Volatile depletion in rocky planets as a chemical fingerprint of hybrid accretion

arXiv:2608.24407 · astro-ph.EP · Submitted 2026-08-25 · Read on arXiv

astro-ph.EP

Submitted: 2026-08-25

Updated: 2026-09-25

Terminology

• Core — 36× in this paper · explained in 2 episodes
• Bayesian Inference — 22× in this paper · explained in 5 episodes
• Abundance — 20× in this paper · explained in 1 episode
• Hybrid Model — 2× in this paper · explained in 2 episodes
• Metallicity — 2× in this paper · explained in 3 episodes
• Pebble-grown Mars — 2× in this paper
• Trace — 2× in this paper · explained in 2 episodes
• Robustness — 1× in this paper · explained in 5 episodes
• Streaming Instability — 1× in this paper · explained in 2 episodes
• Velocity Dispersion — 1× in this paper · explained in 2 episodes

Sources

• Comment on "Did the terrestrial planets of the Solar System form by pebble accretion?"

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