Rings surrounding Uranus Stunning ice giant photo taken by the James Webb Space Telescope
A stunning image of Uranus, taken by the James Webb Space Telescope (JWST), reveals the ice giant's ring system, brightest moons, and dynamic atmosphere in remarkable detail.
The latest
discovery, made on February 6, comes in the wake of a magnificent photo of
Neptune, the second ice giant in the solar system, that JWST recently took.
11 of the
planet's 13 known rings are visible in the most recent photograph of Uranus,
some of which are so bright that they overlap significantly. The fact that
JWST's Near Infrared Camera (NIRCam) equipment is sensitive enough to have
recorded the innermost two of Uranus' hazy rings, however, will truly surprise
astronomers.
Only two
other astronomical observers have caught a glimpse of these dim rings: the
Voyager 2 spacecraft, which passed Uranus in 1986, and more recently, the Keck
Observatory's cutting-edge adaptive optics.
During its
1986 visit, Voyager 2's images of Uranus revealed little more than a lifeless
blue rock devoid any distinguishing markings. This most recent JWST image is a
sharp contrast, depicting a dynamic and altering globe.
The blue
colouring and orange highlights in the JWST image were created by merging
information from two filters. In the representative-color image, Uranus appears
as a light blue snowball, with a dense ice fluid of water, methane, and ammonia
circling it.
The ice
giant Uranus rotates on its side in the solar system, with its orbit tilted at
an angle of around 90 degrees to that of the sun. Due to this tilt, Uranus
experiences severe seasons, with each pole experiencing long stretches of
continuous sunlight followed by an equal swath of darkness.
At Uranus'
northern pole, it is currently spring. This can be seen in the image, where the
ice cap on the right side of the ice giant, which is facing the sun, brightens.
This feature of the polar cap is new to science; it was not visible in even the
most technologically advanced pictures taken by Keck.
A bright
cloud with some fainter extended features is present at the polar cap's edge.
This also features a second, extremely brilliant cloud at Uranus' left limb.
According to JWST team members, clouds like these are normal for Uranus and can
be observed at infrared wavelengths. It is thought that they are linked to
storm activity over the ice giant. Beginning in 2028, Uranus' northern pole
will enjoy its summertime.
The south
pole of Uranus, which is now facing away from the sun and out of view in the
image, is located on the planet's dark side and is obscured by the inky
darkness of space.
When JWST
captured images of the ice giant, it was able to capture six of Uranus' 27
known moons. The other moons are too dim to be seen in a very brief 12-minute
exposure; this one is the brightest of them all.
The powerful
telescope in space will keep observing the ice behemoth. According to members
of the mission team, its extended research should be able to make out two even
fainter outer dust rings that the Hubble Space Telescope found in 2007
Reference:
space.com
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