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Test your basic knowledge |
Praxis Physics Basic Principles
Start Test
Study First
Subjects
:
praxis
,
science
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. Measure of gravitational pull of Earth on an object or between two bodies
Radioactivity
Weight
Thermal Energy
Mass
2. A misguided belief that a system can continuously produce more energy than it consumes.
Stable Isotopes
Density
Perpetual Motion
Thermodynamic Equilibrium
3. Energy transferred to a body by a means other than work. (through the process of heat)
Thermal Energy
Thermal Contact
Density
Radioisotopes
4. Isotopes that have unstable nuclei and can undergo spontaneous nuclear reactions which results in particle or radiation being emitted.
Radioactive Half - life
Matter
Radioactive Isotopes
Stable Isotopes
5. Causes an electron to detach from an atom; occurs in radioactive reactions. Three types: 1. Alpha 2. Beta 3. Gamma
Entropy
Gamma Rays
Heat
Ionizing Radiation (3 types)
6. Substances that consist of only one type of atom
Elements
Ionizing Radiation (3 types)
Heat Engine
Heat
7. 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
Density
Gamma Rays
Stable Isotopes
Chemical Properties
8. Joining of two nuclei; occurs under extreme temperatures and pressure. Fusion occurs naturally in stars (responsible for the release of great energy).
Chemical Change
Physical Changes
Open Systems (physics)
Nuclear Fusion
9. 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.
Specific Gravity
Nuclear Fusion
Radioisotopes
Potential Energy
10. A Machine that converts thermal energy to mechanical energy that can be used to do work
Surrounding Environment (physics)
Heat Engine
Water displacement
Atomic Mass
11. Refers to the energy of an object in motion.
Atomic Weight
Thermodynamic Equilibrium
Kinetic Energy
Volume
12. Substance containing two or more elements; formed by chemical reactions. Can only be separated by a chemical reaction
Entropy
Compound
Electron Shell Configuration
Joule
13. Refers to the fact that the total amount of energy in a closed system is constant
Radiation
Mixtures
Weight
Conservation of Energy
14. How do you determine the volume of an irregularly shaped object?
Matter
Atomic Mass
Mixtures
Water displacement
15. Rate at which work is performed
Physical properties
Heat Engine
Weight
Power
16. Contain two or more substances that are combined but have not reacted chemically. They can be separated using physical methods
Kinetic Energy
Atomic Weight
Chemical Properties
Mixtures
17. This refers to objects that have the same temperature b/c heat is transferred between them to reach equilibrium
Thermodynamic Equilibrium
Compound
Mixtures
Molecule
18. 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.
Work
Alpha Rays
Stable Isotopes
Most abundant Elements in Universe
19. 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.
Mixtures
Water displacement
Radioactive Half - life
Beta Rays
20. Branch of Physics that studies the conversion of energy into work and heat. Concerned w/ variables such as temperature - volume - and pressure
Kinetic Energy
Thermodynamics
First Law of Thermodynamics
Closed Systems (physics)
21. 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.
Work
Isotope
Radioisotopes
Solutions
22. Isotopes that have not been observed to decay
Specific Gravity
Stable Isotopes
Radiation
Mixtures
23. A change that does not result in different substances; when an object changes form but not compostion.
Radioisotopes
Perpetual Motion
Potential Energy
Physical Changes
24. The capacity to do work
Atoms
Energy
Power
Chemical Properties
25. The measure of the ratio of a substance's density compared to the density of water.
Specific Gravity
Radioactive Decay
First Law of Thermodynamics
Chemical Properties
26. Total Kinetic Energy and Potential Energy in a system
Molecule
Alpha Rays
Elements
Thermal Energy
27. A system that can exchange heat and work - but not matter
Ionizing Radiation (3 types)
Radioactive Isotopes
Specific Gravity
Closed Systems (physics)
28. Measure of the amount of substance in an object
Physical Changes
Alpha Rays
Mass
Electron Shell Configuration
29. Capable of interacting with a surrounding environment and can exchange heat - work (energy) and matter outside their system boundaries
Open Systems (physics)
Ionizing Radiation (3 types)
Physical Changes
Weight
30. Refers to the particles that are emitted from nuclei as a result of nuclear instability
Power
Radioactivity
Beta Rays
Elements
31. 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
Power
Thermodynamics
Thermal Contact
Heat
32. A change that results in a different substance. They may release or consume energy.
Heat Engine
Radioactive Half - life
Chemical Change
Compound
33. Substances that have mass and occupy space
Nuclear Fission
Matter
Atoms
Kinetic Energy
34. Two or more atoms held together by covalent bonds
Matter
Weight
Radioactive Half - life
Molecule
35. When energy is emitted by one body and absorbed by another
Radiation
Work
Thermodynamics
Physical properties
36. Conservation of Energy (energy can only be transferred - not created or destroyed)
First Law of Thermodynamics
Chemical Change
Nuclear Fission
Radioactive Isotopes
37. The time it takes for half of the radioactive nuclei in a sample to undergo radioactive decay.
Heat
Mixtures
Compound
Radioactive Half - life
38. Measure of the amount of mass per unit volume.
First Law of Thermodynamics
Electron Shell Configuration
Entropy
Density
39. Splitting of a large nucleus into smaller pieces
Potential Energy
Isolated System (physics)
Nuclear Fission
Elements
40. Hydrogen and Helium are the most abundant. Than Oxygen - Neon - Nitrogen - Carbon - Silicon - and Magnesium.
Nuclear Fusion
Solutions
Most abundant Elements in Universe
Alpha Rays
41. A System that cannot exchange heat - work - or matter with its surroundings. Total Energy & Mass stay constant w/in system
Radioisotopes
Thermodynamics
Isolated System (physics)
Kinetic Energy
42. 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)
Entropy
Heat Engine
Density
Ionizing Radiation (3 types)
43. Measurement of Work
Isolated System (physics)
Joule
Heat
Most abundant Elements in Universe
44. 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.
Thermodynamic Equilibrium
Stable Isotopes
Chemical Change
Gamma Rays
45. The smallest unit of matter that has the characteristics of an element; consists of three main types of subatomic particles: protons neutrons and electrons.
Closed Systems (physics)
Atoms
Physical properties
Perpetual Motion
46. 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.
Molecule
Perpetual Motion
Heat
Atomic Weight
47. Attributes such as appearance - color - mass - and volume.
Physical properties
Heat Engine
Matter
Three states of matter
48. Homogeneous mixtures composed of two or more substances that have become one
Thermal Energy
Atoms
Atomic Mass
Solutions
49. Measurement of the amount of cubic space occupied.
Potential Energy
Chemical Change
Physical properties
Volume
50. 1st (K Shell) = 2 electrons - 2nd (L Shell) = 8 electrons - 3rd (M Shell) = 18 electrons - 4th (N Shell) = 32 electrons
Mixtures
Electron Shell Configuration
Nuclear Fusion
Isolated System (physics)