Open science archive // Stellar spectroscopy // Exoplanetary chemistry

Reading the chemistry
of other worlds

A systematic archive documenting the elemental chemistry of exoplanetary systems — measuring what stars are made of, and using that chemistry to understand what their planets are made of too.

Janssen (55 Cnc e) artist's concept — NASA, ESA, CSA, J. Olmsted (STScI) · JWST 2024
First target
55 Cancri A
IAU name
Copernicus
Distance
40.9 ly
Teff
5196 K
Planets
5
Spectrograph
HARPS R~115k
Model
ATLAS9 / Kurucz
Search the codex

Currently indexed: 1 system (55 Cancri / Copernicus) · More systems added as analysis completes

● Entry 001 — Analysis in progress
Copernicus
55 Cancri A · HD 75732 · HIP 43587

A metal-rich K dwarf 40.9 light years away hosting five planets, including Janssen — a lava-covered super-Earth with CO₂ atmosphere detected by JWST. The C/O ratio of this star remains scientifically contested. We are measuring it.

Teff5196 K
[Fe/H]+0.32
Planets5
Age10.2 Gyr
Step 1 / 6 — Spectrum acquisition
● Entry 000 — Reference system
The Sun
Sol · Our solar system · 8 planets

The calibration anchor for all Codex measurements. Every [X/H] abundance is measured relative to the Sun. Includes Terra, the reference case for all CHNOPS and habitability assessments.

Teff5778 K
[Fe/H]0.00
Planets8
Age4.6 Gyr
Reference data — Lodders 2003 / Asplund 2021
○ Queued — Thesis revisit
HD 89307
G0V · Solar analog

The most solar-like exoplanet host star known. First analyzed in the 2010 thesis that started this project. Now revisited with HARPS at 3× the resolution.

○ Queued — Thesis revisit
Gliese 581
M3 dwarf · Habitable zone planets

Two planets in the habitable zone. Analyzed in 2010 with poor model fit — M-class stars are hard. The 2026 pipeline will settle whether the anomalous Ni, Co, Si were real or an artifact.

○ Future
Submit a system
Suggest a target

Researcher with a system you'd like analyzed? Collaboration welcome. Contact us with your target and scientific rationale.

[λ]
High-res spectroscopy

HARPS spectra at R~115,000. Each absorption line in the stellar photosphere is a fingerprint of one element at one temperature and pressure.

[∫]
Equivalent widths

Gaussian fitting to absorption lines yields equivalent widths — the area of each line — which map directly to elemental column densities.

[K]
Kurucz model atmospheres

ATLAS9/Castelli-Kurucz 1D LTE model atmospheres parameterized by Teff, log g, [Fe/H], and microturbulence. The same workhorse used since 1979.

[σ]
Metrology-grade errors

Type A (random) and Type B (systematic) uncertainties documented for every measurement. Error bars are not optional — they are the science.

"This started as a senior astrophysics thesis in 2010 — three star systems, hand-fitted Gaussians, and a question: can you read the chemistry of a star and know what its planets are made of? I spent fifteen years building lasers and consulting on AI. The question never went away."
— Ryan Schmitt, founder  ·  Montana, 2026

First results coming soon

We're measuring 55 Cancri A now. Get notified when the first Codex entry publishes.