Term
| Kepler's FIrst Law of Planetary Motion |
|
Definition
|
1. Planets follow elliptical orbits; sun is at one focus.
|
|
|
Term
| Kepler's Second Law of Planetary Motion |
|
Definition
|
2. The planets sweep out equal areas of their orbits in equal time
|
|
|
Term
| Kepler's Third law of Planetary Motion |
|
Definition
|
Period squared equals the semi-major axis cubed.
|
|
|
Term
| Newton's First law of Motion |
|
Definition
|
Law of Inertia; An object will remain at rest or in uniform straight motion unless acted upon by an external force
|
|
|
Term
| Newton's second law of Motion |
|
Definition
|
the rate of change of momentum of an object is equal to the external force applied to it. f=ma
|
|
|
Term
| Newton's Third law of Motion |
|
Definition
|
action-reaction law. for every force applied by one body on another, an equal and opposite force is applied on the first body by the second.
Fsub1=-Fsub2
|
|
|
Term
| Newton's Universal Law of Gravitation |
|
Definition
|
curved orbits imply a force which we know to be gravitational
F= - G x Mm/r^2
|
|
|
Term
|
Definition
|
A planet in orbit about the Sun has an angular momentum = m v r...it's a constant, so if the radius increases, the velocity will decrease, and vice versa. Mass stays the same!
|
|
|
Term
|
Definition
|
The laws of physics that are true on the earth are true everywhere. Made earth like every other planet. Big change!
|
|
|
Term
|
Definition
|
laws of physics are the same for all observers
|
|
|
Term
|
Definition
|
distance over which wave repeats itself (distance between two peaks or troughs)
|
|
|
Term
|
Definition
|
|
Term
|
Definition
|
nanometers (1 x 10^-9 meters)
|
|
|
Term
|
Definition
|
|
Term
|
Definition
|
number of crests that passes a point in one second
|
|
|
Term
|
Definition
|
From Violet (short wavelength, high frequency) to Red (the opposite)
|
|
|
Term
| The Electromagnetic Spectrum |
|
Definition
|
From low to high frequency: Radio, microwaves, infrared, optical, ultraviolet, x rays, gamma rays.
|
|
|
Term
| Not all of the EM spectrum makes it through the atmosphere... |
|
Definition
|
|
Term
|
Definition
|
time is not a constant; clocks of observers
|
|
|
Term
|
Definition
|
Light Gathering Power- Dsub1^2/Dsub2^2
...answer is how many times brighter something will seem.
|
|
|
Term
|
Definition
|
|
Term
|
Definition
|
extremely accurate, used quadrants to measure the positions of the planets
GEOCENTRIC....moon orbited earth, other planets orbited sun while it orbited earth.
|
|
|
Term
|
Definition
|
a bright star that appears on the sky that was not there before, no parallax....cellestial sphere changes?!
|
|
|
Term
|
Definition
|
first to utilize the telescope for astronomy, recognized uniform acceleration of objects
|
|
|
Term
|
Definition
|
Lo, Europa, Ganymede, Castillo, other revolutions exist! Geocentricity? No thank you!
|
|
|
Term
| Galileo noticed what with telescopes? |
|
Definition
|
Moons of Jupiter, Craters on Moon, Sunspots, Saturn's Rings, Milky Way Galaxy, Phases of Venus (shouldve been only crescents)
|
|
|
Term
| Who invented the telescope? |
|
Definition
|
|
Term
|
Definition
|
plane of pendulum wants to maintain the same orientation, and will rotate to counteract earth's rotation.
|
|
|
Term
|
Definition
|
inherited Tycho's observations, and came up with laws of planetary motion!
|
|
|
Term
|
Definition
|
wrote Principia, estables laws of motion and law of gravity, and calculus...
|
|
|
Term
|
Definition
|
|
Term
|
Definition
|
|
Term
|
Definition
|
Helped lay foundations for Quantum Mechanics (energy is quantized or kept in bundles) and that light is made of photons.
|
|
|
Term
|
Definition
|
speed of light is a constant; 3 x 10^8 m/s
|
|
|
Term
|
Definition
|
|
Term
| Consequence of Relativity |
|
Definition
|
E=mc^2, where mass can be converted into energy, and back...
|
|
|
Term
| First Postulate - principle of equivalence |
|
Definition
|
observer cannot distinguish locally between the forces of acceleration or gravitation (elevator)
|
|
|
Term
|
Definition
|
Mass determines the curvature of space-time, and the curvature of space-time tells mass how to accelerate.
|
|
|
Term
|
Definition
|
as curvature of space-time increases due to the distance of a mass, time slows
|
|
|
Term
|
Definition
|
light falls toward gravitational body the same as a mass.
|
|
|
Term
|
Definition
|
sound -alternating regions of high and low densities DIRECTION OF TRAVEL
|
|
|
Term
|
Definition
|
Displacement perpendicular to motion of travel!
|
|
|
Term
|
Definition
|
transverse waves of electric and magnetic fields
|
|
|
Term
|
Definition
|
(h) Distance over which wave repeats itself
|
|
|
Term
|
Definition
|
number of crests that passes a point in one second (period of wave= 1/v)
|
|
|
Term
| Frequency versus Wavelength |
|
Definition
|
|
Term
|
Definition
|
collects light and bends light to a focus; pros: no central obstruction, great resolution/contrast... Cons: expensive, glass sags, size limit
|
|
|
Term
|
Definition
|
when focus might not refract all certain wavelengths the same, and you get different colors; stars with halos of red.
|
|
|
Term
|
Definition
|
two lenses of different glass to counteract the Chromatic Aberration
|
|
|
Term
|
Definition
|
invented by Newton; primary mirror collects light, cage at primary focus Pros: No Chrom. Ab., cheap, only one surface, can be supported from backside, no size limit....Cons: central obstruction, poor resolution and contrast
|
|
|
Term
|
Definition
|
uses flat secondary mirror to divert light to side
|
|
|
Term
|
Definition
|
Uses curved secondary mirror
|
|
|
Term
|
Definition
|
designed to align rotation of telescope with Earth's rotation axis; can attach a "clock" that moves telscope to counteract earth's rotation.
|
|
|
Term
|
Definition
|
Analogous to Longitude on the CS; increases eastward from Vernal Equinox (measured in degrees (360) or 24 hours)
|
|
|
Term
|
Definition
|
Latitude on celestial sphere; Celestial Poles have 90deg N/S Dec
|
|
|
Term
|
Definition
|
cheaper, dont align with rotation axis; requires computer control to follow stars, most large telescopes use this...
|
|
|
Term
|
Definition
|
|
Term
|
Definition
|
angle measured from North Cp toward East Cp (north to east...90 degrees....north to south....180....etc.)
|
|
|
Term
|
Definition
|
Photographic Plates (inefficient but cover large areas of sky) Charge-coupled device (CCD)(used by modern instruments)
|
|
|
Term
|
Definition
|
total light emitted by an object
L= 4pi x d^2 F where F(flux)= the amount of light that passes through a unit area
|
|
|
Term
|
Definition
|
brightness of a star located 10 Parsecs away.
|
|
|
Term
| (m-M) (Apparent Magnitude-Absolute Magnitude) |
|
Definition
|
|
Term
|
Definition
|
used to measure the distance to an object (also known as Triangulation)
|
|
|
Term
|
Definition
|
used to measure distance to stars; only used on nearby stars. d=1/p (p-parallax in arcseconds)
|
|
|
Term
|
Definition
|
|
Term
|
Definition
|
Annie Jump Cannon, OBAFGKM (high temp to low temp)
|
|
|