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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 points midway between nodes on a standing wave - where the oscillations are largest.
Newton
De Broglie wavelength
Nuclear fusion
Antinode
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.
Strong nuclear force
Principal axis
Oscillation
Uncertainty principle
3. In an interference or diffraction pattern - the places where there is the least light.
Alpha particle
Minima
Gravitational constant
Amplitude
4. A collision in which the colliding particles stick together.
Angular acceleration
Quark
Completely inelastic collision
Motional emf
5. An equation - PV = nRT - that relates the pressure - volume - temperature - and quantity of an ideal gas. An ideal gas is one that obeys the approximations laid out in the kinetic theory of gases.
Ideal gas law
Latent heat of sublimation
Oscillation
Compression
6. A positively charged particle that - along with the neutron - occupies the nucleus of the atom.
Mass number
Basis vector
Proton
Hypotenuse
7. A particle - which consists of two protons and two neutrons. It is identical to the nucleus of a helium atom and is ejected by heavy particles undergoing alpha decay.
Kelvin
Index of refraction
Unit vector
Alpha particle
8. In a right triangle - the tangent of a given angle is the length of the side opposite the angle divided by the length of the side adjacent to the triangle.
Wave speed
Tangent
Electron
Tail
9. 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.
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10. Also called a converging lens - a lens that is thicker in the middle than at the edges. Convex lenses refract light through a focal point.
Strong nuclear force
Equilibrium
Convex lens
Tip
11. The unit for measuring pressure. One Pascal is equal to one Newton per meter squared - 1 Pa = 1 N/m2.
Optics
Pascals
Transformer
Impulse
12. For two given media - the smallest angle of incidence at which total internal reflection occurs.
Inertia
Nuclear fusion
Radius of curvature
Critical angle
13. 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 - .
Fundamental
Kelvin
Melting point
Hooke's Law
14. Energy associated with an object's position in space - or configuration in relation to other objects. This is a latent form of energy - where the amount of potential energy reflects the amount of energy that potentially could be released as kinetic e
Virtual image
Traveling waves
Potential energy
Total internal reflection
15. If two systems - A and B - are in thermal equilibrium and if B and C are also in thermal equilibrium - then systems A and C are necessarily in thermal equilibrium.
Coefficient of static friction
Zeroth Law of Thermodynamics
Angular velocity
Radius of curvature
16. For a gas held at a constant temperature - pressure and volume are inversely proportional.
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17. A device that breaks incoming light down into spectral rays - so that one can see the exact wavelength constituents of the light.
Elastic collision
Power
Spectroscope
Wavelength
18. The unit of magnetic flux - equal to one T · m2.
Decibel
Momentum
Weber
Torque
19. A nuclear reaction that takes place only at very high temperatures. Two light atoms - often hydrogen - fuse together to form a larger single atom - releasing a vast amount of energy in the process.
Nuclear fusion
Coefficient of linear expansion
Torque
Pitch
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
Gravitational Potential Energy
Magnetic flux
Harmonic series
Directly proportional
21. 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
Superposition
Doppler shift
Longitudinal waves
Equilibrium position
22. 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.
Lenz's Law
Snell's Law
Gravitational Potential Energy
Translational kinetic energy
23. 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
Significant digits
Meson
Beats
24. A body or set of bodies that we choose to analyze as a group.
Radioactivity
Completely inelastic collision
Magnitude
System
25. A device that converts mechanical energy to electrical energy by rotating a coil in a magnetic field; sometimes called a "dynamo."
Atomic number
Electric generator
Weak nuclear force
Optics
26. 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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27. The energy stored in a thermodynamic system.
Internal energy
Directly proportional
Constructive interference
Force
28. 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.
Doppler shift
Nuclear fission
Mass defect
Kinetic friction
29. 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.
Elastic collision
Instantaneous velocity
Sound
Scalar
30. The property by which a charge moving in a magnetic field creates an electric field.
Translational kinetic energy
Electromagnetic induction
Standing wave
Dynamics
31. An image created by a mirror or lens in such a way that light does not actually come from where the image appears to be.
Virtual image
Minima
Faraday's Law
Basis vector
32. A negatively charged particle that orbits the nucleus of the atom.
Total internal reflection
Newton's First Law
Electron
De Broglie wavelength
33. Two materials are in thermal equilibrium if they are at the same temperature.
Thermal equilibrium
Radioactive decay
Vector
Michelson-Morley experiment
34. The points on a standing wave where total destructive interference causes the medium to remain fixed at its equilibrium position.
Completely inelastic collision
Node
Phase
Law of conservation of energy
35. A measurement of a body's inertia - or resistance to being accelerated.
Moment of inertia
Mass
Inclined plane
Zeroth Law of Thermodynamics
36. 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.
Maxima
Significant digits
Pulley
Real image
37. A law - || = - which states that the induced emf is the change in magnetic flux in a certain time.
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38. The stable position of a system where the net force acting on the object is zero.
Equilibrium position
Uniform circular motion
Center of mass
Heat transfer
39. The center of a mirror or lens.
Ground state
Transformer
Vertex
Potential energy
40. A transfer of thermal energy from one system to another.
Polarization
Heat transfer
Kinematic equations
Electron
41. A system with many parts in periodic - or repetitive - motion. The oscillations in one part cause vibrations in nearby parts.
Directly proportional
Wave
Celsius
Diffraction
42. 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.
Zeroth Law of Thermodynamics
Unit vector
Diffraction grating
Angular velocity
43. 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.
Magnification
Speed
Frictional force
Wavelength
44. The amount of heat needed to raise the temperature of one gram of water by one degree Celsius. 1 cal = 4.19 J.
Calorie
Half
Torque
Sine
45. 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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46. 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.
Zeroth Law of Thermodynamics
Antinode
Significant digits
Coherent light
47. The two shorter sides of a right triangle that meet at the right angle.
Reflected ray
Legs
Latent heat of sublimation
Rutherford nuclear model
48. Waves carried by variations in air pressure. The speed of sound waves in air at room temperature and pressure is roughly 343 m/s.
Sound
Centripetal acceleration
Law of reflection
Gamma ray
49. The reaction force of the ground - a table - etc. - when an object is placed upon it. The normal force is a direct consequence of Newton's Third Law: when an object is placed on the ground - the ground pushes back with the same force that it is pushe
Right-hand rule
Normal force
Strong nuclear force
Photon
50. 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.
Constructive interference
Inversely proportional
Hertz (Hz)
Latent heat of fusion