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