Orbits and Gravity Flashcards
Explain Brache
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
Briefly explain Keplers 3 laws
Described the behaviour of planets based on their paths through space
Explain major axis
The widest diameter of the ellipse
Explain semimajor axis
- 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
Explain eccentricity
The ratio of the distance between the foci to the length of the major axis
State Kepler’s first law
Each planet moves around the Sun in an orbit that is an ellipse, with the Sun at one focus of the ellipse
State Kepler’s second law
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 )
State Kepler’s third law
The square of a planet’s orbital period is directly proportional to the cube of the semi-major axis of its orbit
Explain angular momentum
- 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
What are the two classes of objects in heliocentric orbits
Asteroids and comets
Asteroid vs Comet
- 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
Explain Perihelion
Point where a planet is closest to the Sun and has maximum orbital speed
Explain Aphelion
Point where a planet is farthest from the Sun and has minimum orbital speed
Explain why Newton had to determine the exact nature of the attraction
- Explain why/how planets move as described by Kepler’s Laws
- Predict correct behaviour of moving/falling bodies on Earth
Breifly explain Kepers 3rd law
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,
Explain Keplers first 2 law
- 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