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