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Uranus (Nov. 2014 and Nov. 2022)

Two views of the tipped planet Uranus appear side-by-side for comparison.

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.

About the Object

  • Distance
    DistanceThe physical distance from Earth to the astronomical object. Distances within our solar system are usually measured in Astronomical Units (AU). Distances between stars are usually measured in light-years. Interstellar distances can also be measured in parsecs.
    On 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 Description
    Data DescriptionProposal: A description of the observations, their scientific justification, and the links to the data available in the science archive.
    Science Team: The astronomers who planned the observations and analyzed the data. "PI" refers to the Principal Investigator.

    The HST observations include those from programs 13937 , and 16995 (A. Simon)

  • Instrument
    InstrumentThe science instrument used to produce the data.
    WFC3/UVIS
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    09 Nov. 2014, and 09 Nov. 2022
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F467M, F547M, and F845M
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Uranus
  • Object Description
    Object DescriptionThe type of astronomical object.
    Planet
  • Release Date
    March 23, 2023
  • Science Release
    Hubble Monitors Changing Weather and Seasons at Jupiter and Uranus
  • Credit
    NASA, ESA, STScI, Amy Simon (NASA-GSFC), Michael Wong (UC Berkeley); Image Processing: Joseph DePasquale (STScI)

Downloads

  • Full Res (For Display), 2760 × 1388
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  • Full Res (For Print), 2760 × 1388
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  • 2000 × 1006
    png (1.45 MB)
  • Nov. 09, 2014 (For Display), 1388 × 1388
    png (1.53 MB)
  • Nov. 09, 2014 (For Print), 1388 × 1388
    tif (1.1 MB)
  • Nov. 09, 2022 (For Display), 1388 × 1388
    png (1.38 MB)
  • Nov. 09, 2022 (For Print), 1388 × 1388
    tif (1.02 MB)
Two views of the tipped planet Uranus appear side-by-side for comparison.
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

These 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

Compass and Scale
Compass and ScaleAn astronomical image with a scale that shows how large an object is on the sky, a compass that shows how the object is oriented on the sky, and the filters with which the image was made.

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Details

Last Updated
Mar 28, 2025
Contact
Media

Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov