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