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Saturn Prior to Cassini Probe’s Arrival

Saturn Prior to Cassini Probe's Arrival

As NASA's Cassini spacecraft hurtles toward a July 1, 2004 rendezvous with Saturn, the Hubble Space Telescope continues snapping breathtaking pictures of the solar system's most photogenic planet. This latest view, taken on March 22, 2004, is so sharp that many individual ringlets can be seen in Saturn's ring plane.

Though Hubble is nearly a billion miles farther from Saturn than the Cassini probe, Hubble's exquisite optics, coupled with the high resolution of its Advanced Camera for Surveys (ACS), allow it to take pictures of Saturn which are nearly as sharp as Cassini's wide-angle views of the full planet as it begins its approach. Of course, Cassini will ultimately far exceed the resolution of Hubble during its close encounter with Saturn; indeed, Cassini's sharpness began to surpass Hubble's when it approached to within 14 million miles (23 million km) of Saturn this month.

Hubble camera exposures in four filters (blue, blue-green, green, and red) were combined into this image, to render colors similar to what the eye would see through a telescope focused on Saturn. The subtle pastel colors of ammonia-methane clouds trace a variety of atmospheric dynamics. Saturn displays its familiar banded structure, and haze and clouds of various altitudes. Like Jupiter, all bands are parallel to Saturn's equator. Even the magnificent rings, at nearly their maximum tilt toward Earth, show subtle hues, which trace chemical differences in their icy composition.

Over two decades have passed since a robotic emissary from Earth last visited Saturn. This was NASA's Voyager-2 space probe, which flew by Saturn in August 1981. But ever since 1990, Hubble has filled in the gap of high-resolution Saturn imaging by tracking storms and auroral activity, and providing crisp views of the ring plane from various angles, as Saturn drifts along its orbit.

Approaching Saturn at an oblique angle to the Sun and from below the ecliptic plane, Cassini has a very different viewing angle on Saturn than Hubble's earth-centered view. For the first time astronomers can compare equal-sharpness views of Saturn from two very different perspectives.

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.
    The semi-major axis of Saturn's orbit about the sun is 9.5 Astronomical Units (A.U.) or roughly 1.4 billion km.
  • Dimensions
    DimensionsThe physical size of the object or the apparent angle it subtends on the sky.
    The planet (without rings) has a diameter of roughly 75,000 miles (120,000 km) at the equator.

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.
    This Hubble image was created from HST data from proposal 9354: E. Karkoschka and M. Tomasko (University of Arizona)
  • Instrument
    InstrumentThe science instrument used to produce the data.
    HST>ACS/HRC
  • Exposure Dates
    Exposure DatesThe date(s) that the telescope made its observations and the total exposure time.
    March 22, 2004
  • Filters
    FiltersThe camera filters that were used in the science observations.
    F439W (B), F502N ([O III]), F550W (V), F658N (H-alpha)
  • Object Name
    Object NameA name or catalog number that astronomers use to identify an astronomical object.
    Saturn
  • Object Description
    Object DescriptionThe type of astronomical object.
    Planet
  • Release Date
    May 26, 2004
  • Science Release
    Saturn Seen from Far and Near
  • Credit
    NASA, ESA and E. Karkoschka (University of Arizona)

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Saturn Prior to Cassini Probe's Arrival
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.

Blue: F439W (B) Cyan: F502N ([O III]) Green: F550W (V) Red: F658N (H-alpha)

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