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This figure shows the volcanic peak Idunn Mons in the Imdr Regio area of Venus. The topographic backbone (brown color) was derived from data obtained by NASA's Magellan spacecraft and the overlay was derived from data from ESA's Venus Express Spacecraft.
This figure shows the volcanic peak Idunn Mons in the Imdr Regio area of Venus. The topographic backbone (brown color) was derived from data obtained by NASA's Magellan spacecraft and the overlay was derived from data from ESA's Venus Express Spacecraft.

Surface Warmth on a Venus Volcano

This figure shows the volcanic peak Idunn Mons in the Imdr Regio area of Venus. The topographic backbone (brown color) was derived from data obtained by NASA's Magellan spacecraft and the overlay was derived from data from ESA's Venus Express Spacecraft.

Target: Venus
Mission: Magellan, Venus Express
Spacecraft: Magellan, Venus Express
Instrument: Visible and Infrared Thermal Imaging Spectrometer
ID#: PIA13001
Added: 2010-04-08

Views: 9480

Surface Warmth on a Venus Volcano

This figure shows the volcanic peak Idunn Mons in the Imdr Regio area of Venus. The topographic backbone (brown color) was derived from data obtained by NASA's Magellan spacecraft and the overlay was derived from data from ESA's Venus Express Spacecraft.

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The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.
The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.

Venus Hemispherical Globes (with place names)

The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.

Target: Venus
Mission: Magellan
Spacecraft: Arecibo Observatory, Magellan, Pioneer Venus Orbiter
Instrument: Arecibo Radar Data, Radar System
ID#: PIA03167
Added: 2001-08-27

Views: 6813

Venus Hemispherical Globes (with place names)

The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.

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The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.
The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.

Venus Hemispherical Globes

The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.

Target: Venus
Mission: Magellan
Spacecraft: Arecibo Observatory, Magellan, Pioneer Venus Orbiter
Instrument: Arecibo Radar Data, Radar System
ID#: PIA03151
Added: 2001-03-15

Views: 6145

Venus Hemispherical Globes

The images used for the base of this globe show the northern and southern hemispheres of Venus as revealed by more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.

Looking Westward Across the Fortuna Tessera (Right Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00316
Added: 1998-06-04

Views: 5241

Looking Westward Across the Fortuna Tessera (Right Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.

Looking Westward Across the Fortuna Tessera (Left Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00315
Added: 1998-06-04

Views: 5101

Looking Westward Across the Fortuna Tessera (Left Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, is a look westward across the Fortuna Tessera toward the slopes of Maxwell Montes.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.

Sedna Planitia (Right Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00314
Added: 1998-06-04

Views: 4758

Sedna Planitia (Right Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia. Circular depressions with associated fracture patterns, called 'coronae.'
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia. Circular depressions with associated fracture patterns, called 'coronae.'

Sedna Planitia (Left Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia. Circular depressions with associated fracture patterns, called 'coronae.'

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00313
Added: 1998-06-04

Views: 4475

Sedna Planitia (Left Member of a Synthetic Stereo Pair)

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia. Circular depressions with associated fracture patterns, called 'coronae.'

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the impact crater Markham, named after the English aviator Beryl Markham.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the impact crater Markham, named after the English aviator Beryl Markham.

Magellan's View of Crater Markham, 0° N, 163° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the impact crater Markham, named after the English aviator Beryl Markham.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00312
Added: 1998-06-04

Views: 5062

Magellan's View of Crater Markham, 0° N, 163° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the impact crater Markham, named after the English aviator Beryl Markham.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Region.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Region.

Magellan's Perspective View of Ovda Regio, 0° S, 129° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Region.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00311
Added: 1998-06-04

Views: 5122

Magellan's Perspective View of Ovda Regio, 0° S, 129° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Region.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.

Magellan's Perspective View of Ovda Regio, 0° N, 129° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00310
Added: 1998-06-04

Views: 7803

Magellan's Perspective View of Ovda Regio, 0° N, 129° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.

Magellan's Perspective View of Ovda Regio, 0° N, 77° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00309
Added: 1998-06-04

Views: 4581

Magellan's Perspective View of Ovda Regio, 0° N, 77° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows the boundary between the lowland plains and characteristic Venusian highland terrain in Ovda Regio.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowlands to the north of Ovda Regio. The prominent topographic feature is a shield volcano.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowlands to the north of Ovda Regio. The prominent topographic feature is a shield volcano.

