Cards (85)

  • What are the two main types of orbital motion?
    Circular and elliptical
  • The gravitational force between two objects is given by F=F =Gm1m2r2 G \frac{m_{1} m_{2}}{r^{2}}, where rr is the distance between their centers
  • Orbital motion is primarily due to gravitational attraction.
  • Match the type of orbit with its characteristic:
    Circular ↔️ Constant speed and distance
    Elliptical ↔️ Varying speed and distance
  • In a circular orbit, the gravitational force provides the centripetal force needed to keep the object moving in a circle.
  • In a circular orbit, the object's speed is constant.
  • What is an example of an object in a circular orbit?
    Artificial satellites
  • The equation Gm1m2r2=\frac{G m_{1} m_{2}}{r^{2}} =mv2r \frac{m v^{2}}{r} shows the balance between gravitational and centripetal forces in a circular orbit.
  • In a circular orbit, the object's distance from the central object remains constant.
  • What is an example of a circular orbit in our solar system?
    Artificial satellites around Earth
  • The orbital speed vv in a circular orbit can be calculated using the equation v=v =Gm1r \sqrt{\frac{G m_{1}}{r}}, where rr is the radius
  • What equation shows the relationship between orbital speed and radius?
    Gm1m2r2=\frac{G m_{1} m_{2}}{r^{2}} =mv2r \frac{m v^{2}}{r}
  • The equation \frac{G m_{1} m_{2}}{r^{2}} = \frac{m v^{2}}{r}</latex> can be simplified to show the relationship between orbital speed and radius
  • Rearranging the equation Gm1m2r2=\frac{G m_{1} m_{2}}{r^{2}} =mv2r \frac{m v^{2}}{r} for v results in v=v =Gm1r \sqrt{\frac{G m_{1}}{r}}.
  • What is the relationship between orbital speed and radius according to the equation v=v =Gm1r \sqrt{\frac{G m_{1}}{r}}?

    Inversely proportional
  • For satellites around Earth, as the orbital radius increases, their speed decreases
  • What are the two main types of orbits?
    Circular and elliptical
  • A circular orbit maintains a constant speed and distance from the central object.
  • Orbital motion is caused by mutual gravitational attraction
  • What law governs gravitational force?
    Universal Gravitation
  • In a circular orbit, gravitational force and centripetal force are balanced.
  • As the orbital radius increases, what happens to the orbital speed?
    Decreases
  • In a circular orbit, gravitational force provides the necessary centripetal force.
  • The balance between gravitational and centripetal forces in a circular orbit can be represented by the equation Gm1m2r2=G \frac{m_{1} m_{2}}{r^{2}} =mv2r \frac{mv^{2}}{r}.
  • What is the equation for centripetal force?
    Fc=F_{c} =mv2r \frac{mv^{2}}{r}
  • In a circular orbit, gravitational force provides the necessary centripetal force.
  • What is the equation for gravitational force?
    F=F =Gm1m2r2 G \frac{m_{1} m_{2}}{r^{2}}
  • The balance between gravitational force and centripetal force in a circular orbit is represented by the equation Gm1m2r2\frac{G m_{1} m_{2}}{r^{2}}
  • What is the equation for the balance between gravitational force and centripetal force?
    Gm1m2r2=\frac{G m_{1} m_{2}}{r^{2}} =mv2r \frac{mv^{2}}{r}
  • A circular orbit is maintained by a balance between gravitational and centripetal forces.
  • What is the gravitational constant denoted by?
    GG
  • What two forces maintain a circular orbit?
    Gravitational and centripetal
  • A circular orbit requires a precise balance between gravitational and centripetal forces.
  • The gravitational force is given by F=F =Gm1m2r2 G \frac{m_{1} m_{2}}{r^{2}}, where GG is the gravitational constant
  • What do m1m_{1} and m2m_{2} represent in the gravitational force equation?

    Masses of the objects
  • What does rr represent in the gravitational force equation?

    Distance between centers
  • The centripetal force is given by Fc=F_{c} =mv2r \frac{mv^{2}}{r}, where mm is the mass of the satellite
  • What does vv represent in the centripetal force equation?

    Orbital speed
  • What does rr represent in the centripetal force equation?

    Orbital radius
  • For a circular orbit to be stable, the gravitational force must equal the centripetal force.