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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. A reference frame in which Newton's First Law is true. Two inertial reference frames move at a constant velocity relative to one another. According to the first postulate of Einstein's theory of special relativity - the laws of physics are the same i
Inertial reference frame
Weightlessness
Latent heat of transformation
Electron
2. 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.
Conservation of Angular Momentum
Uncertainty principle
Concave mirror
Gravitational Potential Energy
3. The force involved in beta decay that changes a proton to a neutron and releases an electron and a neutrino.
Convex mirror
Weak nuclear force
Uniform circular motion
Inclined plane
4. The property by which a charge moving in a magnetic field creates an electric field.
Electromagnetic induction
Gold foil experiment
Latent heat of vaporization
Deposition
5. The gravitational force exerted on a given mass.
Electromagnetic induction
Induced current
Weight
Right-hand rule
6. 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.
Celsius
Pendulum
Decay constant
Impulse
7. The five equations used to solve problems in kinematics in one dimension with uniform acceleration.
Virtual image
Wavelength
Mass defect
Kinematic equations
8. The study of the properties of visible light - i.e. - the portion of the electromagnetic spectrum with wavelengths between 360 and 780 nm (1 nm = m/s).
Dot product
Moment of inertia
Antinode
Optics
9. The mass number - A - is the sum of the number of protons and neutrons in a nucleus. It is very close to the weight of that nucleus in atomic mass units.
Nucleus
Internal energy
Spring constant
Mass number
10. 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
Refracted ray
Beta decay
Vector
Directly proportional
11. 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.
Convex mirror
Kinetic friction
Work
Torque
12. 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.
Mole
Radian
Dispersion
Kepler's Third Law
13. The building blocks of all matter - quarks are the constituent parts of protons - neutrons - and mesons.
Loudness
Newton's Law of Universal Gravitation
Quark
Latent heat of vaporization
14. A quantity that possesses a magnitude but not a direction. Mass and length are common examples.
Dynamics
Kepler's First Law
Scalar
Pulley
15. The straight line that runs through the focal point and the vertex of a mirror or lens.
Gold foil experiment
Neutrino
Principal axis
Reflect
16. A scalar quantity that tells us how fast an object is moving. It measures the rate of change in distance over time. Speed is to be contrasted with velocity in that there is no direction associated with speed.
Sine
Margin of error
Speed
Angle of incidence
17. 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
Angular acceleration
Second Law of Thermodynamics
Zeroth Law of Thermodynamics
Orbit
18. The angle between a reflected ray and the normal.
Work function
Deposition
Real image
Angle of reflection
19. The points of maximum displacement along a wave. In traveling waves - the crests move in the direction of propagation of the wave. The crests of standing waves - also called anti-nodes - remain in one place.
Tip
Transverse waves
Crest
Kepler's First Law
20. For a gas held at constant pressure - temperature and volume are directly proportional.
21. A law - || = - which states that the induced emf is the change in magnetic flux in a certain time.
22. A property of a metal - the minimum frequency of electromagnetic radiation that is necessary to release photoelectrons from that metal.
Threshold frequency
Significant digits
Dynamics
Hooke's Law
23. 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.
Compression
Coherent light
Longitudinal waves
Neutron number
24. The movement of a rigid body's center of mass in space.
Translational motion
Atom
Concave lens
Zeroth Law of Thermodynamics
25. An object at rest remains at rest - unless acted upon by a net force. An object in motion remains in motion - unless acted upon by a net force.
26. 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.
Rotational motion
Efficiency
Electronvolt
Magnitude
27. When dealing with reflection or refraction - the incident ray is the ray of light before it strikes the reflecting or refracting surface.
Heat
Coherent light
Incident ray
Angular position
28. 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
Proton
Conservation of Angular Momentum
Collision
Mechanical energy
29. Energy cannot be made or destroyed; energy can only be changed from one place to another or from one form to another.
Law of conservation of energy
Boyle's Law
Incident ray
Zeroth Law of Thermodynamics
30. The ray of light that is reflected from a mirror or other reflecting surface.
Distance
Reflected ray
Optics
Component
31. 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
Beta particle
Right-hand rule
Direction
Meson
32. A wavelength - given by = h/mv - which is associated with matter. Louis de Broglie proposed the idea that matter could be treated as waves in 1923 and applied this theory successfully to small particles like electrons.
Sine
Equilibrium
Ground state
De Broglie wavelength
33. A negatively charged particle that orbits the nucleus of the atom.
Electron
Calorie
Traveling waves
Medium
34. The force that binds protons and neutrons together in the atomic nucleus.
System
Deposition
Strong nuclear force
Rotational kinetic energy
35. A form of vector multiplication - where two vectors are multiplied to produce a scalar. The dot product of two vectors - A and B - is expressed by the equation A · B = AB cos .
Electromagnetic wave
Dot product
Law of reflection
Virtual image
36. The unit for measuring pressure. One Pascal is equal to one Newton per meter squared - 1 Pa = 1 N/m2.
Calorie
Neutron number
Pascals
Angular period
37. In an interference or diffraction pattern - the places where there is the most light.
Radioactivity
Maxima
Newton's Law of Universal Gravitation
Longitudinal waves
38. The emf created by the motion of a charge through a magnetic field.
Magnitude
Newton
Charles's Law
Motional emf
39. 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.
Photoelectric effect
Significant digits
Velocity
Pendulum
40. If the net torque acting on a rigid body is zero - then the angular momentum of the body is constant or conserved.
Lenz's Law
Destructive interference
Conservation of Angular Momentum
Medium
41. A system that no external net force acts upon. Objects within the system may exert forces upon one another - but they cannot receive any impulse from outside forces. Momentum is conserved in isolated systems.
Angular momentum
Heat engine
Spring constant
Isolated system
42. 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.
Real image
Radiation
Pitch
Latent heat of sublimation
43. 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
Meson
Legs
Acceleration
44. A wedge or a slide. The dynamics of objects sliding down inclined planes is a popular topic on SAT II Physics.
Diffraction grating
Inclined plane
Heat
Dispersion
45. 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.
Third Law of Thermodynamics
Translational kinetic energy
Transformer
Pendulum
46. The force of gravity - F - between two particles of mass and - separated by a distance r - has a magnitude of - where G is the gravitational constant. The force is directed along the line joining the two particles.
47. The units of frequency - defined as inverse-seconds (1 Hz = 1 s-1). "Hertz" can be used interchangeably with "cycles per second."
Hertz (Hz)
Induced current
Reflect
Heat engine
48. The center of an atom - where the protons and neutrons reside. Electrons then orbit this nucleus.
Nucleus
Equilibrium
Weak nuclear force
Potential energy
49. When electromagnetic radiation shines upon a metal - the surface of the metal releases energized electrons. The way in which these electrons are released contradicts classical theories of electromagnetic radiation and supports the quantum view accord
Photoelectric effect
Angular period
Critical angle
Spring
50. A transfer of thermal energy from one system to another.
Centripetal acceleration
Weight
Photon
Heat transfer