JWST Protoplanetary Disk Winds & Gas Giant Window Simulator

Disk Cross-Section & Wind Morphology MHD Molecular Jets Dominant

Scale: 0.1 – 40 AU (Logarithmic Cross-Section)

Disk Age (Myr) 1.2 Myr

UV/X-ray Photoevaporative Flux 1.0 × Φ₀

MHD Magnetic Field Strength 1.5 B₀

Core Orbit Distance (AU) 5.2 AU

Accretion Race Telemetry

Gas Mass Remaining

38.4 M_Jup

Planetary Mass

1.8 M_Earth

Wind Mode Ratio

84% CO / 16% [Ne II]

Window Status

OPEN (Runaway)

Result Architecture: Jupiter-class Gas Giant

Core reached critical runaway threshold (10 M_Earth) at 2.4 Myr prior to complete atomic gas dispersal at 4.6 Myr.

Spectroscopic Tracer Flux (JWST MIRI/NIRSpec)

            Molecular CO v=1-0 (4.67 μm):
            14.2 × 10⁻¹⁵ W/m²
          
            Atomic [Ne II] (12.81 μm):
            1.8 × 10⁻¹⁵ W/m²
          
            Atomic [O I] (63.18 μm):
            3.1 × 10⁻¹⁵ W/m²

JWST 72-Star Protoplanetary Survey Sample Click any archetype star to load observation data

Star ID	Spectral Type	Est. Age (Myr)	Disk Mass (M_J)	Wind Dominance	Accretion Window	Observed Inner Gap