JWST Spectral Archaeologist

Observatory Online — Target: K2-18 b

Select Target Exoplanet

K2-18 b

Habitable Zone Candidate
124 ly
2.61 R⊕
8.63 M⊕
255 K
Red Dwarf (M2.5 V)
2015

JWST Key Findings NIRISS · NIRSpec

  • Carbon-bearing molecules CH₄ and CO₂ detected (2023)
  • Low NH₃ / CO abundances — consistent with an ocean under a H₂ envelope
  • Tentative dimethyl sulfide (DMS / DMDS) signal reported (2025) — unconfirmed

Observation Parameters

Quick Look Deep Field

📡 Spectral Decoder — Transit Spectroscopy

0.20.40.60.811 μm2 μm3 μm4 μm5 μmWavelength (μm)Relative Flux

Toggle Molecular Signatures

9.2
5

🌑 Transit Simulator

⚫ Out of Transit — Baseline
0.000%
0.0°

🌍 Habitability Assessment

100Score
Promising Biosphere Candidate
40/40
25/25
30/30
15/15
77%
⚠️ Tentative Biosignature

A dimethyl sulfide (DMS) channel is active for K2-18 b. On Earth this compound is produced almost exclusively by marine phytoplankton. The signal is tentative and requires confirmation with additional transit observations.

🧅 Atmospheric Cross-Section

Deep TroposphereSilicate Cloud DeckStratosphereThermosphereColdHot
Click a layer to deploy atmospheric probe
Temperature Profile
Probe Position

Data synthesised from JWST science releases (2022–2025), including the WASP-39 b CO₂/SO₂ detections, the WASP-96 b first-light spectrum, K2-18 b atmospheric studies and the TRAPPIST-1 system observations.

Educational simulation. Spectral features are approximated for demonstration and are not literal transit-depth measurements.