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