When travelling northward, stars in the north get higher in the sky while stars in the south get lower. The reverse happens when travelling south
Looking at the moon during a lunar eclipse
Celestial motion
The motion of planets, the Moons and the stars
Diurnal motion
Daily rotation of the Earth, Moon, Stars and Sun
Annual motion
Revolution of the planet Earth around the Sun for a length of 365 days, and six hours
Terrestrial motion
The motion of everyday objects
Plato's view of the cosmos
The earth was in the center of the universe and did not move
Eudoxus' view of the cosmos
Planets and stars rotated around the Earth in circular motion
Observed that planets did not follow a uniform circular motion and proposed retrograde motion
Aristotle's view of the cosmos
The Earth was the center of the universe
Aristarchus' view of the cosmos
The first to introduce the sun-centered solar system
Interest on the size of the universe and the distance between the planets
Ptolemy's view of the cosmos
Follower of Aristotle's idea and constructed an elaborate model based on Mathematics
The Ptolemaic model, which is geocentric system places the Earth at the center of the universe
Copernicus' view of the cosmos
Gave credit to the first modern heliocentric system
Set the correct order of the planets based on the extent of their retrograde motion
TychoBrahe's contributions
Accurate measurements of the stars and planets for over 20 years
Developed a quadrant that was used to measure the position of the stars with precision
Kepler's contributions
A believer of Copernican's heliocentric universe
Became a major figure in the scientific revolution in the 17th century because of his planetary motion that formed the basis for Newton's theory of universal gravitation
Galileo's contributions
Used his first telescope in 1609 to study the moon, the stars and the sun
These discoveries cast doubts on Ptolemaic geocentric theory that heaven is perfection
Motion
The movement or change in location of an object
Aristotelian concept of motion
Terrestrial motion - Limited and vertical motion
Celestial motion - Circular and endless motion
Projectile motion - The motion of a stone after it leaves the hand of a thrower. Composed of both natural motion and imposed motion. Aristotle believed that everything moved must be moved by something
Galilean concept of motion
Natural motion - not constrained by an external force
Non-naturalmotion - also called Impressed motion, occurs when an object is pushed into some non-natural motion by an external force; projectile motion is the key
Acceleration
An object that is slowing down, speeding up or changing direction is said to be accelerating
Galileo's concept of acceleration and horizontal motion
Lighter object moved slightly ahead of the heavier object during initial stage of free fall but heavier object caught up and eventually passed lighter object
Motion with constant velocity
When object travels the same distance every second, then the object is moving with constant velocity. The magnitude of velocity and direction of velocity both remain constant
Speed
How fast an object moves. This is constant and does not indicate direction of motion
Velocity
Combination of speed and direction, defined as the rate of change of position
Unitsofvelocity
meters per second (m/s), kilometers per hour (km/h or kph) and miles per hour (mi/h or mph)
Constantvelocity
A vector
Newton's first law of motion (lawofinertia)
State of Rest: If body is at rest, it remains at rest until some external forces act on it
State of Motion: If a body is in motion, it continues to move with the same speed in the same direction until an external force acts on it and changes its velocity
Newton's second law of motion (lawofforce)
Acceleration of a body is inversely proportional to its mass, directly proportional to the force and in the same direction as the force
Newton's third law of motion (law of reactions)
For every action, there is an equal and opposite reaction
Visiblelight
The light that humans can see even animals and insects
Light
Scientists often call light electromagneticradiation
Properties of light
Light travels in a straightline and fast in a vacuum while slow down when it passes to an solid object
Particle theory of light
The particle theory suggests that light particles always travel in a straight line
Wave theory of light
The wave theory of light suggests that the beam of light spreads and becomes wider as light passes through a narrow slit
Reflection
Bouncing of lights when it hits an object. If the surface is perfectly smooth, light rays undergo reflection
Refraction
The change in direction of light wave as light passes from one transparent medium to another such as in glass or water
Transmission
Some materials allow much of the light that falls on them to pass through the material without being reflected. Materials such as glass allow transmission of light through them are called transparent
Absorption
This occurs when an object does not reflect or transmit the light instead it is taking in. Ability of objects to absorb light is dependent on the electromagnetic frequency of the light being transmitted and the nature of the atoms in an object