Although orbital dynamics make it highly unlikely that two gas giants would collide, there’s a small chance that such an impact could happen during the formation of a planetary system. The result of a collision mainly depends on the speed and angle of impact.
Head-on collisions would generally lead to a complete merger of the gas giants without any loss of material, either in their solid cores or in their gaseous envelopes. However, a higher speed head-on collision would likely lead to the loss of most of the envelope gas as the two cores merge. Very high speeds would completely fragment and destroy both planets.
Collisions that are not head-on (known as oblique collisions) can give different results. For instance, if the two cores avoid each other completely, both gas giants will lose a substantial fraction of their gaseous envelopes to space, but will not merge. If the cores collide at an angle then the planets may or may not merge, but in all cases a large amount of the gaseous envelope will be lost.
Very oblique collisions do not disrupt the planets at all and both would continue on almost the same orbits without losing any mass. Oblique impacts between gas giants can lead to changes in their shape, or ‘oblateness’. This has been proposed as a means of studying the early impact history of gas giants in other star systems.
Although there is no concrete evidence that Jupiter or Saturn formed from the merger of smaller gas giants, it is a possibility. Jupiter and Saturn have a higher fraction of heavy elements than the Sun, suggesting that one or both of them may have been formed by such a collision.
- Could two planets share the same orbit without colliding?
- What would happen if the Earth became tidally locked to the Sun?
- Could Neptune and Pluto ever collide, as their orbits intersect?
- What would happen if there were no Moon?
Asked by: Mark Buckmaster
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