Hubble Just Took an Astonishingly Detailed Image of Saturn

Above you can see the image that was captured, and if you couldn't pick which planet we are looking at from the image, I'm happy to tell you that it's Saturn.

Annotated version of the Hubble Space Telescope view of Saturn on July 4, 2020.

If you want an iconic picture of the planet Saturn, it doesn't get any better than this.

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A Saturnian year lasts 29.5 Earth years, and summer on Saturn lasts about 8 Earth years. Credit: NASA, ESA, A. Simon (Goddard Space Flight Center), M.H. Wong (University of California, Berkeley), and the OPAL Team.

The Hubble Space Telescope has snapped a stunning picture of our sixth planet, Saturn, and it doesn't even look real.

The image shows the rings in exceptional detail, while also highlighting "a number of small atmospheric storms" that come and go with each annual observation of the planet by the telescope. Saturn's atmosphere is mostly hydrogen and helium with traces of ammonia, methane, water vapor, and hydrocarbons that give it a yellowish-brown color.

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The Hubble space telescope has spent the past 30 years orbiting 547 km (340 miles) above Earth. For case in point, there's a slight crimson haze in the northern hemisphere.

"NASA's Cassini spacecraft measurements of very small grains raining into Saturn's environment counsel the rings can only very last for 300 million additional years, which is 1 of the arguments for a youthful age of the ring technique", mentioned planetary scientist Michael Wong of the University of California, Berkeley.

The reddish haze seen in the northern hemisphere could be due to increased heat from the sunlight, changing the circulation of the atmosphere or removing ices from aerosols, NASA suggested.

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"It is astounding that even more than a several yrs, we're observing seasonal improvements on Saturn", explained planetary scientist Amy Simon of NASA's Goddard Place Flight Centre. The famed telescope took the image on July 4 as part of the Outer Planets Atmospheres Legacy (OPAL) project, which seeks to monitor and study atmospheric conditions on our solar system's gas giants.

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