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The mapping of Venus refers to the process and results of human description of the geological features of the planet Venus. It involves surface radar images of Venus, construction of geological maps, and the identification of stratigraphic units, volumes of rock with a similar age. Satellite radar provides imagery of the surface morphology by ...
The Magellan mission mapped the surface of Venus with radar in the 1990s. The images gave the first global view of what was below Venus’ thick clouds. This radar image aligns with the surface features seen on WISPR images captured by Parker Solar Probe during its third flyby of the planet in July 2020. Credits: Magellan Team/JPL/USGS.
Show in archive: true. This map of the surface of Venus was created from observations accumulated during more than a decade of radar imaging of the planet. Observations made by NASA's Magellan spacecraft between 1990 and 1994 form the base of the image, with gaps in the data filled in by the Arecibo Observatory, which is based in Puerto Rico.
Product Information: This mosaic was created from the Magellan F-BIDRs, (Full resolution Basic Image Data Records), the highest resolution radar images of the Venus surface (~75 m/pixel). For a smaller download, this base is available for processing (clipping and format conversion) using the Map-A-Planet 2 "processing" button on the right.
May 7, 2008 · This global view of the surface of Venus is centered at 180 degrees east longitude. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a computer-simulated globe to create this image. Data gaps are filled with Pioneer Venus Orbiter data, or a constant mid-range value.
- NASA/Jet Propulsion Laboratory-Caltech
Nov 19, 2010 · Image Article. This global view of the surface of Venus is centered at 180 degrees east longitude. Magellan synthetic aperture radar mosaics from the first cycle of Magellan mapping are mapped onto a computer-simulated globe to create this image. Data gaps are filled with Pioneer Venus Orbiter data, or a constant mid-range value.
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This global view of the surface of Venus is centered at 90 degrees east longitude. Magellan synthetic aperture radar mosaics from the three eight-month cycles of Magellan radar mapping are mapped onto a computer-simulated globe to create this image. Magellan obtained coverage of 98 percent of the surface of Venus.
