Quizlet Everyday physics final study guide

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  1. 1 BTU: the heat needed to raise the temperature of 1 pound of water by 1 degree F
  2. Acceleration: change in velocity / time
  3. Acceleration due to gravity on the earth: -10 m/s^2
  4. amplitude: maximum displacement from equilibrium
  5. Aristotle: believed that the natural state of objects was to be at rest
  6. atmospheric pressure (atm): 100,000 n/m^2
  7. azX: z+n
  8. bernoulli’s equation: fluid flow velocity=u, fluid density=p (rho), fluid pressure=P P + ½ p x u^2 + p x g x h= constant
  9. Brahe: Compiled the first detailed observational data on planetary motion (mars), without a telescope.
  10. Buoyant force: weight of displaced water=volume of displaced water in liters x 10 n / liter
  11. c=3x10^8 m/s: ?
  12. Center of gravity (CG): the center of an object
  13. Centripedal acceleration=: velocity squared / radius
  14. Change in internal energy: heat into system – work done by system
  15. Condition for stability: if the CG is above the edge, the object will not fall
  16. Conduction: heat is transferred directly through a material with no bulk movement of material
  17. Conservation of energy: you can’t get more work out than the energy you put in
  18. continuity: v x A= constant
  19. Convection: heat is carried from place to place by the bulk movement of either liquids or gasses
  20. Convert Celsius to Fahrenheit: 9/5T(C)+32
  21. Convert Celsius to Kelven: T(C) +273
  22. Convert Fahrenheit to Celsius: 5/9 [T(F)-32]
  23. definition of Bernoulii’s equation: as the speed of a moving fluid increases, the pressure within the fluid decreases
  24. density of air: 1.25 kg/m^3
  25. density of aluminum: 2,700 kg/m^3
  26. density of lead: 11,000 kg/m^3
  27. density of water: 1,000 kg/m^3
  28. Distance traveled: ½ acceleration x time^2
  29. Einstein: shows in 1905 that newtons laws were not valid for objects moving with speeds near the speed of light.
  30. Emissive: the efficiency with which an object emits thermal radiation. Is a number between 0 and 1. A good emitter has an e close to 1.
  31. Energy of motion (kinetic energy): ½ m v^2
  32. Engine efficiency: work done / heat in
  33. Engine efficiency cannot be 100%: you cant get as much out as you put in
  34. entropy: the total disorder of an object
  35. Equilibrium: net force=0 net torque=0
  36. First Law of thermodynamics: If energy is transferred and the internal energy of system B decreases by some amount then the internal energy of system A must incrase by the same amount.
  37. Flow through a pipe: π(P2-P1)D^4/128Ln n=fluid’s viscosity
  38. Fluid force: pressure x area
  39. Frequency: 1 / period (time)
  40. frequency of light: speed of light / wavelength
  41. Galileo: the first to do experimental studies of the laws of motion and was Imprisoned by Pope Urban VIII in 1633 for advocating the Copernican theory, also know as the heliocentric theory, that the earth was a planet revolving around the sun.
  42. Heat: the energy that flows from one system to another because of their temperature difference.
  43. Heat: mass x specific heat x temperature change
  44. Heat capacity (specific heat): the amount of heat that is required to raise the temperature of one g of a substance by 1 degree C.
  45. Heat capacity equation: heat Q= mass of sample x specific heat x temp change
  46. incoming and outgoing flow rate formula: v1 x A1=v2 x A2
  47. infrasound: sounds below 30 Hz
  48. Internal energy: the sum of the energy of all the molecules in the system
  49. Kepler: analized brahe’s data and verified the heliocentric theory. These regularities are known as Helpers Laws of Planetary motion.
  50. law of conservation of energy: the change in internal energy= the heat absorbed- the work done
  51. mass flow rate formula: p x u x A
  52. measure of density: kg/m^3
  53. measurement of pressure: Pascal (Pa) or pounds per square inch (psi)
  54. mechanical wave: a disturbance that propagates through a medium
  55. Mechanics: why things move
  56. Momentum: mass x velocity
  57. Net force: the total force (positive and negative) acting upon an object
  58. Net force=0 net torque≠0: rod with forces applied at opposite ends in opposite directions
  59. Net force≠0 net torque=0: rod with forces applied at opposite ends in the same direction
  60. Newton: wrote Principia in 1687. Made the 3 laws of mechanics and law of gravity. He also invented calculus.
  61. Newton’s Second Law: f=mass x acceleration
  62. order of states of matter stronger to lesser forces between atoms: solids, liquids, gases
  63. Period: time required to complete one cycle
  64. period of a pendulum T of length L: 2π x square root L/g
  65. period p of a mass m oscillating on a horizontal spring of force constant k: t=2π square root m/k frequency= square root k/m;/2π
  66. Photon energy: hf
  67. Physics: The study of how objects behave (from the very tiny to the very big, and from the beginning of the Universe to its ultimate fate).
  68. Power (watts): current x voltage energy/time (joules per second)
  69. Present velocity: initial velocity = acceleration x time
  70. pressure at depth h: p + density x g h
  71. pressure depends on: number density x temperature
  72. pressure does what when depth is increased: it increases
  73. Pressure=: force per unit area
  74. Projectile: an object that is thrown or struck or shot and then travels under the influence of gravity
  75. Quantum mechanics: new theory that explained behavior at the atomic level
  76. Radiation: the heat transfer by electromagnetic waves – thermal light waves
  77. Resistance: voltage / current
  78. restoring force: the force that brings a system back to equilibrium
  79. Rotational inertia (moment of inertia): how much torque it takes to get an object rotating
  80. Second law of thermodynamics: if the temperature of system A is less then the temperature of system B then heat flows from B to A (hot to cold)
  81. Speed of light: 18600 miles/sec
  82. Stable: not easy to knock over
  83. Stable structures: are wider at the base (which lowers their center of gravity)
  84. static fluid formula: Fbottom=Ftop+mg where mg is the weight of the volume
  85. the pressure of liquids _____ when it goes faster: decreases
  86. The US uses how much of the total world energy consumption?: 25%
  87. Thermal conductivity: the effectiveness of a material in conducting heat
  88. Thermal radiation: T^4
  89. Thermodynamics: the study of heat and its transformation into mechanical energy
  90. Time for an object thrown to reach maximum height: time= the square root of 2 x height / acceleration due to gravity
  91. Torque: the combination of force and point of application
  92. Torque: force x lever arm
  93. Total momentum before collision: equals total momentum after collision
  94. ultrasound: sounds above 20,000 Hz
  95. variation of pressure with depth: Fbottom-Ftop=mg=(density x vol) x g
  96. Velocity required for an object to reach height h: initial velocity= the square root of 2gh
  97. velocity through a medium: c/n
  98. Velocity=: distance traveled / time
  99. viscosity: a tendency for liquids to resist flowing.
  100. Voltage: current x resistance
  101. volume fluid flow rate: gallons per minute (gpm), liters/s, cubic feet per minute (cfm) or m^3/s
  102. volume fluid flow rate formula: tube cross section area A, flow speed u vfr= u x A (m/s x m^2)
  103. wave: a disturbance that moves through something
  104. Wave speed=: wavelength x frequency
  105. wavelength: length of a wave
  106. Wavelength: c / f
  107. Weight: mass x gravity
  108. when ice in water melts what happens?: the level stays the same
  109. Why does something move?: because nothing stops it