02 - Motions of Planets and Other Celestial Bodies Flashcards

1
Q

turning of the body on an axis. A day/A spin

A

Rotation

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2
Q

spinning around an object or star. A year/A orbit

A

Revolution

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3
Q

Earth-Centred Model. Created to seek accuracy in “perfect” geometry

A

Geocentric Universe Model

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4
Q

Sun-Centred Model. Sun-centered scientific revolution - adoption of new paradigm (accepted scientific ideas/assumptions)

A

Heliocentric Universe Model

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5
Q

List the Planets in order from the sun (8)

A
  1. Mercury
  2. Venus
  3. Earth
  4. Mars
  5. Jupiter
  6. Saturn
  7. Uranus
  8. Nepture
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6
Q

Earth’s orbit projected on the celestial sphere. The apparent path of the sun around the sky.

A

Ecliptic

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7
Q

Plato the philosopher proposed perfect motion (constant speed, perfect circles). Planets (wanders) was a big problem to this theory.

A

Uniform Circular Motion

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8
Q

planet moves westward for a few months

A

Retrogade Motion

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9
Q

Sir Isaac Newton’s idea of universal theory of gravitation revealed that objects are actually falling into another, as an apple falls to earth. This explains…

A

Orbital Motion

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10
Q

Mercury, Venus, Earth (moon), Mars are…

A

Terrestial/Inner Planets. Which means they are small in diameter, dense, little or no atmosphere.

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11
Q

Jupiter, Saturn, Uranus, and Neptune are…

A

Jovian/Outer Planets.
Which means they are relatively larger, have no solid surface, “liquid” giants (compressed gas)

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12
Q

Larger in size and cooler than the temperature of the planet. It’s important for retaining gases.

A

Atmosphere

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13
Q

Carbon Dioxide (CO2) rich atmosphere traps heat and raises surface temperature

A

Greenhouse Effect

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14
Q

result of small differences in gravitational force of one massive body on another

A

Tidal Force

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15
Q

Boundary beyond which water vapour could freeze to form ice grains

A

Ice line

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16
Q

Tiny, cold, irregular to sphere in shape, growth or captures asteroids that rotate planets (ex. Jupiter has 74 moons)

A

Satellite System (Moons)

17
Q

Minimum distance of a planet to a satellite that can hold itself together by gravity without tidal forces overcoming it.

A

Roche Limit

18
Q

Stripes that circle the planet parallel to equator (Jupiter)

Belt- darker descending gas lower in atmosphere
Zone- brighter, rising gas cloud high in atmosphere

A

Belt-Zone Circulation

19
Q

small bit of matter (dust, sand, pebble, most less than 1 gram) in space

A

Meteoroid

20
Q

Meteoroid fall that earth’s atmosphere friction heats the surface to incandescent vapour

A

Meteor

21
Q

Large enough that a portion survives fall through atmosphere and strikes the ground.

A

Meteorite

22
Q

small rocky world which most orbit the sun between mars and jupiter

A

Asteroids/Asteroid Belt

23
Q

Collection of Icy Planetstimals orbiting just beyond Neptune

A

Kupier Belt

24
Q

Small icy body that orbits the sun and produces tails of gas and dust when they approach the Sun

A

Comet

25
Q

Hypothetical source of distant comets, icy bodies, spherical. It is the edge of the sun’s reach and is one light year big

A

Oort Cloud

26
Q

space debris incapable of clearning its orbit, many are not spherical, often not on the eclpitic.

A

Dwarf Planet