Magellan's Perspective View of Ovda Regio, 15° N, 77° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowlands to the north of Ovda Regio. The prominent topographic feature is a shield volcano.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00308
Added: 1998-06-04

Views: 7954

Magellan's Perspective View of Ovda Regio, 15° N, 77° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowlands to the north of Ovda Regio. The prominent topographic feature is a shield volcano.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.

Magellan's Perspective View of Sedna Planitia, 45° N, 11° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00307
Added: 1998-06-04

Views: 6456

Magellan's Perspective View of Sedna Planitia, 45° N, 11° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of the lowland plains in Sedna Planitia.

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This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of Sedna Planitia and illustrates a common phenomenon of the lowland plains of Venus.
This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of Sedna Planitia and illustrates a common phenomenon of the lowland plains of Venus.

Magellan's Perspective View of Sedna Planitia, 45° N, 350° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of Sedna Planitia and illustrates a common phenomenon of the lowland plains of Venus.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00306
Added: 1998-06-04

Views: 5825

Magellan's Perspective View of Sedna Planitia, 45° N, 350° E

This perspective view of Venus, generated by computer from NASA's Magellan data and color-coded with emissivity, shows part of Sedna Planitia and illustrates a common phenomenon of the lowland plains of Venus.

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The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 270 degrees east longitude.
The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 270 degrees east longitude.

Hemispheric View of Venus Centered at 270° East Longitude

The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 270 degrees east longitude.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00160
Added: 1998-06-04

Views: 6704

Hemispheric View of Venus Centered at 270° East Longitude

The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 270 degrees east longitude.

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The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 180 degrees east longitude.
The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 180 degrees east longitude.

Hemispheric View of Venus Centered at 180° East Longitude

The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 180 degrees east longitude.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00159
Added: 1998-06-04

Views: 7791

Hemispheric View of Venus Centered at 180° East Longitude

The view of Venus, after more than a decade of radar investigations culminating in the 1990-1994 NASA Magellan mission, is centered at 180 degrees east longitude.

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The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 90 degrees east longitude.
The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 90 degrees east longitude.

Hemispheric View of Venus Centered at 90 Degrees East Longitude

The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 90 degrees east longitude.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00158
Added: 1998-06-04

Views: 7687

Hemispheric View of Venus Centered at 90 Degrees East Longitude

The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 90 degrees east longitude.

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The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 0 degrees east longitude.
The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 0 degrees east longitude.

Hemispheric View of Venus Centered at 0 Degrees East Longitude

The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 0 degrees east longitude.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00157
Added: 1998-06-04

Views: 9059

Hemispheric View of Venus Centered at 0 Degrees East Longitude

The hemispheric view of Venus, as revealed by more than a decade of radar investigations culminating in NASA's 1990-1994 Magellan mission, is centered at 0 degrees east longitude.

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The view from NASA's Magellan spacecraft shows a 100-km-wide nova superposed on Yavine Corona. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.
The view from NASA's Magellan spacecraft shows a 100-km-wide nova superposed on Yavine Corona. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

Nova Superposed on Yavine Corona

The view from NASA's Magellan spacecraft shows a 100-km-wide nova superposed on Yavine Corona. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00150
Added: 1998-06-04

Views: 386

Nova Superposed on Yavine Corona

The view from NASA's Magellan spacecraft shows a 100-km-wide nova superposed on Yavine Corona. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

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The view from NASA's Magellan spacecraft shows most of Galindo (V-40) quadrangle looking east; Atete Corona, in the foreground, is a 600-km-long and about 450-km-wide, circular volcano-tectonic feature.
The view from NASA's Magellan spacecraft shows most of Galindo (V-40) quadrangle looking east; Atete Corona, in the foreground, is a 600-km-long and about 450-km-wide, circular volcano-tectonic feature.

Three-dimensional perspective views of Venusian Terrains composed of reduced resolution left-looking synthetic-aperture radar images merged with altimetry data from the Magellan spacecraft.

The view from NASA's Magellan spacecraft shows most of Galindo (V-40) quadrangle looking east; Atete Corona, in the foreground, is a 600-km-long and about 450-km-wide, circular volcano-tectonic feature.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00096
Added: 1998-06-03

Views: 524

Three-dimensional perspective views of Venusian Terrains composed of reduced resolution left-looking synthetic-aperture radar images merged with altimetry data from the Magellan spacecraft.

The view from NASA's Magellan spacecraft shows most of Galindo (V-40) quadrangle looking east; Atete Corona, in the foreground, is a 600-km-long and about 450-km-wide, circular volcano-tectonic feature.

