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