Test 2 Flashcards
What are the 2 fundamental motions that affect us?
- Rotation on its axis
- Revolution around the sun
What does the Earth’s rotation control?
= controls our day / night
What does the Earth’s Revolution around the sun influence?
= controls the summer/winter
Summer:
=closer to sun
- longer sunlight
Winter:
= farther from sun
- sunlight is diffused
MIDTERM: What are the 3 Properties that fluctuate?
- Tilt
- Eccentricity
- Axel Precession (“Wobble”)
Definition: Tilt
“a metronome”
- oscillates between 22.2 and 24.5 degrees
1 cycle takes 41 000 years
= in phase between hemispheres
MIDTERM: how long is 1 cycle of Tilt
= 41, 000 years
What is our current tilt? is it increasing or decreasing?
23.5 degrees
= decreasing (tilt is getting more vertical)
Definition: Eccentricity
“more circular / elliptical”
= sometimes closer and farther to sun
=how elliptical is the earth’s orbit around the sun
- may be due to the Gravitational pull of Saturn and Jupiter
Controlled by 2 dominent periodcites:
- 100,000 and 413,000
MIDTERM: How long is 1 cycle of eccentricity?
100,000 years
Definition: Axel Precession
= wobble on the axis
Period: 23, 000 years
= out of phase between hemispheres
MIDTERM: How long is 1 period of Precession?
23, 000years
MAX Tilt + Precession coincide with Perihelion or Aphelion?
Perihelion = closest to the sun
Where can you find MAX Warming?
- in the N hemisphere
= when the summer solstice coincides with perihelion - MAX Tilt + precession
What do the 3 fluctuating properties result in?
= these result in a shift in position of the equinoxes (and solstices) around the Earth’s orbit every 23,000 years
What happens every 23,000 years?
= the shift in the position of the equinoxes (and solstices) around the Earth’s orbit
results in a differing amount of sun in the summer
= precession
Definition: Aphelian
= when the Earth is in the farthest position from the Sun
Definition: Perihelion
= when the Earth is in the closest position towards the sun
What is the importance of orbital properties?
= these determine how much radiation is received
Definition: Insolation
= Radiation received at the top of the Earth’s atmosphere
Units: Watts per square metre (W/m2)
T/F: The N/S Hemisphere gets more sunlight all year round and the Equator gets more short term
FALSE
The Equator gets more sunlight all year round
The N/S Hemisphere gets more short term sunlight
____ has a stronger affect at higher latitudes than ____
a) Tilt
b) Precession
Tilt has a stronger affect at higher latitudes than Precession
Out of tilt, precession, and eccentricity, which is the least important?
Eccentricity = least important
- approximately 0.2% incoming solar radiation
- small difference in sunlight
Tilt + Precession:
- approximately 10% difference in long-term mean
Tilt is in phase / out of phase between hemispheres?
In phase
T/F: Tilt affects the N/S hemispheres differently.
FALSE: It affects both hemispheres equally
Both hemispheres get hotter when they face the sun