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Volatility of Sodium in Carbonaceous Chondrites at Temperatures Consistent with Low-perihelion Asteroids

  • Authors: Joseph R. Masiero, Björn J.R. Davidsson, Yang Liu, Kelsey Moore, and Michael Tuite

2021 The Planetary Science Journal 2 165.

  • Provider: AAS Journals

Caption: Figure 2.

Upper left: the total sodium production rate calculated for Phaethon, as a function of heliocentric distance within ∼1 au of the Sun (from 45 days pre-perihelion). Upper right: the location of the sodium sublimation front as a function of the angular distance from the north pole (the colatitude) at perihelion. Middle left: the sodium abundance as a function of depth at latitude 76° S at perihelion, normalized to the initial abundance. Middle right: the pressure created by sodium volatilization as a function of depth for a few rotational phases for 76° S at perihelion. Lower left: the corresponding force caused by the sodium pressure gradient shown in the middle right figure.

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