Chapter 4 Flashcards

1
Q

Gravity-

A

Fundamental force of nature. Mutually attractive force between two objects with mass.

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2
Q

What was gravity as measured by galileo and how does gravity differ at the equator and poles?

A

Measured as 9.8 m/s by Galileo. 9.83 at the poles and 9.78 at the equator.

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3
Q

Weight

A

The gravitation force of a planet acting on an object.

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4
Q

What was the first step Newton Arrived at when figuring out the universal law of gravitation.

A

Gravitational force= Something * Mass of Earth * Mass of Object

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5
Q

Inverse Square Law

A

The gravitational force is dependent on the square of the distance between the two objects.

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6
Q

Universal Gravitational Constant

A

G. Calculated as 6.67 times 10^-11 n^2/m^2

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7
Q

Universal Law of Gravitation

A

F-grav= G times (M1*M2)/r^2 (distance between center of mass)

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8
Q

Why do we experience gravity as pulling us downward when all object on the surface pull on each other object?

A

The sideways forces cancel out because the surface is nearly spherical. Therefore the only gravitational force we feel is pulling us down to the center of gravity of earth.

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9
Q

Orbit

A

Path an object takes when it is free falling around another object.

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10
Q

Free Fall

A

Falling freely in earth’s gravity never hitting the surface.

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11
Q

Centripetal Force

A

A force towards the center of a circle.

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12
Q

Circular Velocity

A

The velocity at which an object must travel in order to orbit in a perfect circle.

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13
Q

Satellite

A

The less massive object which is orbiting a larger object.

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14
Q

Bound Orbit

A

An orbit however eccentric that is gravitationally bound to another object.

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15
Q

Escape Velocity

A

The slowest speed at which an object must reach to no longer be bound to the gravity of another object.

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16
Q

Vcirc=

A

(Square root of GM)/(Square Root of R)

17
Q

Vesc

A

(Square root of 2) times Vcirc

18
Q

Center of Mass

A

The point at which object(s) are orbiting.

19
Q

Orbital Period=

A

Circumference of the orbit/circular velocity