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