Term
|
Definition
|
|
Term
Modern Astronomy and Cosmology |
|
Definition
Study of the entire universe using scientific instruments, methods and simulations |
|
|
Term
Distance from the sun to the earth |
|
Definition
150 million km 1.5 x 10^11 = 93 million miles |
|
|
Term
|
Definition
|
|
Term
|
Definition
|
|
Term
|
Definition
A group of superclusters in which our cluster is a part of |
|
|
Term
|
Definition
Motion of the stars in galaxies suggesting that there is an additional gravitational force due to a large amount of unseen matter What we see may be as little at 10% of total |
|
|
Term
|
Definition
Rate of expansion of the universe that seems to be increasing as if it were pushed outward by some unknown sources of energy |
|
|
Term
1)Prehistoric (<500 B.C.) 2)Classical (500 B.C. - 1400 A.D.) 3)Renaissance (400-1650) 4)Modern (After 1650 |
|
Definition
1) Obscene motion of stars and planets. Learned to keep time 2) Measurements of planetary motion made construction of simple geometrical models for motion 3) Telescope leading to mroe sophisticated models 4) Earth considered creator of the universe. All stars attached to a "Celestial Sphere" |
|
|
Term
|
Definition
All celestial objects (stars, planets, sun, moo) moved as if attached to the celestial sphere |
|
|
Term
Motion around the Celestial Sphere |
|
Definition
Earth takes approximated 365 days each year to revolve around the sun Tilt of earths axis 23.5 degrees causes seasons June - Summer solstice March, Summer - Equinox December - Winter Solstice |
|
|
Term
|
Definition
Determined by the time spent in front of a particular constellation |
|
|
Term
Who invented the telescope? |
|
Definition
Johannes Lippershey, dutch spectacle maker Galileo took idea from Lippershey |
|
|
Term
|
Definition
1) Magnify Images 2) Gather lots of light and see faint objects |
|
|
Term
Sir Isaac Newton 1643-1727 Cambridge University |
|
Definition
Considered most influential person in the history of physics Founding father of planetary motion |
|
|
Term
|
Definition
The Law of Inertia A body continues in a state of rest, or motion in a straight line at constant speed, unless a force is applied to it |
|
|
Term
|
Definition
An object is said to be in uniform motion if its speed and direction remain unchanged Has constant velocity Force will cause it to have non-uniform motion (chanigng velocity) Acceleration - change in velocity |
|
|
Term
Newtons 2nd Law Acceleration |
|
Definition
An object increasing or decreasing in speed along a straight line is accelerating Constant speed moving in a circle is accelerating Produced by a force and the two are proportional (i.e. forces) Measured in meters/second^2 (m/s^2) |
|
|
Term
|
Definition
Amount of matter an object contains Measure of an objects inertia Never changes |
|
|
Term
Newtons Second Law of Motion |
|
Definition
F = ma Amount of acceleration (a) that an object undergoes is proportional to the force applied(F) and inversely proportional to the mass (m) of the object Measured in kilograms (kg) |
|
|
Term
Newtons Third Law of Motion |
|
Definition
When two objects interact, they create equal and opposite forces on each other |
|
|
Term
Newtons Law of Universal Gravity |
|
Definition
Everything attracts everything else G (gravitational constant) = 6.67 x 10^-11 Nm^2/kg^2 |
|
|
Term
|
Definition
|
|
Term
|
Definition
To be able to escape into space from a celestial object, mass must obtain a critical speed called "escape velocity" Escape velocity of moon = 2.4km/s of earth = 11km/s Determined by: Vesc = 26M/R)^1/2 |
|
|
Term
Photoelectric Effect (Einstein) |
|
Definition
Light of a specific energy strikes solid surfaces, only electrons of a specific energy is ejected. |
|
|
Term
|
Definition
h = 6.63 x 10^-34 Nms(Newton meter seconds) |
|
|
Term
|
Definition
Refractor - light bent by lenses Reflector - light bent using mirrors |
|
|
Term
|
Definition
Changing of the direction of a beam of light as it enters a new medium For example - entering water, lenses, atmosphere |
|
|
Term
|
Definition
Largest visible telescopes Keck twin- 10 meter, multi-mirror telescopes in Hawaii |
|
|
Term
|
Definition
How big must a telescope be to see two objects individually |
|
|
Term
|
Definition
One of the first recorded astronomical objects |
|
|
Term
Advantages of space based/ground based telescopes |
|
Definition
Ground - Increased collecting power, equipment easily fixed Space - freddom from atmospheric blurring/absorption |
|
|
Term
|
Definition
Radius = 6,400 km Bulges at equator due to rotation Crest = Oxygen 45% and Silicon 27% Core 6,400 K = 110,000 degrees F Small S/V ratio |
|
|
Term
|
Definition
Shifting of large blocks of the Earth's surface |
|
|
Term
|
Definition
Primarily Nitrogen(78.08%) and Oxygen (20.95%) Remaining about 1% Include Carbon dioxide, ozone, water, and argon First three being important for life |
|
|
Term
|
Definition
Visible light reacts with the Earth's surface and converted to heat |
|
|
Term
|
Definition
Direction from the north magnetic pole to the south pole |
|
|