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Life Factory

Nucleo synthesis - the material of life

The making of the nucleus


BIG BANG

t=0

Universe is a super, super hot plasma. 

  • Protons and neutrons form. 
  • Too hot for atoms — nuclei only.

∙ ~74.99% Hydrogen (1 proton)…

∙ ~24.99% Helium-4 (2 protons, 2 neutrons)…

∙ Trace Lithium-7…

∙ Trace Beryllium-7 (decays to Lithium)…

The universe cools too fast for heavier elements to form

0.007 strong nuclear coupling constant…

  • it governs the binding of all nuclei…

H, He, Li

t+3 minutes

……………dark ages………400,000 years……………………

  • Universe cools enough for electrons to bind to nuclei — first atoms…
  • No stars yet…
    • Just gas…
    • And 3 elements- H, He, Li…
    • Hydrogen and helium clouds drifting in darkness…

…………first stars………100 - 200 million years…………

  • pi, the gear ratio of all circular motion; all motion…
  • Gravity pulls hydrogen into rotating clouds, orbiting; equations based on pi…
  • First Stars ignite…
  • Massive - 100 times our sun…
    • Compression…
    • hot, bright, burns the candle at both ends…
      • don’t last long…

1st Generation stars

  • Stellar fusion begins...
    • the element factory… 92 in total

Each element requires higher temperatures…

 - produces heavier elements:

Each step up the element weight ladder releases energy, causing the star to heat up further for the next element, until

  • Iron
  • because fusing iron
  • consumes energy instead of
  • releasing it…
  • The star can no longer support itself…

And goes…

BANG

  • Explosive nucleosynthesis…

Supernova & neutron star mergers…

∙ r-process: rapid neutron capture

    • In seconds…
    • nuclei are bombarded with neutrons so fast they can’t decay between captures. 
    • Builds the heaviest elements: 
      • gold, platinum, uranium...

Red giant stars

  • Before the bang, in their red giant twilight…

∙ s-process: slow neutron capture 

    • over thousands of years…
    • Neutrons absorbed one at a time with gaps between.
    • Makes some intermediate heavy elements: 
      • barium, lead, strontium…

2nd Generation Stars and Planets

New clouds form from the enriched debris. Enriched with the debris of first generation supernovae…

  • now containing carbon, oxygen, iron, and heavier elements...
  • These stars, with gravity, build planets...
  • Rocky planets...
  • Chemistry becomes possible...
  • Molecules form...

The ingredients for life are in the mix, but not yet cooking…


3rd Generation Stars and Planets

Our sun is a third-generation star (even 4th or 5th see Appendices)…

  • it contains elements that could only have been made in previous supernovae…
  • the Earth condensed from the same debris cloud...
  • Every element heavier than lithium in our bodies was made inside a star that died before our sun was born…

The supply chain of life…




The death of stars is for the life of us…

  • they live on… through us..

Appendix 1

Our sun won’t go bang. It’s too small for a supernova…

  • minimum for BANG is about 8+ solar masses…
    • Our sun is a lightweight…
    • one solar mass…

What will happen in about 

5 billion years:

∙ Hydrogen fuel in the core runs out…

∙ Core contracts, heats up…

∙ Outer layers expand into red giant phase…

∙ Sun swells to engulf Mercury, Venus, probably Earth…

∙ Helium fusion begins in the core makes…

∙ carbon and oxygen…

∙ Outer layers puff off as a gorgeous planetary nebula…

∙ Core remains as a white dwarf…

  • a dense ember of carbon and oxygen, 
    • cooling for eternity
    • No bang. 
      • A sigh…

Just a slow, beautiful exhalation…of C and O… nearly co2…


Appendix 2

Astronomy actually counts star generation backwards; probably to avoid begging the question…

  • “…and then what happens to ‘0’ population stars?”…

The terminology is…

Population III = first generation stars

  • hydrogen and helium only, no metals…
  • Never directly observed…
  • Probably all massive…
    • all dead…
      • all exploded long ago…

Population II = second generation 

  • low metallicity, old…
  • Found in galactic halos and globular clusters...
    • 10-13 billion years old…

Population I = third generation +

  • high metallicity, young…
    • Our sun is Population I…
      • Contains heavy elements from (many) previous generations’ supernovae…

Our sun is considered a 

  • third, fourth, or possibly fifth generation star…
    • based on its high heavy element content…which
      • requires multiple cycles of stellar birth and…
        • death to accumulate…

The generation count is broad brush because gas clouds don’t always know which gen they are and get confused…as

  • each new star forms from a blend of debris in the star nursery, the nebulae, from many predecessors, not a single parent star. 

