Monday, November 28, 2022
HomeScienceScienceAlert: Phobos' Tiger Stripes Mystery May Be Solved

ScienceAlert: Phobos’ Tiger Stripes Mystery May Be Solved

The Universe’s Martian moon Phobos will not last long

Astronomers calculate that the potato-shaped satellite is gradually, but inexorably, drawing closer to its host world. In about 100 million years, gravitational interaction will eventually occur between the two bodies. tear Phobos apartThis temporarily dusty ring was created by the red planet.

New research suggests that these gravitational interactions might already be having an observed effect. The mysterious shallow, parallel grooves that run beneath the surface of the earth may have some explanation. The moon’sFracturing could result in the destruction of its entire surface as its orbit slowly degrades and tidal forces pull harder on its bones.

“Our analysis supports the existence of a layered heterogeneous structure in Phobos, with possibly underlying failure-induced cracks. This could be the precursor to the eventual demise and de-orbiting satellite.” Write a team of astronomersBin Cheng, of Tsinghua University (China) and the University of Arizona is the leader.

Their gravitational interaction creates tide forces that pull bodies together in a system. This causes their structures to stretch along an axis between them.

Most of the time, distortions to solid surfaces have very little impact. Visible effects on land masses are not as obvious as those caused by tidal forces. However, it is possible to observe the movement of planet’s liquid oceans.

However, tidal forces that interact with other solid bodies may have more severe consequences. Stress fracture can result from stretching caused by tidal force. This was evident in Saturn’s moon Enceladus. The icy shell of Enceladus has deep parallel fractures at the south pole. Tidal stress can cause tidal stress.

Phobos orbits in just 7 hours 39 minutes. MarsIt is moving at a speed of approximately 1.8 centimeters per annum. At this distance, it is entirely possible that tidal force could cause surface fracture on the body’s 27 kilometer (16.8 mile) width. This interaction may have led to Phobos’ stripes. ??.

It is not clear if the current interaction between Phobos and Mars could result in the observed stripes. Other explanations, however, are possible. In 2018, a study concluded that the stripes could have been caused by the Results of rolling boulders.

Cheng and his collaborators did 3D mathematical modeling to examine the tidal stretching of a Phobos-like body with a loose rubbly exterior and a cohesive layer below.

Researchers performed hundreds of simulations with their model. A significant number of these simulations showed that tidal forces caused a cohesive layer to fracture in parallel grooves. This allowed the upper loose regolith and subsequently the fractures below to form. The result is a very similar surface to that seen on Phobos.

The team discovered that not all areas of Phobos are consistent with the model. Grooves around were particularly noticeable. The moon’sThe predictions were wrong. However, the results show that at most some stripes could be due to fracturing. The moonDeath spirals by tidal disembowelment. This would signify that Phobos is at the end of its days.

These results may have implications for studying moons with significant orbital decay like Neptune’s Moon Triton. The grooves could be a fascinating area to study for the Mars mission by the NASA. Japanese Space Agency.

This mission is expected to deliver conclusive evidence of the origin of these mysterious stripes – but tidal disruption is certainly appearing to be an intriguing possibility.

“Modelling Phobos as an interior rubble-pile overlaid with a cohesive layer, it is clear that the tidal strain can create parallel fissures with regular spacing.” The researchers wrote in their paper.

“Our analysis suggests the existence of some grooves along the surface Phobos’ is a sign of the possible demise of this satellite.”

Who doesn’t love mashed potatoes?

The research has been published in The Planetary Science Journal.

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