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