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This hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered on the North Pole. NASA's Magellan spacecraft imaged more than 98% of Venus.
This hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered on the North Pole. NASA's Magellan spacecraft imaged more than 98% of Venus.

Hemispheric View of Venus Centered at the North Pole

This hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered on the North Pole. NASA's Magellan spacecraft imaged more than 98% of Venus.
This hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in the 1990-1994 Magellan mission, is centered on the North Pole. NASA's Magellan spacecraft imaged more than 98% of Venus.

Hemispheric View of Venus Centered at the South Pole

This full resolution radar mosaic from NASA's Magellan spacecraftshows an oblique view of the impact crater Riley, named for Margaretta Riley, a 19th Century botanist.
This full resolution radar mosaic from NASA's Magellan spacecraftshows an oblique view of the impact crater Riley, named for Margaretta Riley, a 19th Century botanist.

Venus - Oblique View of Crater Riley

These two radar images from NASA's Magellan spacecraft are centered about 60.5 degrees south latitude and 348.8 degrees east longitude in the eastern Lavinia Region of Venus.
These two radar images from NASA's Magellan spacecraft are centered about 60.5 degrees south latitude and 348.8 degrees east longitude in the eastern Lavinia Region of Venus.

Venus - Left and Right Looking Images of Lavinia Region

Three large meteorite impact craters are seen in this image obtained by NASA's Magellan spacecraft  of the Lavinia region of Venus.
Three large meteorite impact craters are seen in this image obtained by NASA's Magellan spacecraft  of the Lavinia region of Venus.

Venus - Lavinia Region Impact Craters

This Magellan full resolution mosaic, centered at 12.3 north latitude, 8.3 degrees east longitude, shows an area in the Eistla region of Venus.
This Magellan full resolution mosaic, centered at 12.3 north latitude, 8.3 degrees east longitude, shows an area in the Eistla region of Venus.

Venus - Eistla Region

A corona is displayed in this computer-simulated view from NASA's Magellan spacecraft of the surface of Venus.
A corona is displayed in this computer-simulated view from NASA's Magellan spacecraft of the surface of Venus.

Venus - Three Dimensional Perspective View of Idem-Kuva

This image from NASA's Magellan spacecraft, with radar illumination from west to east, shows three unusual volcanoes located in the Guinevere Planitia lowland.
This image from NASA's Magellan spacecraft, with radar illumination from west to east, shows three unusual volcanoes located in the Guinevere Planitia lowland.

Venus - Volcanos in Guinevere Planitia

This false color image from NASA's Magellan spacecraft shows a portion of Bereghinya Planitia (plains) in the northern hemisphere of Venus.
This false color image from NASA's Magellan spacecraft shows a portion of Bereghinya Planitia (plains) in the northern hemisphere of Venus.

Venus - False Color of Bereghinya Planitia

This false color Magellan image shows a portion of Eistla Regio (region) in the northern hemisphere of Venus, centered at 1 degrees south latitude, 37 degrees east longitude.
This false color Magellan image shows a portion of Eistla Regio (region) in the northern hemisphere of Venus, centered at 1 degrees south latitude, 37 degrees east longitude.

Venus - False Color of Eistla Regio

Southwest Lakshmi Planum (plains) is bounded on the south by the Danu Montes (mountains) as shown by NASA's Magellan spacecraft.
Southwest Lakshmi Planum (plains) is bounded on the south by the Danu Montes (mountains) as shown by NASA's Magellan spacecraft.

Venus - Danu Montes and Lakshmi Planum

Landslides on Venus! The image on the left was taken in late November of 1990 during Magellan's first trip around Venus. The image on the right was taken July 23, as the Magellan spacecraft passed over the region for the second time.
Landslides on Venus! The image on the left was taken in late November of 1990 during Magellan's first trip around Venus. The image on the right was taken July 23, as the Magellan spacecraft passed over the region for the second time.

Venus - Aphrodite Terra

Two unusual volcanic domes are shown in this full-resolution mosaic obtained by NASA's Magellan spacecraft.
Two unusual volcanic domes are shown in this full-resolution mosaic obtained by NASA's Magellan spacecraft.

