Lecture 6 - Marina Isotope Record Flashcards
isotopes
stable isotopes of carbon
12C and 13C
- do not break down in any other way
- useful because they behave differently in ecosystems
isotopes
stable isotopes of oxygen
16O - common, light (8P, 8N)
18O - rare, heavy (8P, 10N)
microorganisms & chemical clues
how do microorganisms give chemical clues
skeletons made using CaCO3, in shallow oceans limestone sedimentary rocks deposited from skeletons of these organims
- chemical sed rock = long term tombs for microorganisms
microorganisms & chemical clues
steps of hydrolgic cycle
during non-glacial periods
- water evaporates and makes clouds
- some rain, all the water rains back down into the ocean
- complete cycle
during glacial periods
- water evaporates and makes clouds
- rain over land, snow over glaciers
- glacier snow never makes it back to ocean
- sea level goes down
- ice becomes light isotope rich and leaves 18O enriched sea water
microorganisms & chemical clues
why does 16O get carried into clouds and leave 18O behind
takes more heat energy to melt heavy oxygen
massive international effort
deep sea drilling project
1968-1983
- ocean drilling program: 1985-present
- drills in deep sea come up with sedimentary cores
- can get precise recordof O2 records in the sea
cyclical changes in solar energy
differences in how much solar energy hits the earth at given periods
obliquity - axial tilt
what is it, why is it important
Earth does not spin vertical, but on tilted axis
- also wobbles back and forth (btwn 22.1 and 24.5 degrees)
- gives cause to season, part of earth tilted towards sun = summer
- more extreme tilts means more extreme winters/summers
obliquity - axial tilt
pattern of obliquity
increase obliquity affects poles
- increases seasonal differences
- 41k year cycle btwn relative min and max, cycles don’t always go to the extremes
axial precession
axial precession
earth spins on axis at tilt, and wobbles
- wobble results in “The Precession of Equinoxes”
axial precession
what are equinoxes
equal illumination on N and S hemispheres
- autumn and spring
axial precession
what are solstices
Earth’s axis pointed toward or away from Sun
- summer, pointed directly for N hem
- winter, pointed away for N hem
- as axis wobbles, changes point of orbit during which pole pointed towards sun
axial precession
occurence of precession
periodicites of 23k and 100k
- increases and decreases seasonality, currently N Hem seasonality reduced
what is eccentricity
how much of a circle vs oval the orbit is
- season in elongated part of the orbit lasts longer
- can amplify effects of precession
- periods of 100k and 413k
Miankovitch Cycles
eccentricity, axial precession, obliquity
- all are mathematically defined through analysis of orbit
- periodicity is very regular
- have profound effects on cycles in Earth’s climate