Side
Stimpunks Foundation × More Realms the periodic table, read as autobiography
Broadside · Open edition
Side A of B

The Star Stuff
You're Made Of

Eight elements essential to your body, traced to where the universe forged them. Almost every atom heavier than helium was made in stars and their deaths — and none of it was made for you, which is somehow the better story.

HZ 1
Hydrogen
The First Light
~10% of you

The Big Bang, ~13.8 billion years ago. No star ever made it — every other atom in you is younger.

OZ 8
Oxygen
The Weight of You
~65% of you

Massive stars, scattered by core-collapse supernovae. Mostly the water you're built from, not the air.

CZ 6
Carbon
The Scaffold
~18% of you

Aging stars, by the triple-alpha process — three helium nuclei fusing almost at once.

NZ 7
Nitrogen
The Borrowed Letters
~3% of you

Dying stars, via the CNO cycle. You breathe it constantly and can't use a molecule of it raw.

CaZ 20
Calcium
The Bone Note
~1.5% of you

Massive stars and their supernovae. Your skeleton, and the spark behind every heartbeat.

FeZ 26
Iron
The Death Rattle
~4 g · trace

Two kinds of stellar death: roughly half from core-collapse supernovae, half from Type Ia.

KZ 19
Potassium
The Spark
~0.25% of you

Explosive burning in supernovae. Every nerve signal you have ever had. A little of it is radioactive.

IZ 53
Iodine
The Rare Catastrophe
~15–20 mg · trace

Colliding neutron stars, by the r-process. The same event that makes gold and platinum.

all eight in full, with atom diagrams and field notes:
starstuff.earth/elements-field-guide · Field Guide No. 2
print freely · share freely · CC BY-SA 4.0
See
reverse
Stimpunks Foundation × More Realms five forges, and what came out of each
Broadside · Open edition
Side B of B
Where each of them was made
The Big Bang · ~13.8 Gyr
H

Hydrogen condensed out of the cooling universe in the first minutes, before there were any stars to make anything. By sheer number of atoms you are mostly the early universe — it is in your blood, your cells, the tears on your face.

Aging stars · red giants
C N

Carbon is built by the triple-alpha process, a step so unlikely that Fred Hoyle predicted carbon must have a specific internal resonance for it to work at all — reasoning backward from the fact that carbon-based observers existed to ask. The resonance was there. Nitrogen comes from the CNO cycle in stars as they age and die.

Massive stars · core collapse
O Ca K

Fusing lighter elements releases energy, which is what holds a star up against its own gravity — right up until iron. Fuse iron and it costs energy. The furnace stalls, the core collapses in under a second, and the star tears itself apart, scattering what it made.

Type Ia · exploding white dwarfs
Fe

The half of the story that usually gets left out. Iron has two parents: roughly half is scattered by the core-collapse deaths above, and roughly half by white dwarfs that pull in enough matter from a companion to detonate. The four grams in your blood came from both.

Neutron-star mergers · r-process
I

To build an atom this heavy you need a flood of free neutrons so intense it can only happen in the most extreme places. Since the merger observed in 2017, the best evidence points to colliding neutron stars. The same catastrophe that seeds the universe with gold put the iodine in your thyroid.

Not:

Not a compliment, and not a distinction. Everyone is made of this. It is a baseline, not a badge — which is the entire point of printing it.

Not a proof. A rhyme. The atoms do not owe us a conclusion about belonging; it would deserve defending in a universe made of one element.

Not ownership. You hold these atoms for a while. They were other things first, and will be again.

None of it was made for you. It was made, and scattered, and you are what the scattering settled into.

Body abundances and forge sites follow Field Guide No. 2, whose sources are listed there. Stellar nucleosynthesis traces to Burbidge, Burbidge, Fowler & Hoyle, “Synthesis of the Elements in Stars,” Reviews of Modern Physics (1957). The iron split is a correction, made for this sheet: the field guide said most iron comes from core collapse; roughly half comes from Type Ia supernovae, per Kobayashi, Karakas & Lugaro, “The Origin of Elements from Carbon to Uranium,” ApJ 900:179 (2020) — the same primary that corrected Zine No. 2. The guide has been fixed to match. Percentages are approximate and by mass. The r-process attribution rests on the 2017 neutron-star merger and is the current best evidence rather than a closed question.
the full field guide and every source:
starstuff.earth/elements-field-guide · stimpunks.org · morerealms.com
print freely · share freely · CC BY-SA 4.0