Gravitational Fields Flashcards

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1
Q

Gravitational fields

A

a region of space where a mass experiences a force due to the gravitational attraction of another mass

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2
Q

Equation for gravitational field

A

g = Fg / m

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3
Q

Describe the field lines of gravitational fields on a planet

A
  • Field lines always toward the centre of the mass
  • Gravitational force gets wearker as you get further away from the planet’s surface
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4
Q

Newton’s law of gravitation

A

any two point masses attract each other with a force that is directly proportional to the product of their masses and inversely proportional to the square of their seperation

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5
Q

Equation of Newton’s law of gravitation

A

Fg = GMm / r^2

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6
Q

The inverse square law

A

when a mass is twice as far away from one another, the force due to gravity reduces by 1/4 ; 1/r^2 relation

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7
Q

Gravitational field strength

A

a point where gravitational force exerted per unit mass on a small object is placed at that point

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8
Q

Equation for gravitational field strength

A

g = GM / r^2

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9
Q

GPE

A

the energy an object possess due to its position in a gravitational field

GPE = mgh

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10
Q

Gravitational potential

A

the work done per unit mass in bringing a test mass from infinity to a defined point

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11
Q

Equation of gravitational potential

A

ϕ = -GM / r

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12
Q

Why does gravitational potential have a negative value?

A

Because potential near an isolated mass when r is infinity is defined as 0

Gravitational forces are always attractive so when r decreases, positive work is done by the mass when moving from infinity to that point

Mass closer to each other = grav. potential becomes more negative

Mass further from each other = grav. potential becomes more positive

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13
Q

Equation for GPE of two point masses

A

GPE = -GMm / r

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14
Q

Equation for change in GPE of two point masses m and M from r1 to r2:

A

△ ϕ = GM (1/r1 - 1/r2)

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15
Q

Circular orbits in gravitational frields

A

Fg = F circ

GMm / r^2 = mv^2/r

Therefore: v^2 = GM / r

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16
Q

The orbital period

A

T^2 = √ 4πr^3 / GM

T^2 is directly proportional to r^3