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