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