1Diurnal Motion
apparent daily motion of the sun, moon, stars etc
2The sidereal rate
The earth rotates 360 degrees in one day, so celestial objects appear to move across the sky at 15 degrees an hour
3Measuring angles in the sky
Extending your arm, your fist is 10 degrees
4Nautical Twilight
The center of the sun is geometrically 12 degrees below the horizon, so the horizon is still visible and allows reliable navigational star sightings
5Civil twilight
Center of sun is geometrically 6 degrees blow the horizon, artificial illumination isn’t required outdoors
6Astronomical twilight
Center of sun is geometrically 18 degrees below the horizon, light from sun is less than starlight
7Annual motion
Yearly motion, the complete motion around the sun
8Seasons
Earth has a rotational axial tilt of 23.5 degrees, which causes ____
9Horizon calendar
The rising and setting points of the sun
10Ptolemaic system
A solar system with Earth in the center, equinoxes/eclipses/solstices were off by days to months
11Nikolas Copernicus
Proposed the heliocentric solar system and explained retrograde motion as an optical illusion
12Galileo Galilei
Best known for using his telescopic observations and supporting the copernican system, wrote Sidereus Nuncius and discovered Sun’s spots, Jupiter’s moons
13Tycho Brahe
Didn’t accept the Copernican model, believed in teh Tychonic system, built a planetarium to prove his theory correct and made incredibly accurate measurements of Mars
14Johannes Kepler
Discovered the three laws of planetary motion
15First law of planetary motion
The orbits of the planets are ellipses with the sun as one focus, eccentricity describes the shapes of the planet’s orbits
16Second law of planetary motion
Law of areas, a line from the sun to a planet sweeps out an equal area in an equal amount of time, planets move faster the closer it is to the sun
17Third law of planetary motion
Harmonic law, the square of the planet’s orbital period is proportional to the cube of its mean distance from the sun. If you know a planet’s distance from the sun, you can determine it’s orbital period
18Isaac Newton
Invented physics, the laws of motion, the law of universal gravitation and explained orbits
19First law of motion
Law of inertia, a body in motion will remain in motion unless acted upon by an outside force, and will remain at rest until acted upon
20Second law of motion
In order to accelerate a mass you must apply a force, usually expressed as an algebraic equation f=ma
21Third law of motion
For every action there is an equal and opposite reaction
22Law of universal gravitation
Gravity works between pairs of objects, between any two objects in the universe there is a mutual attraction that is proportional to the product of their masses and inversely proportional to the square of the distance of separation between their centers
23Orbits
An object is actually in a constant state of falling, tangential velocity and acceleration combine to create this