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