Detecting Oxygen in Exoplanet Atmospheres

Project lead & developer: Antonika Shapovalova — Habitable Worlds Observatory scenario

HWO profile: D=6.0 m, efficiency 20%, R≈150, Sun-like host at 10 pc.

Theme: “Detecting Oxygen in Exoplanet Atmospheres Using the Habitable Worlds Observatory”.

Mission statement

Habitable Worlds Observatory forward model + retrieval benchmark for the O₂ A-band. Dashboard tracks photon budgets, systematics, and detectability thresholds for Earth analogs at 5–30 pc.

Theme: Detecting oxygen with HWO

Line-core depth

84.2 ppm

3.23e+07 photons/s

Hours for SNR=5

0.04

noise floor 7.0 ppm

SNR after 100 h

12.0

cloud-top 15 km
1. Spectrum & key diagnostics

Static spectrum

spectrum

Key wavelengths

Featureλ (nm)Depth (ppm)Photon ratehrs@SNR=3hrs@SNR=5hrs@SNR=10
Line core762.784.23.232e+070.010.040.39
Continuum748.083.93.205e+070.010.040.41
760 nm759.984.13.227e+070.010.040.40
2. SNR diagnostics
SNR vs wavelength
Hours for SNR=5
SNR scaling
Distance curve
Distance (pc)Hours for SNR=5SNR (100 h)
5.00.00912.0
10.00.03712.0
20.00.3946.0
30.04.0
3. Atmosphere & transit geometry
4. Interactive spectrum
5. Retrieval-style O₂ threshold

Detectability drops once O₂ falls below ≈21.00% (100 h, SNR=5)

vmr curve
O₂ VMR (%)SNR (100 h)Hours for SNR=5
21.000<0.1
12.340<0.1
7.260<0.1
4.260<0.1
2.510<0.1
1.470<0.1
0.870<0.1
0.510<0.1
0.300<0.1
0.180<0.1
0.100<0.1
0.060<0.1
0.040<0.1
0.020<0.1
6. Instrument comparison instrument comparison
InstrumentHours for SNR=5SNR (100 h)
HWO0.03712.0
JWST/NIRSpec0.0488.4
Roman0.2477.0