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