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License = https://en.wikipedia.org/wiki/File:PIA23791-Venus-NewlyProcessedView-20200608.jpg
Title = Venus is the second planet from the Sun. It is named after the Roman goddess of love and beauty. As the second-brightest natural object in Earth's night sky after the Moon, Venus can cast shadows and can be, on rare occasion, visible to the naked eye in broad daylight.0x005B150x005D0x005B160x005D Venus lies within Earth's orbit, and so never appears to venture far from the Sun, either setting in the west just after dusk or rising in the east a bit before dawn.
URL = https://upload.wikimedia.org/wikipedia/commons/a/a9/PIA23791-Venus-NewlyProcessedView-20200608.jpg
2_CompareEarth/License = https://en.wikipedia.org/wiki/File:Venus,_Earth_size_comparison.jpg
2_CompareEarth/Title = Size comparison of Venus (using a false-colour, radar-based image of the surface) and Earth
2_CompareEarth/URL = https://upload.wikimedia.org/wikipedia/commons/9/92/Venus,_Earth_size_comparison.jpg
3_Rotation_1_Topographic/License = https://en.wikipedia.org/wiki/File:Topographic_Globe_of_Venus.gif
3_Rotation_1_Topographic/Title = Topographic Globe of Venus from Magellan radar altimetry data
3_Rotation_1_Topographic/URL = https://upload.wikimedia.org/wikipedia/commons/0/0b/Topographic_Globe_of_Venus.gif
3_Rotation_2_Radar/License = https://en.wikipedia.org/wiki/File:Radar_Globe_of_Venus.gif
3_Rotation_2_Radar/Title = Radar map of Venus
3_Rotation_2_Radar/URL = https://upload.wikimedia.org/wikipedia/commons/8/8b/Radar_Globe_of_Venus.gif
4_LaviniaPlanitia/License = https://en.wikipedia.org/wiki/File:PIA00103_Venus_-_3-D_Perspective_View_of_Lavinia_Planitia.jpg
4_LaviniaPlanitia/Title = Impact craters on the surface of Venus (false-colour image reconstructed from radar data). Three impact craters are displayed in this three-dimensional perspective view of the surface of Venus. The center of the image is located at approximately 27 degrees south latitude, 339 degrees east longitude in the northwestern portion of Lavinia Planitia. Magellan synthetic aperture radar data is combined with radar altimetry to develop a three-dimensional map of the surface.
4_LaviniaPlanitia/URL = https://upload.wikimedia.org/wikipedia/commons/6/60/PIA00103_Venus_-_3-D_Perspective_View_of_Lavinia_Planitia.jpg
5_RadarView/License = https://en.wikipedia.org/wiki/File:Venus_globe.jpg
5_RadarView/Title = False-color global radar view of Venus (without the clouds) from Magellan between 1990 and 1994. 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. Simulated color is used to enhance small-scale structure. 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 and is a single frame from a video released at the October 29, 1991, JPL news conference. It is important to note that Venus is completely shrouded in clouds. A bright elongated region in the center is Aphrodite Terra.
5_RadarView/URL = https://upload.wikimedia.org/wikipedia/commons/8/85/Venus_globe.jpg
6_FromEarth/License = https://en.wikipedia.org/wiki/File:Venus-pacific-levelled.jpg
6_FromEarth/Title = Venus reflected on the Pacific Ocean. Venus, pictured center-right, is always brighter than all other planets or stars as seen from Earth. Jupiter is visible at the top of the image.
6_FromEarth/URL = https://upload.wikimedia.org/wikipedia/commons/5/52/Venus-pacific-levelled.jpg
7_GroundVenera9/License = https://en.wikipedia.org/wiki/File:Foto_de_Venera_9.png
7_GroundVenera9/Title = Image of the surface of Venus taken by Venera 9 in 1975. 
7_GroundVenera9/URL = https://upload.wikimedia.org/wikipedia/commons/f/ff/Foto_de_Venera_9.png
90_Explore_1_Vega2/License = https://en.wikipedia.org/wiki/File:Vega_model_-_Udvar-Hazy_Center.JPG
90_Explore_1_Vega2/Title = Vega solar system probe bus and landing apparatus (model) 
90_Explore_1_Vega2/URL = https://upload.wikimedia.org/wikipedia/commons/5/52/Vega_model_-_Udvar-Hazy_Center.JPG
90_Explore_1_Vega2_2_Balloon/License = https://en.wikipedia.org/wiki/File:Russian_"Vega"_balloon_mission_to_Venus_on_display_at_the_Udvar-Hazy_museum.jpg
90_Explore_1_Vega2_2_Balloon/Title = Russian "Vega" balloon mission to the atmosphere of Venus on display at the Steven F. Udvar-Hazy Center of the Smithsonian Institution. 
90_Explore_1_Vega2_2_Balloon/URL = https://upload.wikimedia.org/wikipedia/commons/3/33/Russian_"Vega"_balloon_mission_to_Venus_on_display_at_the_Udvar-Hazy_museum.jpg
90_Explore_3_VEX/License = https://en.wikipedia.org/wiki/File:Venus_Express_in_orbit_(crop).jpg
90_Explore_3_VEX/Title = Venus Express (VEX) was the first Venus exploration mission of the European Space Agency (ESA). Launched in November 2005, it arrived at Venus in April 2006 and began continuously sending back science data from its polar orbit around Venus. Equipped with seven scientific instruments, the main objective of the mission was the long term observation of the Venusian atmosphere. The observation over such long periods of time had never been done in previous missions to Venus.
90_Explore_3_VEX/URL = https://upload.wikimedia.org/wikipedia/commons/0/0b/Venus_Express_in_orbit_(crop).jpg
90_Explore_4_Akatsuki/License = https://en.wikipedia.org/wiki/File:H-IIA_F17_launching_AKATSUKI.jpg
90_Explore_4_Akatsuki/Title = H-IIA Launch Vehicle Flight 17, launching Venus Climate Orbiter "AKATSUKI".
90_Explore_4_Akatsuki/URL = https://upload.wikimedia.org/wikipedia/commons/f/fb/H-IIA_F17_launching_AKATSUKI.jpg

Edit single sub keys only: 2_CompareEarth / 3_Rotation_1_Topographic / 3_Rotation_2_Radar / 4_LaviniaPlanitia / 5_RadarView / 6_FromEarth / 7_GroundVenera9 / 90_Explore_1_Vega2 / 90_Explore_1_Vega2_2_Balloon / 90_Explore_3_VEX / 90_Explore_4_Akatsuki / License / Title / URL

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