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AI Exoplanet Detective | SmartCircuits
NASA KEPLER • SINGLE-FILE CLASSROOM PLATFORM • SMARTCIRCUITS

🪐 AI Exoplanet Detective

Use real NASA Kepler data to investigate transit signals and classify an object as a likely exoplanet candidate or a non-planet signal.

1. Enter a NASA Kepler object

Enter a KOI such as K00752.01. The platform looks up the NASA KOI record and then automatically tries to load a real Kepler light curve from the public MAST archive.

Accepted: 1.01, KOI 1.01, K00752.01
Ready.

2. Load the REAL Kepler light curve

Automatic: after NASA lookup, this page tries to find a public Kepler light-curve FITS file in the MAST archive and read it in your browser. If the browser blocks the archive, you can still upload a NASA FITS/CSV file manually.

Automatic mode reads the real Kepler FITS light curve. Manual CSV upload must contain a real light curve with TIME + FLUX/PDCSAP_FLUX values. A NASA KOI catalog CSV (kepid, kepoi_name, koi_disposition, etc.) is metadata only and cannot be plotted as a light curve.

Or paste NASA CSV data

AI / signal evidence

Repeated dip
Transit depth
Periodicity
Signal quality

📈 REAL Kepler Light Curve

Data points
Median flux
Transit depth
NASA status
AI / signal-analysis result
Waiting for real data
Load a NASA light curve to begin.

Important: A transit-like dip is evidence, not proof of an exoplanet. This browser classifier is an educational signal-analysis model. NASA's archive classification is shown separately.
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