Uranus is perhaps the strangest of all the planets within the solar system. Additionally, the planet itself is not necessarily strange, but a true oddity is its unusual behavior and enigmatic past. While Uranus is visible to the naked eye, because of the dimness of the planet and the slow orbit mistaken as a star for a long period of time. Furthermore, Uranus, the seventh planet from the Sun was the first planet to be discovered by the scientist.
British astronomer William Herschel discovered Uranus with his telescope on March 13, 1781, while observing all the stars which is 10 times dimmer than the naked eye can see. After some research, Herschel found one star looking peculiar and noticed that the star followed a planetary orbit within a year.
Uranus was named after Ouranos, the Greek sky god, the first of celestial gods. In addition, it is the only planet to be named after a Greek deity and not a Roman one. After its discovery, several names were suggested for the new planet like Hypercronius, Minerva and Herschel.
Although Herschel proposed the name Georgium Sidus, the idea was unpopular outside England. Later, the German astronomer Johann Bode, who studied the orbit of the planet, gave the planet its final name as Uranus. Likewise, Bode argued that the new planet would be named after Saturn’s parent; since Saturn was Jupiter’s parent.
Lately, the team of researches of Japan’s Tokyo Institute of Technology tackles one of the biggest question marks about Uranus. The researches have tried to solve the biggest question marks about Uranus. The questions like How did it get its strange, lopsided rotation, and what evidence still remains from that event? is a matter of curiosity for everyone.
It has long been thought that at some stage in its history, Uranus suffered a huge impact. The researchers took other possibilities into account and used Earth’s own past as an example of what happens when two massive objects collide in space. One hypothesis about Earth’s Moon formation is that a massive body of Mars crashed into Earth many billion years ago. As a result, materials were dispersed into space and ultimately contributing to the planet and moon we see today.
Although the Earth developed so much closer to the Sun than Uranus, Scientists believe the type of body that served as its impactor was probably much different, likely made of water ice or ammonia. Unlike the collision that formed the Earth and Moon, scientists believe that a wealth of gas and smaller debris would have been produced by the impact between Uranus and this unknown icy body.
Don’t Miss: Could there be Life on Mars?
The planet tipped to its side and slowly accumulated all of the residual material from the collision, while the tiny moons of the planet were created by some large chunks.
Uranus is one of the weird planets by its behavior. Some of the weird parts of the planet are discussed below.
Planets spin in a number of ways around their axis. Some, such as Mercury and Jupiter, have a spin that ensures their north poles point to the plane of their orbital path around the Sun at nearly the right angles. On the other hand, the planet like Earth and Saturn is tilted towards their axis. Likewise, sometimes their north pole is pointing towards the Sun a little more, while at other times it’s away from the Sun.
Then we have Uranus, the solar system’s most inebriate planet: it has tipped over absolutely on its side. In particular, Uranus, like Venus, spins from east to west; the opposite of what Earth does. That means for 21 Earth-years; a piece per Uranian year, its north and south poles take turns directly looking down the furnace at the heart of our solar system.
Unlike Jupiter and Neptune, Uranus has a thin network of 13 rings which was detected for the first time in 1977. Voyager 2 saw two of its 13 rings and 11 of its 27 diminutive moons as it skimmed over its cloud tops back in January 1986.
You May Be Interested in- Simple Ways Humans are Destroying the Environment
Its rings consist of a combination of water-ice and rocky material. Particularly, the individual units of which can be smaller than household dust. Its inner rings are thinner and darker; its outer rings are more vibrant and light.
Around 80 percent of Uranus’ mass consists of salt, methane, and ammonia, all revolving around a fairly small rocky core. Things are extremely frigid in the upper atmosphere of the Uranus. Additionally, with its molecular hydrogen and atomic helium, it’s temperature can reach up to -214 °C (-353 °F).
On the other hand, Diving deep into its vaporous interior, things really start heating up inside Uranus. Temperatures rise to about 5,000 °C (9,000 ° F) near the heart with all the gas squashing down on itself. Uranus also encounters some strong gusts. Winds blow around Uranus at velocities up to 900 kilometers (560 miles) per hour.
Keep Supporting Wikye.com For More Trending Topics