Nuclides planetory redox

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Biogeochemistry Wk 1

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45 Terms

1
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What determines the chemical reactivity of an atom?

The arrangement of electrons

2
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What is the ‘valley of stability’?

A region where stable nuclides lie; unstable ones are high energy and lie either side.

3
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What are magic numbers in nuclear stability?

Nuclei with the Z and/or N of 2,8,20,28,50 and 126 are anamously stable are are magic.

4
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What is the difference even and odd Z numbered elements? 

  • Even Z typically have more stable isotopes than elements with odd Z

  • Odd Z tend to have nuclides with odd masses and even Z tend to have even masses

5
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What happens during beta decay?

A neutron emits an electron and anti-neutrino → increasing the atmoic number by 1

6
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What happens during positron emission?

A proton becomes a neutron, emitting a positron and a neutrino

7
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What happens during electron capture?

The nucleus captures an electron, converting a proton into a neutron.

8
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Why is 26Al important?

It has a long half-life and is used in early solar system chronology and exposure dating.

9
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What are gamma rays?

High energy photons emitted when a nucleus transitions from an excited to a stable state.

10
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Name 3 heavy isotopes with long-half lives.

232Th, 235U, 238U

11
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What is alpha decay?

Emission of a 4He nucleus which reduces the mass by 4 and atomic number by 2

12
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What is spontaneous fission?

A nucleus splits into two fragments without external stimulation

13
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Why is spontaneous fission significant?

It produces neutron-rich fragments that undergo multiple beta decays

14
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How are heavier elements formed?

Through stellar nucleosynthesis - fusion and neutron addition in stars

15
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What is galactic chemical evolution?

The process by which elemental and isotropc compositions change over time as matter cycles through stars

16
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Why are younger stars more metal rich?

As they contain more lements beyond H and He due to prior stellar generations

17
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What light nuclei formed minutes after the Big Bang?

2H, 3He, 4He, 7Li

18
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Why are nuclei with mass numbers 5 and 8 rare?

As they are highly unstable and radioactive

19
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What is the sun’s composition?

~73% hydrogen, ~25% helium, ~2% metals 

20
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Why are Li, Be and B scarce?

They are destroyed by fusion rather than created

21
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Why is Fe a local maximum in abundance?

It represents the peak of nuclear stability

22
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What is the mass defect?

The difference between the mass of reactants and products, converted into binding energy

23
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What prevents nuclei from fucing easily?

Electrostatic repulsion between positively charged nuclei

24
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Why is fusion of H to He fusion efficient?

Low repulsion and high energy field

25
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What happens when H is exhausted in small stars?

Core contracts → red giant forms → nebula formation

26
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What happens when fuel is exhausted in large stars?

Core collapse → super red giant → supernova → black hole/neutron star

27
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What process creates heavier nuclides?

Neutron addition (s-process and r-process)

28
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What is photodissociation?

Neutron loss bia high-energy gamma irradiation

29
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Where does the s-process occur?

In low-mass stars during hydrostatic burning

30
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What follows neutron addition in the s-process?

Beta decay to reach stability

31
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Where does the r-process occur?

In high-energy environments like supernoave or neutron stars

32
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What is the r-process?

Flux of neutron addition and once the flux stopped undergoes beta decay to become stable and form neutron rich nuclides

33
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What is the p-process?

Gamma-induced neutron loss - reverse of neutron gain

34
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Where does the p-process occur?

In high-temperature environments beyond the Fe peak

35
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Why is N2 abundnat in the atmosphere?

It’s chemically inert and poorly soluble so it remains afetr other gases are removed

36
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What governs volcanic gas speciation?

Mantle redox state and oxygen fugacity 

37
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What species dominate under low fO2?

Methane (CH4)

38
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What species dominate under high fO2?

Carbon dioxide (CO2)

39
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What is a redox buffer?

A mineral reaction that stabilises oxygen fugacity by counteracting changes in O2

40
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Name 3 redox buffers

  • IW (Iron-Wüstite),

  • WM (Wüstite-Magnetite),

  • FMQ (Fayalite-Magnetite-Quartz)

41
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What does the IW buffer involve?

Fe + ½O₂ ⇌ FeO — sets fO₂ when both phases are present.

42
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How does mantle composition affect IW buffering?

Activities of Fe and FeO are lower than pure phases, shifting fO₂ ~2 log units below pure IW.

43
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What drives mantle oxidation?

Iron disproprtionation in the lower mantle

44
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What is the thermal water trap?

A mechanism that retains water in the lower atmosphere by freezing it before it reaches UV- rich layers. Without it water would be lost to space

45
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Why does methane escape more easily?

It rises higher, undergoes photodissociation, and releases hydrogen radicals that excape Earth’s gravity.