System Earth Ch 12 Flashcards

(55 cards)

1
Q

What is the young sun paradox?

A

the fact that the earth must have been warm enough for liquid water to exist throughout its history but that the sun used to be 30% less bright

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2
Q

why has the sun’s brightness changed over time?

A

luminosity increase is due to a change in density caused by the conversion of hydrogen into helium.

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3
Q

what does it mean that luminosity change for the sun is a robust model?

A

does not depend sensitively on the details of the model - the specifics may be different but the core of the issue will not go away.

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4
Q

How well do we understand the sun?

A

turns out, pretty well. We have found out that it emits neutrinos in a type that went unmeasured for a very long time. This is how the sun produces energy.

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5
Q

how does teh sun loose mass?

A

solar wind - outflow of charged particles from the sun’s corona. There us also a rapid rotation which with the magnetic field heats up the star’s corona, driving a stellar wind.

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6
Q

Can we calculate the faint young sun paradox mathematically?

A

yes, you can look at 30% decrease in luminosity -> 22 degrees temperature change and do your maths from there, while including feedback loops.

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7
Q

what are the three possible solutions to the faint young sun paradox?

A
  1. planetary albedo was lower in the past.
  2. larger GHE
  3. additional heat sources present.
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8
Q

geothermal heat?

A

heat produced by the decay of radioactive elements in the Earth’s crust and mantle.

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9
Q

what is the problem with the geothermal heat flux?

A

it is not enough. It would have been enough to keep deep ocean warm but not the top from freezing.

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10
Q

why is albedo not a solution to the faint sun paradox?

A

the albedo would have had to be near 0 which is impossible.

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11
Q

what is probably the solution to the faint young sun paradox and which options are wrong?

A

enhanced GHE but it could not have been water vapour alone. Ammonia is also not an option

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12
Q

Why were there more reduced gases in the atmosphere prior to 2.4 By ago?

A

This was before an oxygenated atmosphere. So ammonia could have been present were it not for ultraviolet radiation.

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13
Q

is CO2 an option for the faint sun paradox?

A

with the silicate, carbon cycle, it is definitley a possibility. We would have needed 1000 times current levels, but this is quite possible.

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14
Q

serpentinization

A

serpentine minerals are formed in a reaction with watera nd iron and magnesium- rich basalts. If CO2 is in the water, methane is formed.

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15
Q

early form of bacteria?

A

methanogenic bacteria

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16
Q

why is the sky blue

A

scattering of sunlight by N2 and O2 molecules - Rayleigh scattering

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17
Q

What is Rayleigh scattering

A

when the shorter wavelengths are scattered preferentially to long wave. So we see a blue sky

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18
Q

Mie scattering

A

scattering particles that are close in size to the wavelength.

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19
Q

thermophile

A

organisms with optimum temp between 40 and 80

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20
Q

hyperthermophile

A

organisms with optimum temp above 80 degrees

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21
Q

organic haze effect

A

the temperature decreases due to the anti greenhouse effect.

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22
Q

deep sea cores

A

go back 200 My

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23
Q

oxygen isotopes

A

look at carbonate rocks. but may have been influenced by other processes such as a change in seawater compositon.

24
Q

tillites

A

mixtures of cobbles, pebbles, and and mud that have been packed together to form rocks.

25
moraines
terminal point or flank of a glacier
26
dropstones
misplaced chunks of rocks that you find in laminated areas
27
Huronian glaciation
2.3 By ago radiometiric age dating glacial deposits uranite deposits HIGH O2
28
warm period after huronian glaciation
probably due to weathering
29
Late protozoic glaciation
Australia at the equator and covered in ice. high incoming radiation enhanced weathering, reduced CO2 all continents at the equator fewer glaciers - more weathering. potential snowball earth
30
snowball earth graph
you have stability points you have to force to get there.
31
Phanerozoic eon
permo carboniferous sufficient O2 to prevent CH4 accumulation carbon burial rate doubled - formation of coal beds atmospheric CO2 based on paleosol data -> decreased CO2 - ice ago triggered.
32
vascular plants
can help enhanced weathering but would not have occured in carboniferous - there were no vascular plants at that point.
33
warm mesozoic era
dinosaurs! deep ocean was 12 K warmer than today. higher CO2 look at 12C ratio reversed thermohaline circulation with upwelling at poles. more efficient hadley cell circulation
34
paleomagnetic data
efficient seafloor spreading - faster spreading - enhanced CO2 production.
35
12-C and 13-C
plants and plankton take up 12-C more than 13-C. low 13/12 shows photosynthesis produced OM under elevated CO2 more 13-C => less 12-C in atm.
36
paleo-eocene
isotopic info low 13C Thermal Maximum 55My ago 25 degrees at poles aerosol cloud mechanisms methane aerosol forcing
37
Cenozoic climate
india collides with asia weathering increases and high albedo very active but quite slow first formation of ice sheet 35 My ago delta 18O => cooling conditions
38
Last 1.8M y
are there different mechanisms or do we have much more data? resolution has increased by factor of 10
39
Pleistocene glaciation
land/sea distribution similar long term trend - we are heading towards a glaciation
40
positive delta 18 O
cold conditions
41
how has peiodicity changed in the last 100kyr?
it has become in line with Milankovitch cycles
41
eccentricity
oval or circular orbit - 100kyr
42
obliquity
tilt - 40 kyr
43
precession
spinning top - 26 kyr
44
Q1. why does the sun get brighter with time?
luminosity increases with density change
45
Q2. how migh tcarbon silicate cycle helped save the faint young sun paradox?
the negative feedback loop kept the global temperature in check.
46
Q3. methan in Archaen era?
kept the planet warm and methanogenic bacteria
47
Q4. What triggered the Huronian glaciation?
Great Oxygenation Event
48
Q5. Types of geologic evidence used to infer past glaciation?
deep sea ice cores and oxygen isotopes
49
Q6. How many separate periods of glaciation have occurred in Earth's history?
5
50
Q7. What types of geologic evidence support snowball earth model?
location of continents and evidence on Australia
51
Q8. carbon isotopes?
13C is high in plants - lower 12C in atmosphere. Plants take up12 more easily
52
Q9. atmospheric CO2 and plants
photo and respiration
53
Q10. What mechanisms explain warm climate of mesozoic era?
thermohaline circulation. high CO2 ratio and efficient hadley cell circulation.
54
Q11. Why has the climate cooled in the last 40M y?
India collided with Asia and then weathering.