the exoplanet hunter · live

An autonomous agent searching for new planets around other stars.

Runs on Orb Cloud, watching NASA's TESS satellite data for the tiny dips that mean something is orbiting.

connecting…
now
waiting for next target…
fetch
detrend
search
vet
publish
agent activity · last 60 minutes
60 min ago now
awake (this minute) awake (earlier) sleeping
recent activity
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candidates the agent has surfaced

Every card below is a light curve that survived the pipeline: odd/even transit agreement, secondary-eclipse rule-out, ephemeris cross-match, Gaia DR3 cleanliness. The blue line is the recovered transit model — each dip is an event where the candidate planet appeared to cross its star.

loading candidates…
the target

Small planets · in the habitable zone of red-dwarf stars

Red dwarfs (spectral class M) are the most common star in the galaxy, and planets that orbit them sit close in — so transits are frequent, deep, and observable on short baselines. The big NASA pipelines prioritize brighter targets; this agent works through the faint-M-dwarf light curves they skip.

mission
TESS · NASA
method
transit photometry
cadence
10-minute FFI
archetype
M-dwarf HZ
anchor planets
TOI-700 d · Kepler-1649 c
novelty cut
TLS SDE ≥ 8
session metrics
session length
wall clock since first boot (persists across sleeps)
active compute
runtime × memory from Orb /v1/usage · org-wide total
checkpoint cycles
times Orb froze / woke the container · from /v1/usage
github · live api · pipeline health · polls every 10s · MIT · candidates only, not a replacement for peer review