Orbits and Gravity Flashcards

1
Q

Explain Brache

A

His extensive and precise observations enabled him to note that the positions of the planets varied from those given in published tables, which were based on the work of Ptolemy

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2
Q

Briefly explain Keplers 3 laws

A

Described the behaviour of planets based on their paths through space

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3
Q

Explain major axis

A

The widest diameter of the ellipse

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4
Q

Explain semimajor axis

A
  • Half this distance—that is, the distance from the centre of the ellipse to one end
  • Is usually used to specify the size of the ellipse
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5
Q

Explain eccentricity

A

The ratio of the distance between the foci to the length of the major axis

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6
Q

State Kepler’s first law

A

Each planet moves around the Sun in an orbit that is an ellipse, with the Sun at one focus of the ellipse

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7
Q

State Kepler’s second law

A

The straight line joining a planet and the Sun sweeps out equal areas in space in equal intervals of time

( known as the Law of Equal Areas )

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8
Q

State Kepler’s third law

A

The square of a planet’s orbital period is directly proportional to the cube of the semi-major axis of its orbit

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9
Q

Explain angular momentum

A
  • Angular momentum is a measure of the rotation of a body as it revolves around some fixed point
  • l = mvr
  • As a planet approaches the Sun on its elliptical orbit and the distance to the spin centre decreases, the planet speeds up to conserve the angular momentum. Similarly, when the planet is farther from the Sun, it moves more slowly
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10
Q

What are the two classes of objects in heliocentric orbits

A

Asteroids and comets

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11
Q

Asteroid vs Comet

A
  • Asteroids generally have orbits with smaller semi-major axes than those of comets
  • Reside in the asteroid belt
  • Comets have large orbits (elliptical, parabolic or hyperbolic) with larger eccentricity
  • K2 therefore tells us they spend most of their time far from the Sun, moving very slowly.
  • When comets approach the Sun, they get heated up and star ejecting gas. That’s when we see them
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12
Q

Explain Perihelion

A

Point where a planet is closest to the Sun and has maximum orbital speed

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13
Q

Explain Aphelion

A

Point where a planet is farthest from the Sun and has minimum orbital speed

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14
Q

Explain why Newton had to determine the exact nature of the attraction

A
  • Explain why/how planets move as described by Kepler’s Laws
  • Predict correct behaviour of moving/falling bodies on Earth
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15
Q

Breifly explain Kepers 3rd law

A

P^2 = a^3

  • P is measured in years, and a is measured in astronomical units (AU), the two sides of the proportionality relation become equal to one another
  • Says that a planet’s orbital period squared is proportional to the semi-major axis of its orbit cubed,
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16
Q

Explain Keplers first 2 law

A
  • Kepler’s first two laws of planetary motion describe the shape of a planet’s orbit and allow us to calculate the speed of its motion at any point in the orbit
  • Second law deals with the speed with which each planet moves along its ellipse, also known as its orbital speed

-First law said that the orbits of all the planets are ellipses