Slow rotation of the whole pattern of stars around the ecliptic axis
Perihelion
Happens in early JANUARY
Earth moves FAST
Aphelion
Happens in early JULY
Earth moves SLOW
Rotation
1. Spinning of the earth on its axis
2. Axis - imaginary line from North to South pole; tilted 23.5˚
3. 24 hours or 1 day
Revolution
1. Movement of the earth around the sun
2. One complete revolution takes 365 1/4 days or 1 year
Diurnal motion
DAILY motion of stars and other celestial bodies
Refers to the daily rising and setting of the sun
Rise - East
Set - West
Due to Earth's rotation
Annual motion
YEARLY motion of stars and other celestial bodies
Due to Earth's revolution
Precession of the equinoxes
26,000 years
Hipparchus
Precession is caused by the gravitational pull of the sun and moon
Precession of the equinoxes is a slow rotation of the whole pattern of stars around the ecliptic axis
Kinematics
A branch of mechanics that is the science of describing the motion of objects using words, diagrams, numbers, graphs, and equations
Free-falling bodies
All objects fall at the same rate regardless of their weight
Leaning Tower of Pisa
Galileo discovered through this experiment that the objects fell with the same acceleration
Galileo stated that in the absence of air resistance all objects fall with the same uniform acceleration
Inclined Plane Experiment
No force is needed to keep an object moving with constant velocity
Galileo explained that if there were no interferences, objects moving in a straight line will continue to move without the need of a FORCE
Push or pull is NOT needed for the object to move
Projectile motion
It is a combination of uniform forward motion and free-fall motion
Galileo was the first person to describe projectile motion, accurately. He segregated motion into horizontal and vertical components
If the projection angle is other than 90o, the ball follows curved paths
If the projection angle is 90o with horizontal, the ball follows a vertical path
Nothing accelerates a projectile horizontally, so horizontal acceleration is always zero
Vertical and horizontal components of projectile motion are independent of each other
A projectile follows a two-dimensional motion: vertically or horizontally, the motion can be studied as a combination of two simultaneous one-dimensional motions
Galileo Galilei
An Italian astronomer who used his own telescope to make astronomical observations and found significant evidence supporting the HELIOCENTRIC MODEL
Galileo's views on motion
Observation & experiment
Free falling bodies
Projectile motion
Uniform motion
Aristotle's views on motion
Push and pull
Natural/resting place
Based on composition - earth/land, water, fire, and air
Heavier objects fall faster
Force is required in Violent motion
Galileo's views on motion
No push or pull is required to keep an object from moving
No natural place/resting place
Air resistance - objects fall at the same rate regardless of their weight
Force is not necessarily required for Violent motion
Kinematics
A branch of mechanics that is the science of describing the motion of objects using words, diagrams, numbers, graphs, and equations
Celestial bodies
Objects in space such as the moon, sun, planets, and stars
Celestial
Outer space; heaven; sky
Terrestrial
Earth; land
Terrestrial sphere
Made of four elements: earth, air, fire, and water, subject to change and decay
Celestial spheres
Made of a fifth element, an unchangeable aether
Ancient Greeks believed the cosmos or the universe was divided into two realms - celestial and terrestrial
Motion of celestial realm
Perfect and circular, revolving around Earth
Motion of terrestrial realm
Unstable and imperfect, requires a cause
Natural motion
Where objects tend to go back to their natural state, based on the element that composes them, does not require an external cause
Violent motion
Motion requires force, refers to the action necessary to move things horizontally, does not happen without action