Set: Astronomy Lect. 10

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All 28 terms

TermDefinition
Isaac Newtonduring a closure of Cambridge during 1665-1666 bc of the plague, invented the integral and differential calculus, developed the binomial theorem, started fundamental work on optics, formulated his laws of motion and gravitation
Newton's SynthesisThe Principia is one of the most important books in history: Laid the foundations of modern physics, swept away the last vestiges of the Aristotelian view of the world, replaced older, empirical descriptions with quantifiable, physical explanations of teh nature of the world, unified ALL motions into three simple laws
Newtons 1st lawevery body will stay in a state of rest or uniform motion in a straight line unless that state is changed by forces impressed upon it, often called the law of inertia
inertiaproperty of matter that it resists having its state of motion changed
speedhow fast its going
directionwhere its going
velocityall motion comprised of two parts, speed and direction, combination is call this=how fast and in what direction
accelerationchanges in motion, measures how fast the velocity changes, change can be in speed,direction or both (does not have to always get faster, can be slowing down too)
Newtons 2nd lawthe size of accleration is directly proportional to the force applied, and inversely proportional to the mass of the body (the resulting acceleration is in the same direction as the applied force) a=f/m, or f=ma, quantifies force in terms of its effects on a massive body
accelerationsforces produce
more massthe ______ a body has, the less it can be accelerated by a given force
Newtons laws applied to planetary motionplanets are continually changing the speed and direction as they orbit the sun, move along ellipses with sun at one focus, fastest at perihelion, slowest at aphelion,
accelerating in response to force of gravitywhy does the speed and direction of planets change continually? -They are
Newtons 3rd lawfor every force applied to a body, there is an equal and oppositely directed force exerted in response
newton's laws of motionprovide a complete, quantitative explanation of the motions of objects, are simple & easily stated in words/mathematics, they are universal physical laws applicable to all objects on the earth or in the heavens, they unify phenomena, explaining all motions with the same set of self-consistent laws
the calculusthe full statement of the laws required the invention of a new mathematical language, independtly invented by newton and Leibnitz, the mathematics of change, gives us a way to describe the change in the velocity of a moving object with time, sets geometry into motion, provides a framework for exploring motion
law of falling bodiesin the absence of air, heavy objects and light objects fall at the same, constant rate of acceleration
attractive forcegravity is an ________, works to bring massive objects closer together
universal forcegravity is a _______, works everywhere in the Universe
mutual forcegravity is a _______, works between pairs of massive objects
masses, distancethe force of gravity between any two objects depends only upon the ______of the two objects, and the ________ between them
more massive_____ objects exert a stronger force of gravity
strongerthe force of gravity gets ______ as they move closer
weakerthe force of gravity gets ______ as they move apart
the force of gravitydoes not depend on the shapes, colors, or compositions of the objects
the law of universal gravitationthe force of gravitational attraction between any two massive bodies is proportional to their masses and inversely proportional to the square of the distance between their centers, in math: force of gravity= (Gravitational Force Constant x mass of first object x mass of second object)/(distance between their centers squared)
the gravitational force constantG=(6.7 x 10^-11 Newtons meter ^2)/(kilograms^2)
Newtonsthe metric of force, 4.41 of them equal 1 pound

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Creator nancypants
Created May 4, 2009
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  1. the law of universal gravitation the force of gravitational attraction between any two massive bodies is proportional to their masses and inversely proportional to the square of the distance between their centers, in math: force of gravity= (Gravitational Force Constant x mass of first object x mass of second object)/(distance between their centers squared) - 4 misses
  2. the gravitational force constant G=(6.7 x 10^-11 Newtons meter ^2)/(kilograms^2) - 3 misses
  3. newton's laws of motion provide a complete, quantitative explanation of the motions of objects, are simple & easily stated in words/mathematics, they are universal physical laws applicable to all objects on the earth or in the heavens, they unify phenomena, explaining all motions with the same set of self-consistent laws - 2 misses
  4. Newtons 2nd law the size of accleration is directly proportional to the force applied, and inversely proportional to the mass of the body (the resulting acceleration is in the same direction as the applied force) a=f/m, or f=ma, quantifies force in terms of its effects on a massive body - 2 misses
  5. more mass the ______ a body has, the less it can be accelerated by a given force - 2 misses
  6. Newton's Synthesis The Principia is one of the most important books in history: Laid the foundations of modern physics, swept away the last vestiges of the Aristotelian view of the world, replaced older, empirical descriptions with quantifiable, physical explanations of teh nature of the world, unified ALL motions into three simple laws - 2 misses
  7. more massive _____ objects exert a stronger force of gravity - 2 misses