Unit 2 - Radiocarbon Dating Flashcards

(11 cards)

1
Q

What are the naturally occurring isotopes of carbon?

A

^12C - 98.89%
^13C - 1.11%
^14C - 0.00000000010% (1 in 10^12)

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2
Q

How does cosmic radiation work?

A
  1. cosmic rays (from the sun) enter the earth’s atmosphere and collide with an atom, creating an energetic neutron.
  2. neutron collides with a nitrogen atom (replacing one of the protons), the nitrogen-14 turns into a carbon-14 atom.
  3. plats absorb the CO2 and incorporate Carbon-14 through photosynthesis.
  4. animals and humans eat plants, taking in carbon-14
  5. following death, wood and bones lose C-14 as it returns to N-14 via beta decay.
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3
Q

How to calculate number of nuclei at a certain time?

A

Nt = N0 x (1/2)^n

(number of nuclei at time t = initial number of nuclei x number of half lives)

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4
Q

What is the activity of a radioactive source?

A

The number of nuclear disintergrations per unit time occurring in a radioactive material

In the international system of units (SI), the becquerel (Bq) is the unit of radioactivity.

One Bq is 1 disintergration per second.
One curie is 37 billion Bq.

Since the Bq represents such a small amount, you are likely to see a prefix used with Bq:
1MBq (27 microcuries), 1GBq (27 millicuries), 37 GBq (1 curie), 1 TBq (27 curies).

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5
Q

Three ways to detect radiation

A

Ionisation (Geiger) counter
Scintillation counter
Accelerator Mass Spectrometry (AMS)

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6
Q

Scintillator detector

A

Effective at measuring gamma radiation.

the scintillator material emits light that is collected in photomultiplier tubes.

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7
Q

Accelerator mass spectrometry (AMS)

A
  • ultra sensitive isotope ratio mass spectrometry of small prepared samples
  • most advanced way of measuring C-14
    Isotopes typically measured include a handful of long-lived radioisotopes that are naturally lowly abundant due to their instability, yet difficult to measure by their infrequent decay.
    -ions are characterised by combined conventional mass spectrometry and high-energy collisions within the accelerator and in a final detector.
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8
Q

AMS vs Radiation counters

A

AMS:
- counts number of atoms in a sample
- AMS would give 1000 counts in 0.1 seconds.

Scintillation counter:
- measures the infrequent radioactive decay events in the sample ]
- counts would take 5 days.

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9
Q

Calculating dates

A

Relationship between the rate of decay and the number of radioactive nuclei (N)

K is the decay constant and is characteristic of the radionuclide.

Activity = rate of decay = k x N

(Activity proportional to number of nuclei)

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10
Q

Exponential decay

A

Radioactivity follows an exponential decay

The number of nuclei (N) remaining after time t is given by : N = Noe^-kt
Where No is the number of radioactive nuclei present initially, at t = 0.

N and No can be measured in number of nuclei or mass present (as proportional to number of nuclei) or as activity.

(Intereted in ratio so units doesn’t matter)

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11
Q

cosmic rays

Give the formula for the nuclear reaction that creates C-14 in the atmosphere

A

(14:7)N + (1:0)n -> (14:6)C +(1:1)H

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