Module 3 Flashcards
List the 4 most common elements in the bulk Earth
Fe, O, Mg, Si
Briefly describe how the solar system was formed, which types of elements ended, up in rocky and gaseous planets
condensation, accretion, element distribution
Solar system formed:
-giant molecular cloud
-gets denser -> gravitational collapse
-collisions produces heat
-High T. Sun, start fusion, H-burning
condensation:
-Centre of solar system was very hot, edges cold
-Hot nebular gases
-cool and solidify into solid grains of dust
-Solar wind drives volatiles to outer solar system
accretion:
-Dust grains join to become planets
-Produces planetesimals
-Planetesimals attract each other
-growth of planetary embryos
-Collisions between planetary embryos
-Volatiles stay gaseous longer (get further from sun), refractory solidify near sun
Rocky planets -> small amounts of volatiles
Gas giants -> rocky/icy core, high amounts of volatiles
Name the four most common types of meteorites and which parts of the Earth they are similar to
Carbonaceous chondrites:
-pre-planetary solar nebula composition
-reflects first solids formed in the protoplanetary disk
Achondrites:
-Fragments of differentiated
asteroids/planets
-Many are similar to igneous rocks
found on Earth
stony iron meterorites
-equal amount of Fe-Ni alloy and silicate minerals
-edge of core/mantle of differentiated
asteroids
-similar to earth core/mantle boundary
iron meteorites
-Fe-Ni alloy
-core of differentiated asteroids
-similar to the core of earth
Describe the four Goldschmidt classifications of elements, where they are on the periodic table (generally), the kinds of bonds they form and where they are concentrated in the Earth
chalcophiles
-cu-loving
-bond with s, form sulphides
-Cu-S, between sidero and litho
right side of table
-both core and crust/mantle depending on how metallic (dense) they are
lithophiles
-bond with si and o, form silicates and oxides
-alkali, halogens, lanthanides, left side of table
-crust, mantle
atmophiles
-gas loving
-form gas and liquid
-volatiles, noble gases
-atmosphere
siderophiles
-fe-loving (form native metals)
-middle transition metals
-dissolve in liquid Fe and sink to core
-core
Explain how the current chemical composition of the atmosphere developed
Started off high in H and He from sun
volcanic outgassing
evolution of oxygenic photosynthesis,
biogeochemical cycles
weathering
sedimentation
Has changed through time: gained N2 and O2; lost CO2 and CH4
What are the 3 kinds of dissolved ions in water?
What is the relationship between residence time and mixing time
Conservative
-Constant concentration in water column relative to salinity
Recycled
-concentration increases with deeper water depth
-Organisms take up nutrients in surface waters, die and sink, nutrients back to deep waters
- Scavenged (e.g. Pb, Mn)
-concentration decreases with deeper water depth
-Adsorb to surfaces of solid particles and sink into sediments
Residence time:
-time a single atom/molecule remains in reservoir of interest
conservative
residence time»_space; ocean water mixing time (1000 yr)
recycled or scavenged
residence time «_space;mixing time