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21 hours ago · Venus is the second planet from the Sun.It is a terrestrial planet and is the closest in mass and size to its orbital neighbour Earth.Venus is notable for having the densest atmosphere of the terrestrial planets, composed mostly of carbon dioxide with a thick, global sulfuric acid cloud cover.
3 days ago · Venus’s mean radius is 6,051.8 km (3,760.4 miles), or about 95 percent of Earth’s at the Equator, while its mass is 4.87 × 10 24 kg, or 81.5 percent that of Earth. The similarities to Earth in size and mass produce a similarity in density—5.24 grams per cubic centimetre for Venus, compared with 5.52 for Earth.
- Venus and Earth share similarities in their masses, sizes, densities, and relative locations in the solar system. Since they were presumably formed...
- Venus orbits the Sun at a mean distance of 108 million km (67 million miles), which is about 0.7 times Earth's distance from the Sun.
- When viewed through a telescope, Venus presents a brilliant yellow-white and a featureless face to the observer. Its obscured appearance results fr...
- Venus's mean radius is 6,051.8 km (3,760.4 miles), or about 95 percent of Earth's at the Equator, while its mass is 4.87 × 1024 kg, or 81.5 percent...
- Venus has the most massive atmosphere of all the terrestrial planets. Its gaseous envelope is composed of more than 96 percent carbon dioxide and 3...
3 hours ago · A strange, gargantuan wall of acid-filled clouds on our neighboring planet Venus has been spotted by a hobbyist astronomer. This structure, known as the Venus Cloud Discontinuity, is around 5,000 ...
- 56 sec
- Jess Thomson
3 days ago · Venus - Atmosphere, Surface, Evolution: Much less is known about the interior of Venus than about its surface and atmosphere. Nevertheless, because the planet is much like Earth in overall size and density and because it presumably accreted from similar materials (see solar system: Origin of the solar system), scientists expect that it evolved at least a crudely similar internal state.
1 day ago · The small number of impact craters on Venus (~1,000) indicates that their contribution to resurfacing is minor. Volcanism and tectonics are the principal geological processes operating on Venus during its observable geologic history.Landforms of the volcanic and tectonic nature have specific morphologies, which indicate different modes of formation, and their relationships permit one to ...
3 days ago · Venus - Atmosphere, Greenhouse, Gases: Venus has the most massive atmosphere of the terrestrial planets, which include Mercury, Earth, and Mars. Its gaseous envelope is composed of more than 96 percent carbon dioxide and 3.5 percent molecular nitrogen. Trace amounts of other gases are present, including carbon monoxide, sulfur dioxide, water vapour, argon, and helium. The atmospheric pressure ...
4 days ago · The surface of Venus is a nightmarish place, with 100 times the atmospheric pressure of Earth and temperatures high enough to melt lead. It's also still volcanically active, and it rains sulfuric ...
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