Venus - Volcanic Domes East of Beta Regio

This image rom NASA's Magellan spacecraft shows part of the northern boundary of Ovda Regio, one of the large highlands ringing the equator of Venus.
This image rom NASA's Magellan spacecraft shows part of the northern boundary of Ovda Regio, one of the large highlands ringing the equator of Venus.

Venus - Ovda Regio

This full resolution radar image from NASA's Magellan spacecraft is centered along the eastern edge of Lakshmi Planum and the western edge of Maxwell Montes.
This full resolution radar image from NASA's Magellan spacecraft is centered along the eastern edge of Lakshmi Planum and the western edge of Maxwell Montes.

Venus - Lakshmi Planum and Maxwell Montes

This image is a full-resolution mosaic of several images from NASA's Magellan spacecraft. The radar smooth region in the northern part of the image is Lakshmi Planum, a high plateau region above the mean planetary radius.
This image is a full-resolution mosaic of several images from NASA's Magellan spacecraft. The radar smooth region in the northern part of the image is Lakshmi Planum, a high plateau region above the mean planetary radius.

Venus - Lakshmi Planum

This image mosaic from NASA's Magellan spacecraft is of an impact crater located in Guinevere Planitia on Venus.
This image mosaic from NASA's Magellan spacecraft is of an impact crater located in Guinevere Planitia on Venus.

Venus - Impact Crater in Guinevere Planitia

This view of the surface of Venus acquired by NASA's Magellan spacecraft shows a geographically young region of lowland plains. The location is near the equator between two highland areas known as Asteria Regio and Phoebe Regio.
This view of the surface of Venus acquired by NASA's Magellan spacecraft shows a geographically young region of lowland plains. The location is near the equator between two highland areas known as Asteria Regio and Phoebe Regio.

Venus - Asteria Regio and Phoebe Regio

This image mosaic from NASA's Magellan spacecraft shows the impact crater Golubkina.
This image mosaic from NASA's Magellan spacecraft shows the impact crater Golubkina.

Venus - Crater Golubkina

Many of the impact craters of Venus revealed by NASA's Magellan spacecraft have characteristics unlike craters on any other planetary body. This crater, named Adivar, is located just north of the western Aphrodite highland.
Many of the impact craters of Venus revealed by NASA's Magellan spacecraft have characteristics unlike craters on any other planetary body. This crater, named Adivar, is located just north of the western Aphrodite highland.

Venus - Adivar Crater

The western half of the planet is displayed in this simple cylindrical map of the surface of Venus obtained by NASA's Magellan spacecraft.
The western half of the planet is displayed in this simple cylindrical map of the surface of Venus obtained by NASA's Magellan spacecraft.

Venus - Simple Cylindrical Map of Surface (Western Half)

This computer-generated perspective view of Latona Corona and Dali Chasma on Venus shows NASA's Magellan radar data superimposed on topography.
This computer-generated perspective view of Latona Corona and Dali Chasma on Venus shows NASA's Magellan radar data superimposed on topography.

Venus - Three Dimensional Perspective View of Latona Corona and Dali Chasma

The northern hemisphere is displayed in this global view of the surface of Venus as seen by NASA's Magellan spacecraft.
The northern hemisphere is displayed in this global view of the surface of Venus as seen by NASA's Magellan spacecraft.

Venus - Computer Simulated Global View Centered at 90 Degrees East Longitude

This perspective view of Ishtar Terra was derived from data obtained by NASA's Pioneer Venus spacecraft's altimetry radar instrument.
This perspective view of Ishtar Terra was derived from data obtained by NASA's Pioneer Venus spacecraft's altimetry radar instrument.

Perspective View of Ishtar Terra

In September 1990, Magellan imaged this impact crater that is representative of Venusian craters that are of the proper diameter (about 15 kilometers) to be 'transitional' in their morphology between 'complex' and irregular' craters.
In September 1990, Magellan imaged this impact crater that is representative of Venusian craters that are of the proper diameter (about 15 kilometers) to be 'transitional' in their morphology between 'complex' and irregular' craters.

Venus - 'Transitional' Crater

Currently displaying images 1-25 of 101
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