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Gravitational fields

lizabeth rawson physics A level English 43 cards

what does the graph of F against r look like

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  1. 1define gravitational fielda field created around any object with mass, extending all the way to infinity, but diminishing as the distance from the centre of mass of the object increases
  2. 2define gravitational field strengththe gravitational force exerted per unit mass at a point within a gravitational field
  3. 3define gravitational field lineslines of force used to map the gravitational field pattern around any object having mass
  4. 4define radial fielda symmetrical field that diminishes with distance^2 from its centre, such as the gravitational field around a spherical mass or the electrical field around a spherical charged object
  5. 5define point massa mass with negligible volume
  6. 6define uniform gravitational fielda gravitational field in which the field lines are parallel and the value for g stays constant
  7. 7define newton's law of gravitationthe force between two point masses is directly proportional to the product of the masses and inversely proportional to the square of the separation between them
    F = G(Mm)/R^2
  8. 8define gravitational constantthe constant in newton's law of gravitation F = G(Mm)/R^2
    with a value of 6.67x10^-11
  9. 9define kepler's first lawthe orbit of a planet is an ellipse with the sun at one of the two foci
  10. 10define kepler's second lawa line segment connecting a planet to the sun sweeps out equal areas during equal intervals of time
  11. 11define kepler's third lawthe square of the orbital period T of a planet is directly proportional to the cube of its average distance r from the sun
  12. 12define ellipsean elongated circle with two foci
  13. 13define eccentricitya measure of the elongation of an ellipse
  14. 14define aphelionthe furthest point from the sun in an orbit
  15. 15define perihelionthe closest point to the sun in an orbit
  16. 16define astronomical unitthe mean distance from the earth to the sun
  17. 17define geostationary satellitesa satellite that remains in the same position relative to a spot on the Earth's surface, by orbiting in the direction of the earth's rotation over the equator with a period of 24 hours
  18. 18define gravitational potentialthe work done per unit mass to bring an object from infinity to a point in the gravitational field
  19. 19give the equation for gravitational field strengthg = f/m
  20. 20give the equation for newton's law pf gravitationF = G(Mm)/R^2
    where F is the force between two point masses, G is 6.67x10^-11, M is the mass of the object orbited, m is the mass of the object orbiting, and R is the distance between them
  21. 21what is F directly proportional to1/R^2
    Mm
  22. 22what does the graph of F against r look likewhat does the graph of F against r look like
  23. 23what does the graph of F against 1/r^2 look likewhat does the graph of F against 1/r^2 look like
  24. 24how do you derive the equation for gravitational field strength in a radial field?how do you derive the equation for gravitational field strength in a radial field?
  25. 25what does the negative sign in the equation for gravitational field strength represent?it shows that the gravitational field strength is in the opposite direction to the displacement from the centre of mass
  26. 26what is the gravitational field strength directly proportional toM
    1/r^2
  27. 27why are most planets orbits modelled as circles?they have low eccentricity
  28. 28how can kepler's third law be written as an equationT^2 / r^3 = constant
  29. 29how does centripetal force relate to gravitational forcecentripetal force on planet = gravitational force on planet
    mv^2 / r = GMm/r^2
    or
    v^2 = GM / r
  30. 30how can you find the speed of a planetv = 2pi r / T
  31. 31what is the equation for T^2T^2 = (4pi^2/GM)r^3
  32. 32define satellitea body orbiting around a planet
  33. 33what is the equation for gravitational force of a satelliteF = mv^2/r = GMm/r^2
  34. 34what is the equation for speed of a satellitev = square root (GM/r)
  35. 35name uses of geostationary satellites and advantages and disadvantagesTV and phone signals, local weather satellites. lower resolution, expensive, risk of them falling back to earth, likely to break or malfunction
  36. 36name uses of polar satellites a advantages and disadvantagndesGPS systems, military spying, space research since they have lower orbit so higher resolution, cannot continuously communicate with a spot on earth's surface
  37. 37what are polar orbitsorbits which circle the poles
  38. 38what is low earth orbitorbits which are close to the earth,
  39. 39what is symbol for gravitational potential and example valueVg, all values are negative because it is 0 at infinity, all are negative because gravitational force is attractive
  40. 40what are the factors which decide the gravitational potential in a radial fielddistance from the point mass producing the gravitational field to that point, the mass of the point mass
  41. 41what is the equation for gravitational potentialVg = -GM/r
  42. 42what is the equation for gravitational potential energyE = m(Vg) = - GMm/r
  43. 43what is the equation for escape velocityv = square root (2GM/r)

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physics A level (M5 Chapter 18 Gravitational fields ) Flashcards on Gravitational fields , created by lizabeth rawson on 03/12/2021.
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