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