It’s a mulch, a pig’s breakfast, a paddy’s parliament…


Appendix 3

Lithium is element 3, one of the 

  • ‘ancient’ trinity, with H and He, harry and hetty…and li’l puff
    • in the first 3 minutes…
      • Not in stellar fusion…

li’l puff because that’s what happens to lithium in star forges; it turns to ‘puff’…

So, free range lithium is a refugee from the big bang, a victim of genocide by stars…plus small amounts made by cosmic ray spallation — the same process that makes boron and beryllium…

This is why lithium is relatively rare despite being element 3…

  • the universe made it first and has been destroying it ever since…
  • The oldest element that’s been running from its own creator for 13.8 billion years…
  • And now we mine it for batteries...to meet its creator…

The element that survived the Big Bang and billions of years of stellar destruction ends up in my iPad...

  • so I can write its eulogy…

Appendix 4

Atomic number

Atomic number, not atomic weight

  • runs from 1 to 92.

Atomic number = the number of protons in the nucleus. 

  • this defines the element…
    • Hydrogen has 1 proton…
    • Helium has 2…
    • Lithium has 3…
      • Carbon has 6…
      • Iron has 26….
      • Uranium has 92…

The atomic number IS the element’s identity…

So, the fusion ladder in climbing atomic numbers:

∙ Hydrogen: 1 proton

∙ Helium: 2 protons

∙ Carbon: 6 protons

∙ Neon: 10

∙ Oxygen: 8

∙ Magnesium: 12

∙ Silicon: 14

∙ Sulphur: 16

∙ Iron: 26

Notice the jumps aren’t sequential 

  • Hydrogen to helium is 1→2. 
    • helium to carbon is 2→6 (three heliums fusing). 

The triple alpha process skips 3, 4, 5 entirely…


Not a product of stellar fusion…in fact.. destroyed by it…are…

∙ Lithium: 3 protons

∙ beryllium: 4 protons

∙ boron: 5 protons…

The 92 naturally occurring elements fill atomic numbers 1 to 92, but the universe didn’t make them in order. 

It made them by whatever fusion or neutron capture process the physics allowed, skipping around the periodic table like a jazz musician, not a scales player.​​​​​​​​​​​​​​​​


Atomic weight

Atomic weight (or atomic mass) is different…

  • it’s the total number of protons plus neutrons. 
  • This varies because elements can have different numbers of neutrons (isotopes). 
  • Carbon-12 has 6 protons + 6 neutrons = atomic weight 12.
  • Carbon-14 has 6 protons + 8 neutrons = atomic weight 14. 
  • Still carbon 
    • same atomic number, different weight.
  • Lithium-7 (the most common isotope from the Big Bang) has 3 protons + 4 neutrons = atomic weight 7…see in graphic above…
  • Lithium-6 has 3 protons + 3 neutrons = atomic weight 6. Rarer…
  • Both are lithium because both have 3 protons.
    The neutron count changes the weight but not the identity.​​​​​​​​​​​​​​​​..

Appendix 5

Heat death of the universe

In about 10^100 years a googol,

  • the Internet will still be running as Google;
  • all hydrogen will be consumed…
    • no new stars can form...
    • Existing stars burn out...
    • White dwarfs cool to black dwarfs...
    • Neutron stars fade...
    • Black holes evaporate via Hawking radiation...

The universe reaches maximum entropy 

    • uniform temperature, 
      • no energy gradients…
      • no work possible...
      • No structure...
      • No chemistry...
      • No life…
        • cold, dark…
          • expanding nothing...

The Life Factory has closed its doors…

Permanently…