The surface of Venus is dominated by geologic features that include volcanoes, large impact craters, and aeolian erosion and sedimentation landforms. Venus... 22 KB (2,743 words) - 10:27, 5 May 2024 |
and bulk composition (Venus is both the closest planet to Earth and the planet closest in size to Earth). The surface of Venus is covered by a dense atmosphere... 72 KB (184 words) - 14:33, 30 January 2024 |
dioxide into a supercritical state close to Venus's surface. Internally, Venus has a core, mantle, and crust. Venus lacks an internal dynamo, and its weak... 214 KB (19,463 words) - 14:16, 8 May 2024 |
Water on Venus refers to the hypothesis that water was once on the surface of the planet Venus. Scientists and authors long proposed Venus was habitable... 13 KB (1,362 words) - 19:05, 4 April 2024 |
Venus snow is a brightening of the radar reflection from the surface of Venus at high elevations. The "snow" appears to be a mineral condensate of lead(II)... 5 KB (501 words) - 15:23, 4 January 2024 |
The surface of Venus is dominated by volcanic features and has more volcanoes than any other planet in the Solar System. It has a surface that is 90%... 31 KB (3,786 words) - 20:48, 6 March 2024 |
The geology of Venus is the scientific study of the surface, crust, and interior of the planet Venus. Within the Solar System, it is the one nearest to... 50 KB (6,395 words) - 03:32, 3 April 2024 |
presence of mountain ranges on Venus may provide evidence that the planet's surface is in motion. Key DIAM — Longest dimension of feature in kilometres AS —... 24 KB (176 words) - 19:49, 25 April 2024 |
list of named coronae on Venus. With a few exceptions, cytherean coronae are named after fertility and earth goddesses. List of montes on Venus List of craters... 29 KB (64 words) - 15:32, 4 March 2022 |
The atmosphere of Venus is the very dense layer of gasses surrounding the planet Venus. Venus's atmosphere is composed of 96.5% carbon dioxide and 3.5%... 92 KB (10,568 words) - 09:49, 22 April 2024 |
Ishtar Terra (redirect from The northern continent of Ishtar) Terra /ˈɪʃtɑːr ˈtɛrə/ is the second largest of the three continental terrae regions on the planet Venus, the others being Aphrodite Terra and Lada Terra... 4 KB (356 words) - 17:36, 23 August 2023 |
Aphrodite Terra (redirect from The southern continent of Aphrodia) view of the surface of Venus from space (Parker Solar Probe, July 2020) Parker Solar Probe images showing features on the Venusian surface, such as the... 5 KB (535 words) - 15:47, 27 September 2023 |
: 164 Venus has a thick layer of clouds that prevents telescopic observation of the surface, giving writers free rein to imagine any kind of world below... 64 KB (5,871 words) - 21:08, 20 April 2024 |
Arachnoid (astrogeology) (category Surface features of Venus) are of unknown origin, and have been found only on the surface of the planet Venus. They appear as concentric ovals surrounded by a complex network of fractures... 3 KB (281 words) - 23:49, 30 July 2023 |
Phoebe Regio (category Surface features of Venus) the planet Venus. It lies to the southeast of Asteria Regio. It is 2,852 kilometres (1,772 mi) in diameter and is the principal feature of the V41 quadrangle... 1 KB (87 words) - 09:16, 20 October 2023 |
with the discovery of Venus's extremely hostile surface environment, attention has largely shifted towards the colonization of the Moon and Mars instead... 18 KB (1,987 words) - 22:05, 1 May 2024 |
planets, but the surface of Venus is obscured by an atmosphere opaque to visible light. As one of the brightest objects in the sky, Venus has been known... 80 KB (6,932 words) - 03:17, 3 March 2024 |
Channel (geography) (redirect from Channel (body of water)) The term is also traditionally used to describe the waterless surface features on Venus. Channel initiation refers to the site on a mountain slope where... 11 KB (1,274 words) - 12:43, 9 May 2024 |
Lada Terra (category Surface features of Venus) realizing relative ages of the extensional belts and coronae, as well as the complex tesserae features present planet-wide. In 1990 the Venus Radar Mapper revealed... 15 KB (1,764 words) - 10:33, 5 May 2024 |
Magellan (spacecraft) (redirect from Venus Radar Mapper) 282 lb) robotic space probe launched by NASA of the United States, on May 4, 1989, to map the surface of Venus by using synthetic-aperture radar and to measure... 46 KB (4,620 words) - 15:16, 5 May 2024 |
Sedna Planitia (category Surface features of Venus) Sedna Planitia is a large lowland area of Venus, south of Ishtar Terra. It is thought to be lava-covered and similar to a lunar mare. Its name is derived... 2 KB (138 words) - 09:07, 25 April 2024 |
Alpha Regio (category Surface features of Venus) exceptions to the rule that the surface features of Venus are to be named for females: women or goddesses. The surface of the region is what is known as... 3 KB (295 words) - 03:22, 13 February 2020 |
Minona Corona (category Surface features of Venus) Minona Corona is a corona found on the planet Venus at 23°30′N 218°30′E / 23.5°N 218.5°E / 23.5; 218.5. It is located in quadrangle V-27 (Ulfrun Regio)... 1 KB (92 words) - 06:01, 5 March 2021 |
Beta Regio (category Surface features of Venus) and Beta Regio are the three exceptions to the rule that the surface features of Venus are to be named for women or goddesses. Volcanic rises are broad... 2 KB (272 words) - 08:36, 15 January 2024 |
characterize the atmosphere and surface of Venus. It continued to transmit data until October 1992. The Pioneer Venus Multiprobe deployed four small probes... 8 KB (803 words) - 23:36, 22 April 2024 |
Dali Chasma (category Surface features of Venus) Diana Chasma system consist of deep troughs that extend for 7,400 kilometers (4,600 mi) and are very distinct features on Venus. Those chasma connect the... 1 KB (126 words) - 10:25, 5 May 2024 |