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