A new type of planetary object, "Synestia", revealed in a recent study


A recent study, published in the Journal of Geophysical Research: Planets, revealed in the journal Geophysical Union of America a new type of planetary object – rotating, in the form of donuts, a mass of hot and evaporated rocks that have the appearance of a planet as a spatial object. Scientists have named this rarely celestial body Synestia.

According to some theories, rocky worlds, such as Earth, Mars or Venus, were created in the early solar system due to collisions between smaller objects. Due to the strength of these influences, the original results were the mass of melted, sometimes even steamed rocks. Those who eventually cooled down and solidified in spherical shapes – the planets, as we know them today.

But a recent study focused on collisions between objects that are already rotating. In fact, the front planetary object maintains its torque even after being struck by other similar stones. More specifically, the research focused on the behavior of objects rotating in the size of the Earth, which are violently colliding, while maintaining a high angular momentum.

"Synestia" is a new type of planetary object proposed by scientists in a new study

For their study, scientists analyzed data that had been recorded about important impacts in space, and found that due to these violent collisions a new type of planetary object could be created. Statistically, researchers found that heavy crashes during the spinning of the planet would give birth to a new planetary object – "Synestia", as they called it.

Scientists believe that a new type of planetary object is formed due to the moment of rotating the impact elements, which causes scaling bodies to form as a ballistic object similar to the planet. The planets are made of rocks, but when they collide, sometimes the rocks turn melt or gasy and expand.

"Most planets are likely to experience collisions that could at some point during their creation form a" sinister. "For an object such as Earth," Synestia "would not last very long – perhaps a hundred years – before it lost enough heat to condensed back into a solid object, but "Synestia", which originated from larger or hotter objects such as gaseous planets or stars, could last longer, "explains Sarah Stewart, a planetary scientist at the University of California Davis.


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