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