What is the Exoplanet Detective multi-solver?

Exoplanet Detective is a guided workflow that chains 2 individual PolySim solvers into one end-to-end analysis, piping each result into the next step.

Yes. Every step runs entirely in your browser using real numerics — no install, no account, no cloud cost. Custom or private solver packs are available as a paid service.

Biology & Aerospace Pack · Multi-Solver

Exoplanet Detective

Transit to mass. This multi-solver chains 2 solvers into a single guided workflow — run each step in order and carry the result forward.

Workflow steps

or unlock everything with Pro →

Exoplanet Transit

open full solver →

Exoplanet TransitLive

the transit method · light curves

Controls

Speed1×

Presets

Planet/star radius (Rp/Rs)

Impact parameter b

As a planet crosses its star, it blocks a tiny fraction of the light — a dip of depth (Rp/Rs)². This is how Kepler and TESS have found thousands of exoplanets. Impact parameter sets how centrally the planet crosses, changing the transit shape and duration. Drag the planet across the star to set its phase, or up and down to set the impact parameter — the light curve updates live.

▶ Run in Python

Data Inspector

Transit depth1.00%

Rp/Rs0.10

Impact b0.20

Governing equation

\frac{Δ F}{F} = (\frac{R _{p}}{R _{⋆}})^{2} = (0.10)^{2} = 1.00%

Reading this result: The dip depth is almost exactly (Rp/Rs)², so measuring how much light is blocked directly gives the planet's size relative to its star. The width of the dip is the transit duration, which — combined with how often it repeats — follows from the planet's orbital period and speed across the disk.

Runs locally in your browser — free forever. Scale to the cloud when reality gets heavy.

↓

H-R Diagram

open full solver →

Hertzsprung-Russell DiagramLive

the map of the stars

Controls

Presets

Your star temperature (K)

The H-R diagram plots stars by temperature and luminosity, revealing the main sequence (a diagonal band), red giants, supergiants, and white dwarfs. Your star (pink ring) sits on the main sequence where luminosity scales as T⁴.

▶ Run in Python

Data Inspector

Spectral classG

Luminosity1.00 L☉

Temperature5,778 K

Governing equation

\frac{L}{L _{⊙}} = (\frac{T}{T _{⊙}})^{4} = (\frac{5778}{5778})^{4} = 1.00

Reading this result: A cool orange K-type star: lower temperature places it low-right on the main sequence, dimmer and longer-lived than the Sun.

Runs locally in your browser — free forever. Scale to the cloud when reality gets heavy.

Need a private, branded version?

We build custom solvers and workflows for labs, firms, agencies, and courses — your parameters, your branding, your data.

Explore Custom Solver Sets →

More in the Biology & Aerospace pack

Epidemic Response Model Pharmacokinetics Suite Neuroscience Lab Population Ecology Lab Tumor Growth Cardiac Rhythm Vaccine Strategy Enzyme Pathway

Frequently asked questions

What is the Exoplanet Detective multi-solver?: Exoplanet Detective is a guided workflow that chains 2 individual PolySim solvers into one end-to-end analysis, piping each result into the next step.
Is it free to use?: Yes. Every step runs entirely in your browser using real numerics — no install, no account, no cloud cost. Custom or private solver packs are available as a paid service.