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