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