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