Hubble image archive

Uranus (Nov. 2014 and Nov. 2022)

Planetary oddball Uranus rolls on its side around the Sun as it follows an 84-year orbit, rather than spinning in a more-vertical position as Earth does. Uranus has a weirdly tipped "horizontal" rotation axis angled just eight degrees off the plane of the planet's orbit. One rece...

Date
Jan 1, 2023
Mission
Hubble Space Telescope
Archive ID
hubblesite-images-2023-007-01gv3fq5aqatqv8gtkpkn5sa5w
By

Planetary oddball Uranus rolls on its side around the Sun as it follows an 84-year orbit, rather than spinning in a more-vertical position as Earth does. Uranus has a weirdly tipped "horizontal" rotation axis angled just eight degrees off the plane of the planet's orbit. One recent theory proposes that Uranus once had a massive moon that gravitationally destabilized it and then crashed into it. Other possibilities include giant impacts during planetary formation, or even giant planets exerting resonant torques on each other over time. The consequences of the planet's tilt are that for stretches of time lasting up to 42 years, parts of one hemisphere are completely without sunlight. When the Voyager 2 spacecraft visited during the 1980s, the planet's south pole was pointed almost directly at the Sun. Hubble's latest view shows the northern pole now tipping toward the Sun.

[left]—This is a Hubble view of Uranus taken in 2014, seven years after northern spring equinox when the Sun was shining directly over the planet's equator, and shows one of the first images from the OPAL program. Multiple storms with methane ice-crystal clouds appear at mid-northern latitudes above the planet's cyan-tinted lower atmosphere. Hubble photographed the ring system edge-on in 2007, but the rings are seen starting to open up seven years later in this view. At this time, the planet had multiple small storms and even some faint cloud bands.

[right]—As seen in 2022, Uranus' north pole shows a thickened photochemical haze that looks similar to the smog over cities. Several little storms can be seen near the edge of the polar haze boundary. Hubble has been tracking the size and brightness of the north polar cap and it continues to get brighter year after year. Astronomers are disentangling multiple effects—from atmospheric circulation, particle properties, and chemical processes—that control how the atmospheric polar cap changes with the seasons. At the Uranian equinox in 2007, neither pole was particularly bright. As northern summer solstice approaches in 2028 the cap may grow brighter still, and will be aimed directly toward Earth, allowing good views of the rings and north pole; the ring system will then appear face-on. This image was taken on November 10, 2022.

Credits

Science

NASA, ESA, STScI, Amy Simon (NASA-GSFC), Michael H. Wong (UC Berkeley)

Image Processing

Joseph DePasquale (STScI)

Image Details

About The Object
Object NameUranus
Object DescriptionPlanet
DistanceOn Nov. 09, 2014 Uranus was 19.18 AU (1.78 billion miles). On Nov. 14, 2022 Uranus was 18.68 AU (1.74 billion miles).
About The Data
Data DescriptionThe HST observations include those from programs , and (A. Simon)
InstrumentWFC3/UVIS
Exposure Dates09 Nov. 2014, and 09 Nov. 2022
FiltersF467M, F547M, and F845M
About The Image
Color InfoThese images are a composite of separate exposures acquired by the WFC3 instrument on the Hubble Space Telescope. Several filters were used to sample medium wavelength ranges. The color results from assigning different hues (colors) to each monochromatic (grayscale) image associated with an individual filter. In this case, the assigned colors are: Blue: F467M, Green: F547M, Red: F845M

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