Celestial Objects
Measurements
Astronomists
Newtons World
Poles
100

a star which generates its own energy
1 AU from Earth
self luminous object (gives off its own light)

The Sun

100

Distance from sun to earth

1 Astronomical Unit (AU)

100

Earth was at the center of the universe

In Pre-Copernican astronomy, it was universally believed that...

100

The greater the mass of an object, the greater the amount of force is needed to accelerate it

Newtons Second Law

100

the apparent path of the sun against the background

Eliptic

200

groups of stars that make an apparent pattern in the sky

Constelations

200

distance traveled by light in one year

1 Light Year

200

Spots on the sun, craters on the moon, moons around Jupiter, and moon like phases of Venus

Galileo found with a telescope

200

An object continues in its state of rest or motion, unless an external force is applied to it

Newtons 1st Law

200

Polaris appears closer to the horizon

At lower altitudes

300

a great cloud of stars, gas and dust held together by gravity and all its matter

Galaxy

300

109 earth diameters

Diameter of the Sun

300

Spots on the sun, craters on the moon, moons around Jupiter, and moon like phases of Venus

Tycho Brahe's greatest contribution to astronomy

300

a property of matter by which it continues in its existing state of rest or uniform motion in a straight line, unless that state is changed by an external force.

Inertia

300

causes the north celestial pole to trace a circle on the sky, once every 26000 years

Precission

400

planets and all objects orbiting the sun

Solar System

400

in one hour stars move an angular distance of 15 degrees

Rate at which stars move

400

a planet should move at its greatest speed when it is closest to the sun.

Kepler's second law

400

For every action, there is an equal and opposite reaction

Newtons third law

400

projection of Earth's south pole on the Celestial Sphere

South Celestial Pole

500

Cluster of galaxies

Supercluster

500

4 minutes

How much earlier stars will rise than the previous night

500

He developed a theory of Gravity that could explain orbital motion.

Newton's greatest contribution to astronomy

500

Increases with the mass of the objects and decreases with the distance between them

The force due to gravity between objects

500

point on the Celestial Sphere directly underneath

Nadir