On the Astronomy Final!
- The Night Sky
 - Altitude & Azimuth
 - Horizon
 - Zenith & Nadir
 - Celestial Sphere
 - What it is
 - Diurnal/Annual Motion
 - Celestial poles – no diurnal/annual motion
 - Celestial Equator
 - Right Ascension/Declination
 - Ecliptic
 - Zodiac what it is, not every constellation
 - What is a constellation
 - Asterisms – be able to recognize them and their stars
 - Conjunctions/oppositions...inferior/superior planets
 - Seasons
 - Axial tilt 23° 27”...reason for seasons
 - Equinoxes and Solstices
 - What they are
 - Where they are on the Celestial Sphere
 
- History of Astronomy
 - Geocentric vs Heliocentric Models
 - Major proponents of each model
 - Eudoxus, Aristarchus, Ptolemy, Copernicus, Tycho, Galileo & Kepler
 - Problems with each model
 - Geocentric ...Retrograde motion of planets
 - Heliocentric ... lack of apparent parallax
 - Solutions to each problem:
 - (Geo) Epicycles.... increasing complexity
 - (Helio) That stars are unthinkably far away
 - Shape and Size of the Earth
 - Since Aristotle all “old world” people knew Earth was a sphere
 - 2-reasons:
 - Shape of Shadow of Earth on the Moon (in an Eclipse)
 - All stars not visible everywhere
 - Size of Earth
 - Aristarchus proves Sun is larger than Earth and Moon is smaller
 - Eratosthenes calculated the size accurately ca 250 BC!
 - Galileo’s Discoveries (using a telescope) and what they mean:
 - Confirming the Heliocentric Model
 - Size of Universe/Stars are Suns
 - Planets & Moons are worlds
 - Inertia
 - Kepler’s 3 Laws
 - Know the 3-laws
 - Solve a 3rd law problem
 
- Newton’s laws
 - 3 for Motion
 - Universal Gravity
 - All masses attract each other
 - Directly related to mass.
 - Obeys the inverse square law
 - How these laws affect Astronomy:
 - Surface Gravity
 - Orbits
 - Satellites are falling just missing the planet/star
 - Orbital Velocity
 - Speed and shape of orbit
 - Escape Velocity
 
- Optics
 - What Light is
 - Ray, Wave or Particle
 - Electro-magnetic waves
 - Wave-particle Duality
 
- Colors are different wavelengths/frequencies of light
 
- c = fλ (f & λ are inversely related)
 - Visible light λ= 400-700nm
 - Roy G Biv (increasing f)
 - White Light and a spectrum
 - The Electro-magnetic spectrum
 - Radio, Micro, IR, Visible, UV X-rays and Gamma Rays (Increasing f)
 
- Know the properties of the different EM-waves
 - which pass through the atmosphere
 - which are dangerous
 - Energy is directly related to frequency
 - Relationship between color and temp of stars
 - 3 types of Spectra
 - Photo-electric effect
 - Source of each type
 - Continuous ... Hot Solid/ high pressure Gas (star)
 - Emission Spectrum...bright lines...Hot Gas
 - Absorption Spectrum...dark lines...passed thru cold gas
 - E/A spectra act like elemental fingerprints
 - Doppler effect...Red & Blue Shifts.
 
- 5 ways light changes direction.
 
Reflection, Refraction, diffraction, scattering, gravity
- what each is
 - basic rules
 - Optical instruments
 - No optical effects, aberrations or image questions!
 
But know why reflectors make better big telescopes
- Telescopes
 - Properties of the parts of a telescope
 - Properties of the scopes
 - Properties of the image
 - How the three above are related
 - Types of telescopes
 
- What we’ve learned about the Earth
 - Numerical Stats: Radius, Mass Density, Orbital Radius
 - Layers of the Lithosphere
 - Composition of the Lithosphere
 
- Temperature Scales and Units
 - Know the 3 used Fahrenheit, Celsius and Kelvin
 - Zero on Each scale and Absolute Zero
 - Know what a Light-year, and an Astronomical Unit are
 
