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Image Date Added Target Mission Instrument ID# Rating Views

NASA's ACRIMSAT Observes Venus Transit

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2012-06-15

Venus

ACRIMSAT

ACRIM3

PIA15820

2377

NASA's ACRIMSAT Observes Venus Transit

Observations of the total solar irradiance made with the ACRIM3 instrument on NASA's ACRIMSAT satellite on June 5 and 6, 2012, tracked the effect of the transit of Venus, which lasted about six hours.

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Surface Warmth on a Venus Volcano

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2010-04-08

Venus

Magellan, Venus Express

Visible and Infrared Thermal Imaging Spectrometer

PIA13001

12004

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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Mariner 2 (Artist's Concept)

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2003-06-27

Venus

Mariner

PIA04594

9503

Mariner 2 (Artist's Concept)

NASA's Mariner 2 was the world's first successful interplanetary spacecraft. Launched August 27, 1962, on an Atlas-Agena rocket, Mariner 2 passed within about 34,000 kilometers (21,000 miles) of Venus.

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Venus Hemispherical Globes (with place names)

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2001-08-27

Venus

Magellan

Arecibo Radar Data, Radar System

PIA03167

7672

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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Venus Hemispherical Globes

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2001-03-15

Venus

Magellan

Arecibo Radar Data, Radar System

PIA03151

6943

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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Venus Cloud Tops Viewed by Hubble

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1999-05-18

Venus

Hubble Space Telescope (HST)

Imaging Science Subsystem - Narrow Angle

PIA01544

13629

Venus Cloud Tops Viewed by Hubble

Venus Cloud Tops Viewed by Hubble. This is a NASA Hubble Space Telescope ultraviolet-light image of the planet Venus, taken on January 24 1995, when Venus was at a distance of 70.6 million miles (113.6 million kilometers) from Earth.

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

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1998-06-04

Venus

Magellan

Radar System

PIA00316

5758

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

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1998-06-04

Venus

Magellan

Radar System

PIA00315

5591

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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Sedna Planitia (Right Member of a Synthetic Stereo Pair)

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1998-06-04

Venus

Magellan

Radar System

PIA00314

5371

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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Sedna Planitia (Left Member of a Synthetic Stereo Pair)

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1998-06-04

Venus

Magellan

Radar System

PIA00313

5007

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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Currently displaying images 1-10 of 148
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