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Test your basic knowledge |
Praxis Physics Basic Principles
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Subjects
:
praxis
,
science
Instructions:
Answer 50 questions in 15 minutes.
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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. Branch of Physics that studies the conversion of energy into work and heat. Concerned w/ variables such as temperature - volume - and pressure
Molecule
Volume
Electron Shell Configuration
Thermodynamics
2. A system that can exchange heat and work - but not matter
Closed Systems (physics)
Heat Engine
Three states of matter
Radiation
3. Can be Beta - Minus or Beta Plus. Beta - Minus: contain an energetic electron Beta - plus: emitted by positrons and can result in gamma photons. Beta particles can be stopped by thin metal.
Beta Rays
Thermodynamic Equilibrium
Mass
Heat
4. Isotopes that have not been observed to decay
Radioactive Decay
Solutions
Stable Isotopes
Thermal Energy
5. Homogeneous mixtures composed of two or more substances that have become one
Surrounding Environment (physics)
Physical properties
Solutions
Most abundant Elements in Universe
6. Causes an electron to detach from an atom; occurs in radioactive reactions. Three types: 1. Alpha 2. Beta 3. Gamma
Physical properties
Radioisotopes
Ionizing Radiation (3 types)
Thermal Contact
7. A variation of an atom; occur when the number of protons in the nucleus are the same but the number of neutrons are not. Written as the element plus the number of Neucleons (i.e. Carbon -13 (6 Protons - 7 Neutrons)
Weight
Isotope
Specific Gravity
Atomic Weight
8. 1st (K Shell) = 2 electrons - 2nd (L Shell) = 8 electrons - 3rd (M Shell) = 18 electrons - 4th (N Shell) = 32 electrons
Ionizing Radiation (3 types)
Electron Shell Configuration
Joule
Thermal Energy
9. The quantity of energy transferred by one system to another due to changes in a system that is the result of external forces; also can be described as the amount of energy that must be transferred to overcome a force.
Gamma Rays
Thermal Energy
Radiation
Work
10. Measure of the amount of substance in an object
Chemical Change
Mass
Conservation of Energy
Mixtures
11. Total Kinetic Energy and Potential Energy in a system
Atomic Mass
Water displacement
Power
Thermal Energy
12. Refers to the particles that are emitted from nuclei as a result of nuclear instability
Specific Gravity
Volume
Solutions
Radioactivity
13. The smallest unit of matter that has the characteristics of an element; consists of three main types of subatomic particles: protons neutrons and electrons.
Elements
Atoms
Heat Engine
Isotope
14. Positive; larger than Beta. Because of their large mass they can be easily stopped (even with a sheet of paper.) Can cause severe damage if ingested.
Most abundant Elements in Universe
Compound
Stable Isotopes
Alpha Rays
15. Transfer of Energy from a body or system as a result of thermal contact. Heat consists of random motion and the vibration of atoms - molecules - & ions. Higher the temperature - greater the atomic/molecular motion
Atomic Mass
Stable Isotopes
Heat
Density
16. Substances that consist of only one type of atom
Ionizing Radiation (3 types)
Elements
Beta Rays
Gamma Rays
17. Contain two or more substances that are combined but have not reacted chemically. They can be separated using physical methods
Mixtures
Nuclear Fission
Stable Isotopes
Volume
18. Properties concerned with the constituent particles that make up a substance. Can include: Atomic Number - Category - Group - Period - Block - weight - electron configuration - electrons per shell - phase - density - Sublimation point - specific heat
Physical Changes
Chemical Properties
Thermal Contact
Solutions
19. Refers to everything outside a thermodynamic system.
First Law of Thermodynamics
Gamma Rays
Surrounding Environment (physics)
Density
20. Two or more atoms held together by covalent bonds
Compound
Most abundant Elements in Universe
Molecule
Radioisotopes
21. A change that results in a different substance. They may release or consume energy.
Nuclear Fission
Electron Shell Configuration
Chemical Change
Radioactive Isotopes
22. Refers to the amount of energy in a system that is no longer available for work. (also used to describe the amount of disorder in a group)
