Extended Data Fig. 4: Evolution of the planetary 14N/15N as a function of the mass accreted in solids (rock and ice). | Nature

Extended Data Fig. 4: Evolution of the planetary 14N/15N as a function of the mass accreted in solids (rock and ice).

From: 15NH3 in the atmosphere of a cool brown dwarf

Extended Data Fig. 4: Evolution of the planetary 14N/15N as a function of the mass accreted in solids (rock and ice).The alternative text for this image may have been generated using AI.

This computation assumes a planet that forms outside the NH3 iceline but inside the N2 iceline. The dotted black line denotes the value expected for pure NH3 ice.

Back to article page