Gravity, Satellites and Elliptical Orbit Flashcards

1
Q

Just to recap, what is gravity exactly? 0-0

A

Gravity is a fundamental force of nature that pulls (attracts) two objects toward each other.

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2
Q

So, what is a gravitational field?

A

It’s a region in space surrounding a mass where other masses experience a force of attraction (gravity).

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3
Q

Can you draw a gravitational field with a smaller mass (test mass) and a larger mass, and indicate the direction of gravitational force?

A

SLAYYYY

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4
Q

What’s the concept of gravitational field?

A

An object with mass will experience a gravitational force if it’s within a gravitational field of another mass

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5
Q

Finish the sentence! Let’s say small planet SY is nearby larger planet J

The larger mass planet J will have gravitational field….

A

stronger than than SY, which is why S Y gets pulled towards J due to gravity

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6
Q

What’s the formula of gravitational field strength?

A

𝑔⃗=𝐺𝑚/𝑟^2

m is larger mass right??

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7
Q

Can yall prove that Earth’s gravitational field strength is 9.80m/s^2?

A

YALL SHOULD 0-0

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8
Q

What’s Newton’s Law of Universal Gravitation about?

A

Every body in the universe attracts every other body with a *force directly proportional to the product of the 2 masses *and is *inversely proportional to r^2 *(square of distance between them from the centre)

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9
Q

About Newton’s Law of Universal Gravitation…

WHAT DA FORMULA?

A

F = G ((m1m2)/r^2))

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10
Q

About Newton’s Law of Universal Gravitation formula…

What does G represent?

A

That’s the Universal Gravitational Constant of 6.674 x 10^-11

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11
Q

What are satellites?

A

Any body that orbits a more massive object due to gravitational attraction between the two

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12
Q

What’s a natural satellite?

A

Satellites that are natural like the moon orbiting the earth or the earth orbiting the sun

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13
Q

What’s an artifical satellite?

A

A man-made satellite for GPS, internet, comms, military etc

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14
Q

What’s the centripetal force for satellites that allow them to always be in circular orbit?

A

Gravity!!

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15
Q

If satellites are at lower attitude, what should they do to keep orbit?

A

Increase their speed!

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16
Q

What happens if satellites can’t be in circular orbit no more, what do they turn to?

A

They do an elliptical orbit instead!

17
Q

Why if satellites’ speed are too high, they go in elliptical orbit?

A

Because if the speed to too much, then they need more centripetal force. But centripetal force is gravity which you can’t change.

18
Q

What is the formula to help determine the speed of the satellite & how do yall derive that?

A

V = square root of (GM/r)

19
Q

Can a satellite orbit earth NOT in the centre?

A

NO! because centripetal force is directed towards the centre. If no centre -> IMPOSSIBLE girliesss

20
Q

What is an equatorial orbit?

A

An orbit that’s geostationary = to remain above the same point on Earth’s surfaces

It orbits side to side on the the Earth’s surface

21
Q

What are equatorial orbits good for?

A

Good for monitoring things, communicating

22
Q

What are equatorial orbits NOT good for

A

Taking detailed satellite images because it’s far away from surface

If are any issues -> $$$$$ to go up there and fix it

23
Q

What is a polar orbit?

A

Low earth orbits (<1000m) that have low periods of 1.5-2hrs cuz they fast

Orbits around the polar caps (up and down if yk what i mean?)

24
Q

What are polar orbits good for?

A

If combine it with many polar orbits, they can take very detailed images which is good for weather maps!

25
Q

What is Kepler’s 1st Law?

A

All planets move in elliptical orbits with the Sun at one focus, which meant the sum of the distances from any point to the two foci is constant.

26
Q

Can you draw a diagram that explains Kepler’s 1st Law?

A

YALL SHOULD 0-0

27
Q

What’s Kepler’s 2nd Law?

A

“The radius vector drawn from the Sun to a planet sweeps equal areas in equal time intervals” which means the areas are always equal in size no matter where.

28
Q

Can yall draw a diagram that explains Kepler’s 2nd Law?

A

YALL SHOULD

29
Q

In regards to Kepler’s 2nd Law

Why is it when something is near the Sun, the acceleration increases?

A

1) When it’s near the Sun, there’s more gravity force.

2) When it’s near the Sun, distance (r) between them decreases, which increases gravity force.

F = ma, when F increase, a increase
F= (Gm1m2)/r^2 , r decrease, F incre

30
Q

What’s Kepler’s 3rd Law?

A

A formula that T^2 = (4piesquaredrcubed)/GM

31
Q

In regard to Kepler’s 3rd Law

Can you use that formula for anything? 0-0

A

NO only for circular orbits