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Saturn — October 1997
About the Object
- DistanceDistanceThe 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.
- DimensionsDimensionsThe 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 DescriptionData 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.Principal Astronomers: R.G. French (Wellesley College), J. Cuzzi (NASA/Ames Research Center), L. Dones (SwRI), and J. Lissauer (NASA/Ames Research Center). - InstrumentInstrumentThe science instrument used to produce the data.HST>WFPC2
- Exposure DatesExposure DatesThe date(s) that the telescope made its observations and the total exposure time.October 1997
- FiltersFiltersThe camera filters that were used in the science observations.F675W (R), F555W (V), and F439W (B)
- Object NameObject NameA name or catalog number that astronomers use to identify an astronomical object.Saturn
- Object DescriptionObject DescriptionThe type of astronomical object.Planet
- Release DateJune 7, 2001
- Science ReleaseA Change of Seasons on Saturn
- Credit
Color Info
Color InfoA brief description of the methods used to convert telescope data into the color image being presented.
Blue: F439W (B) Green: F555W (V) Red: F675W (R)
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Last Updated
Mar 28, 2025
Contact
Media
Claire Andreoli
NASA’s Goddard Space Flight Center
Greenbelt, Maryland
claire.andreoli@nasa.gov