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The view from NASA's Magellan spacecraft shows part of Galindo (V40) quadrangle looking north; Nagavonyi Corona is in the foreground. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.
The view from NASA's Magellan spacecraft shows part of Galindo (V40) quadrangle looking north; Nagavonyi Corona is in the foreground. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

Three-dimensional perspective views of Venusian Terrains composed of reduced resolution left-looking synthetic-aperture radar images merged with altimetry data from the Magellan spacecraft.

The view from NASA's Magellan spacecraft shows part of Galindo (V40) quadrangle looking north; Nagavonyi Corona is in the foreground. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00095
Added: 1998-06-03

Views: 532

Three-dimensional perspective views of Venusian Terrains composed of reduced resolution left-looking synthetic-aperture radar images merged with altimetry data from the Magellan spacecraft.

The view from NASA's Magellan spacecraft shows part of Galindo (V40) quadrangle looking north; Nagavonyi Corona is in the foreground. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

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The view from NASA's Magellan spacecraft shows Yavine Corona, looking northeast. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.
The view from NASA's Magellan spacecraft shows Yavine Corona, looking northeast. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

Close-up View of Yavine Corona

The view from NASA's Magellan spacecraft shows Yavine Corona, looking northeast. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00098
Added: 1998-06-03

Views: 428

Close-up View of Yavine Corona

The view from NASA's Magellan spacecraft shows Yavine Corona, looking northeast. Coronae are roughly circular, volcanic features believed to form over hot upwellings of magma within the Venusian mantle.

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This view from NASA' Magellan spacecraft is a close-up of Atete Corona, a 600-km-long and 450-km-wide feature at latitude 16 degrees S., longitude 244 degrees; looking north.
This view from NASA' Magellan spacecraft is a close-up of Atete Corona, a 600-km-long and 450-km-wide feature at latitude 16 degrees S., longitude 244 degrees; looking north.

Close-up View of Atete Corona

This view from NASA' Magellan spacecraft is a close-up of Atete Corona, a 600-km-long and 450-km-wide feature at latitude 16 degrees S., longitude 244 degrees; looking north.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00097
Added: 1998-06-03

Views: 469

Close-up View of Atete Corona

This view from NASA' Magellan spacecraft is a close-up of Atete Corona, a 600-km-long and 450-km-wide feature at latitude 16 degrees S., longitude 244 degrees; looking north.

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A portion of Alpha Regio is displayed in this three-dimensional perspective view of the surface of Venus from NASA's Magellan spacecraft. In 1963, Alpha Regio was the first feature on Venus to be identified from Earth-based radar.
A portion of Alpha Regio is displayed in this three-dimensional perspective view of the surface of Venus from NASA's Magellan spacecraft. In 1963, Alpha Regio was the first feature on Venus to be identified from Earth-based radar.

Venus - Three-Dimensional Perspective View of Alpha Regio

A portion of Alpha Regio is displayed in this three-dimensional perspective view of the surface of Venus from NASA's Magellan spacecraft. In 1963, Alpha Regio was the first feature on Venus to be identified from Earth-based radar.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00481
Added: 1996-12-02

Views: 9353

Venus - Three-Dimensional Perspective View of Alpha Regio

A portion of Alpha Regio is displayed in this three-dimensional perspective view of the surface of Venus from NASA's Magellan spacecraft. In 1963, Alpha Regio was the first feature on Venus to be identified from Earth-based radar.

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Crater Isabella is seen in this radar image from NASA's Magellan spacecraft. The second largest impact crater on Venus, the crater is named in honor of the 15th Century queen of Spain, Isabella of Castile.
Crater Isabella is seen in this radar image from NASA's Magellan spacecraft. The second largest impact crater on Venus, the crater is named in honor of the 15th Century queen of Spain, Isabella of Castile.

Venus - Impact Crater 'Isabella

Crater Isabella is seen in this radar image from NASA's Magellan spacecraft. The second largest impact crater on Venus, the crater is named in honor of the 15th Century queen of Spain, Isabella of Castile.

Target: Venus
Mission: Magellan
Spacecraft: Magellan
Instrument: Radar System
ID#: PIA00480
Added: 1996-11-26

Views: 5839

Venus - Impact Crater 'Isabella

Crater Isabella is seen in this radar image from NASA's Magellan spacecraft. The second largest impact crater on Venus, the crater is named in honor of the 15th Century queen of Spain, Isabella of Castile.

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