Origin of Martian Moons from Binary Asteroid Dissociation

TL;DR

This paper proposes that the Martian moons Deimos and Phobos originated from binary asteroid dissociation, where tidal forces during close planetary encounters can strip moons from asteroids, offering a plausible capture mechanism.

Contribution

It introduces a novel hypothesis that binary asteroid dissociation explains the origin of Martian moons, linking asteroid moon phenomena to planetary capture processes.

Findings

Binary asteroid dissociation can produce captured moons.

Tidal forces during close approaches facilitate moon stripping.

This mechanism offers a new explanation for Martian moons' origin.

Abstract

The origin of the Martian moons Deimos and Phobos is controversial. One hypothesis for their origin is that they are captured asteroids, but the mechanism requires an extremely dense martian atmosphere, and the mechanism by which an asteroid in solar orbit could shed sufficient orbital energy to be captured into Mars orbit has not been well elucidated. Since the discovery by the space probe Galileo that the asteroid Ida has a moon "Dactyl", a significant number of asteroids have been discovered to have smaller asteroids in orbit about them. The existence of asteroid moons provides a mechanism for the capture of the Martian moons (and the small moons of the outer planets). When a binary asteroid makes a close approach to a planet, tidal forces can strip the moon from the asteroid. Depending on the phasing, the asteroid can then be captured. Clearly, the same process can be used to explain the origin of any of the small moons in the solar system.