Electron Shell Configuration
Isotope
Entropy
First Law of Thermodynamics
23. Energy transferred to a body by a means other than work. (through the process of heat)
Weight
Thermal Contact
Radioactive Decay
Elements
24. Measurement of Work
Joule
Heat Engine
Chemical Properties
Perpetual Motion
25. Hydrogen and Helium are the most abundant. Than Oxygen - Neon - Nitrogen - Carbon - Silicon - and Magnesium.
Solutions
Heat
Most abundant Elements in Universe
Three states of matter
26. Measure of gravitational pull of Earth on an object or between two bodies
Weight
Radiation
Alpha Rays
Kinetic Energy
27. A Machine that converts thermal energy to mechanical energy that can be used to do work
First Law of Thermodynamics
Heat Engine
Radiation
Nuclear Fusion
28. Type of High energy electromagnetic radiation consisting of photons. It rids the decaying nucleus of excess energy after it has emitted either alpha or beta radiation. They can cause serious damage to living tissue. It takes thick lead to stop them.
Radioisotopes
Solutions
Gamma Rays
Stable Isotopes
29. Rate at which work is performed
Power
Thermal Energy
Radioactive Isotopes
Atomic Mass
30. A misguided belief that a system can continuously produce more energy than it consumes.
Perpetual Motion
Isotope
Thermodynamics
Atomic Weight
31. A change that does not result in different substances; when an object changes form but not compostion.
Entropy
Molecule
Physical Changes
Thermal Contact
32. The measure of the ratio of a substance's density compared to the density of water.
Radioactive Decay
Work
Specific Gravity
Thermodynamic Equilibrium
33. Refers to the energy of an object in motion.
Thermodynamic Equilibrium
Solutions
Stable Isotopes
Kinetic Energy
34. Atoms that have an unstable nucleus that has excess energy and the potential to make radiation particles within the nucleus or undergo radioactive decay which can result in the emission of gamma rays. May occur naturally or artificially produced.
Joule
Radioisotopes
Compound
Volume
35. This refers to objects that have the same temperature b/c heat is transferred between them to reach equilibrium
Weight
Thermodynamic Equilibrium
Thermal Energy
Electron Shell Configuration
36. Measurement of the amount of cubic space occupied.
Isotope
Mixtures
Joule
Volume
37. AKA Mass Number. The total number of protons and Neutrons in the nucleus of an atoms. Referred to as 'A.'
Atomic Mass
Radiation
Ionizing Radiation (3 types)
Potential Energy
38. The time it takes for half of the radioactive nuclei in a sample to undergo radioactive decay.
Thermodynamic Equilibrium
Radioactive Half - life
Joule
Power
39. The capacity for doing work that is based upon position or configuration.
Potential Energy
Physical properties
Alpha Rays
Heat Engine
40. Attributes such as appearance - color - mass - and volume.
Compound
Thermodynamic Equilibrium
Volume
Physical properties
41. How do you determine the volume of an irregularly shaped object?
Most abundant Elements in Universe
Entropy
Alpha Rays
Water displacement
42. Conservation of Energy (energy can only be transferred - not created or destroyed)
Radioisotopes
First Law of Thermodynamics
Chemical Change
Power
43. Measure of the amount of mass per unit volume.
Nuclear Fission
Density
Volume
Work
44. Refers to the fact that the total amount of energy in a closed system is constant
Conservation of Energy
Open Systems (physics)
Density
Atomic Weight
45. Capable of interacting with a surrounding environment and can exchange heat - work (energy) and matter outside their system boundaries
Entropy
Water displacement
Closed Systems (physics)
Open Systems (physics)
46. Joining of two nuclei; occurs under extreme temperatures and pressure. Fusion occurs naturally in stars (responsible for the release of great energy).
Chemical Change
Isolated System (physics)
Potential Energy
Nuclear Fusion
47. Ratio of the average mass per atom of a sample (which can include various isotopes) to 1/12 of the mass of an atom of carbon -12.
Chemical Change
Alpha Rays
Compound
Atomic Weight
48. The capacity to do work
Mixtures
Chemical Change
Energy
Isotope
49. Substances that have mass and occupy space
Surrounding Environment (physics)
Most abundant Elements in Universe
Matter
Joule
50. A System that cannot exchange heat - work - or matter with its surroundings. Total Energy & Mass stay constant w/in system
Energy
Entropy
Most abundant Elements in Universe
Isolated System (physics)
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