Boiling point
49. Waves that oscillate in the same direction as the propagation of the wave. Sound is carried by longitudinal waves - since the air molecules move back and forth in the same direction the sound travels.
Work function
Thermal equilibrium
Center of mass
Longitudinal waves
50. The force that binds protons and neutrons together in the atomic nucleus.
Diffraction grating
Strong nuclear force
Second Law of Thermodynamics
Potential energy