midterm Flashcards
what are the 4 spheres?
hydrosphere
biosphere
lithosphere
atmosphere
what is the difference between: galaxy, universe and solar system?
Galaxy: collection of thousands to billions of stars held together by gravity
Universe: all of space and time
Solar System: a set including a star and the matter that orbits it including planets, moons, asteroids, comets, and other object
what is geography?
‘study of the relationships among natural systems and processes, geographic areas, society and culture over space
what is a system? closed and opened
–set of ordered components linked by flows of energy and matter, distinct from surrounding
open: not self contained (river)
closed: self contained (aunt colony)
map projections:
Cylindrical: preserves shape but not area (Mercator)
Conic: preserves area but not shape (Gnomonic)
Planar/Azimuth: doesn’t preserve either (Albers equal- area)
Milky Way Galaxy
collection of stars and gasses
-50 billion planets
flatted disc shaped
Perihelion
Aphelion
Perihelion- closest to the sun (Jan 3rd)
Aphelion- furthest away from sun (July 4th)
Sun
star in the Galaxy
Energy source for Earth
Our Solar System
planets orbit the Sun in elliptical path (plane of ecliptic)
Fusion
reactions between hydrogen nuclei that release large amounts of energy
Sunspots
sun experiences magnetic storms –> sunspots
have lower temp than surroundings
11 year activity cycle
Solar Winds
Sunspots can produce solar winds
clouds of electrically charged particles
Magnetosphere deflects solar wind poleward
The Earth’s farthest position from the Sun can be described as:
Aphelion
electromagnetic spectrum
solar energy occupies part of the electromagnetic spectrum
electromagnetic radiation
energy that travels in waves
short wavelength
higher energy, higher frequency, higher temp
longer wavelength
lower energy, lower frequency, lower temp
Wien’s displacement Law
objects radiate energy in __ related to their energy
Blackbody radiator
perfect absorber of radiant energy
insolation
solar radiation intercepted by Earth ( incoming solar radiation)
solar constant
average insolation @ the top of the atmosphere
subsolar point
location where insolation is perpendicular to the surface
migrates between 23.5 N and 23.5 S
Net radiation
incoming shortwave- outgoing long wave
Seasonality
seasonal variation in the Sun’s position above the horizon and changing daylight
Reasons for seasons
revolution rotation tilt axial parallelism sphericity
revolution
earth revolves around the sun
length of voyage: 365 days
earth’s orbital speed