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Venera 13 and venera 14 spacecraft Stock Photos and Images

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Venera 13 and venera 14 spacecraft Stock Photos and Images

This global view of the surface of Venus is cantered 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. Simulated colour is used to enhance small-scale structure. The simulated hues are based on colour images recorded by the Soviet Venera 13 and 14 spacecraft. 1991 Stock Photo
RMD98X8G–This global view of the surface of Venus is cantered 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. Simulated colour is used to enhance small-scale structure. The simulated hues are based on colour images recorded by the Soviet Venera 13 and 14 spacecraft. 1991
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. Simulated color is used to inhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. Stock Photo
RM2AH3000–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. Simulated color is used to inhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft.
A volcano named Sapas Mons dominates this computer-generated view of the surface of Venus in image released June 30, 2005. Lava flows extend for hundreds of kilometers across the fractured plains shown in the foreground to the base of the mountain, which measures 248 miles across 0.9 mile high. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. The image was produced by the Solar System Visualization project and the Magellan Science team at the JPL Multimission Image Processing Laboratory. (UPI Photo/NASA/JPL) Stock Photo
RMW0M717–A volcano named Sapas Mons dominates this computer-generated view of the surface of Venus in image released June 30, 2005. Lava flows extend for hundreds of kilometers across the fractured plains shown in the foreground to the base of the mountain, which measures 248 miles across 0.9 mile high. The simulated hues are based on color images recorded by the Soviet Venera 13 and 14 spacecraft. The image was produced by the Solar System Visualization project and the Magellan Science team at the JPL Multimission Image Processing Laboratory. (UPI Photo/NASA/JPL)
MOSCOW, RUSSIA - SEPTEMBER 28, 2020: Postage stamp printed in Soviet Union shows Unmanned Interplanetary Space Flights of 'Venera-13 & 14', “Venera” S Stock Photo
RF2D5CTA9–MOSCOW, RUSSIA - SEPTEMBER 28, 2020: Postage stamp printed in Soviet Union shows Unmanned Interplanetary Space Flights of 'Venera-13 & 14', “Venera” S
A portion of western Eistla Regio is shown in this three dimensional, computer-generated view of the surface of Venus. The Stock Photo
RMD98X8J–A portion of western Eistla Regio is shown in this three dimensional, computer-generated view of the surface of Venus. The
The north pole is at the center of the image; with 0 degrees, 90 degrees , 180 degrees, 270 degrees east longitudes at 6, 3, 12 and 9 0'clock positions, repectively, of an imagery clock face. Magellan synthetic aperture radar mosaics from the first cycle of Magelolan mapping are mapped onto a computer-simulated globe to create this image. Data gaps are filled with Pioneere-Venus Orbiter data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 & 14 spacecraft. Stock Photo
RM2AH300R–The north pole is at the center of the image; with 0 degrees, 90 degrees , 180 degrees, 270 degrees east longitudes at 6, 3, 12 and 9 0'clock positions, repectively, of an imagery clock face. Magellan synthetic aperture radar mosaics from the first cycle of Magelolan mapping are mapped onto a computer-simulated globe to create this image. Data gaps are filled with Pioneere-Venus Orbiter data, or a constant mid-range value. Simulated color is used to enhance small-scale structure. The simulated hues are based on color images recorded by the Soviet Venera 13 & 14 spacecraft.
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