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

TL;DR

This study explores how sodium in carbonaceous chondrites can sublimate at low perihelion temperatures, potentially explaining activity in asteroids like Phaethon through experimental heating and theoretical modeling.

Contribution

It demonstrates sodium's role as a volatile in low-perihelion asteroids, supported by experimental sodium loss in heated meteorite samples and theoretical sublimation models.

Findings

Sodium sublimates from specific mineral phases at high temperatures.

Heating experiments show sodium loss comparable to asteroid surface conditions.

Sodium outgassing could drive activity in low-perihelion asteroids.

Abstract

Solar system bodies with surface and sub-surface volatiles will show observational evidence of activity when they reach a temperature where those volatiles change from solid to gas and are released. This is most frequently seen in comets, where activity is driven by the sublimation of water, carbon dioxide, or carbon monoxide ices. However, some bodies (notably the asteroid (3200) Phaethon) show initiation of activity at very small heliocentric distances, long after they have reached the sublimation temperatures of these ices. We investigate whether the sodium present in the mineral matrix could act as the volatile element responsible for this activity. We conduct theoretical modeling which indicates that sodium has the potential to sublimate in the conditions that Phaethon experiences, depending on the mineral phase it is held in. To test this, we then exposed samples of the carbonaceous chondrite Allende to varying heating events similar to what would be experienced by low perihelion asteroids. We measured the change in sodium present in each sample, and find that the highest temperature samples show a significant loss of sodium from specific mineral phases over a single heating event, comparable to a day on the surface of Phaethon. Under specific thermal histories possible for Phaethon, this outgassing could be sufficient to explain this object's observed activity. This effect would also be expected to be observed for other low-perihelia asteroids as well, and may act as a critical step in the process of disrupting small low-albedo asteroids.