Saturn: Researchers now know how it got its rings

According to one study, the destruction of the Moon 100-200 million years ago led to the formation of Saturn’s rings. This also explains the apparent large inclination of the planet’s rotation axis. US researchers came to this conclusion based on a new analysis of data from the Cassini space probe and computer simulations. In order to confirm the model, however, the internal structure of Saturn must be examined more closely, the scientists wrote in the journal
Sciences
.

“The angle between the equatorial plane of the planet and the plane of its orbit, at 26.7 degrees, is too large to appear during the formation phase of Saturn from the disk of gas around the sun,” explains Jack Wisdom of MIT. Technology (MIT) and colleagues. Because the conservation of angular momentum ensures that the axis of rotation of any developing planet is approximately perpendicular to the orbital plane. So there must be a later reason to tilt this axis.

What role does Neptune play?

Astronomers have discussed an echo between Saturn and Neptune, the farthest planet in the solar system, as a possible cause for nearly two decades. Because Saturn’s axis of rotation “oscillates”–the researchers call it anticipation–in the same rhythm as Neptune’s orbit. As a result, small perturbations from Neptune accumulate over such a long period of time that what was originally a small inclination of the axis can increase to the present value.

However, the influence of Neptune on Saturn depends on its moons and on the exact distribution of Saturn’s internal mass. That’s where Wisdom and colleagues come in: Based on orbital data sent back to Earth by the Saturn probe Cassini—particularly during the crash of the target probe on September 15, 2017—the researchers built an improved model of the planet. And we came to a disappointing conclusion at first: So Saturn is not in the zone of resonance with Neptune, but outside.

But the team did not give up. Researchers’ idea: Saturn may have initially been in harmony with Neptune, but was then alienated by an event in that region. “So we started looking for a way to get Saturn out of Neptune’s echo,” Wisdom says.

Debris remains form Saturn’s rings today

Based on theoretical considerations and a large number of simulations of the planet and from it moons Scientists finally found a solution:
Saturn must originally have another larger moon.
Just with that extra moon – about the size of the third largest moon Satellites It was supposed to be Japetus – he managed to maintain Saturn’s resonance with Neptune for a long time.

But the orbits of Saturn’s moons change. In particular, the orbit of Saturn’s largest moon, Titan, is slowly moving outward. Sometime between 100 and 200 million years ago, this caused a severe disturbance to the orbit of the previous extra moon, which Wisdom and his team dubbed “Chrysalis”: in a chaotic orbit, it approached Saturn so closely that the planet’s tidal forces were torn apart. With the disappearance of Chrysalis, Saturn deviated from the echo of Neptune.

A lot of debris fell on the planet,
The remains eventually formed what are now Saturn’s rings
. So this model can explain both the rings and the tilt of Saturn’s axis. However, this scenario also depends heavily on the distribution of mass in the planet’s interior. Therefore, more accurate data from future space probes are needed to confirm the model.