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Venerian - перевод на русский
[vi'ni(ə)riən]
существительное
общая лексика
венерианец
обитатель планеты Венера (в фантастике)
[vi'nju:ʒ(ə)n]
синоним
![boundary stone]] of [[Meli-Shipak II]], dating to the twelfth century BC.](https://commons.wikimedia.org/wiki/Special:FilePath/Kudurru Melishipak Louvre Sb23 n02.jpg?width=200 "boundary stone]] of [[Meli-Shipak II]], dating to the twelfth century BC.")
![High Altitude Venus Operational Concept (HAVOC)]] crewed floating outpost on Venus](https://commons.wikimedia.org/wiki/Special:FilePath/NASA Cloud City on Venus.jpg?width=200 "High Altitude Venus Operational Concept (HAVOC)]] crewed floating outpost on Venus")
![[[Impact crater]]s on the surface of Venus (false-colour image reconstructed from radar data)](https://commons.wikimedia.org/wiki/Special:FilePath/PIA00103 Venus - 3-D Perspective View of Lavinia Planitia.jpg?width=200 "[[Impact crater]]s on the surface of Venus (false-colour image reconstructed from radar data)")
![Mercury]], Venus,
Earth and [[Mars]])](https://commons.wikimedia.org/wiki/Special:FilePath/Terrestrial planet sizes2.jpg?width=200 "Mercury]], Venus,
Earth and [[Mars]])")
![[[2012 transit of Venus]], projected to a white card by a [[telescope]]](https://commons.wikimedia.org/wiki/Special:FilePath/Transit of Venus viewed in Wagga Wagga (2).jpg?width=200 "[[2012 transit of Venus]], projected to a white card by a [[telescope]]")
![Rectified and colourized surface image, [[Venera 10]] (1975)](https://commons.wikimedia.org/wiki/Special:FilePath/USSR Venera 10 Venus ground 1975 colorized by Don P. Mitchell.png?width=200 "Rectified and colourized surface image, [[Venera 10]] (1975)")
![Cloud structure of the Venusian atmosphere, made visible through [[ultraviolet]] imaging](https://commons.wikimedia.org/wiki/Special:FilePath/Venus - December 23 2016.png?width=200 "Cloud structure of the Venusian atmosphere, made visible through [[ultraviolet]] imaging")
.svg?width=200 "alt=A complex, spiral, floral pattern with five loops encircling the middle")
.svg?width=200 "♀")
Определение
Википедия
The terraforming of Venus or the terraformation of Venus is the hypothetical process of engineering the global environment of the planet Venus in order to make it suitable for human habitation. Adjustments to the existing environment of Venus to support human life would require at least three major changes to the planet's atmosphere:
- Reducing Venus's surface temperature of 737 K (464 °C; 867 °F)
- Eliminating most of the planet's dense 9.2 MPa (91 atm) carbon dioxide and sulfur dioxide atmosphere via removal or conversion to some other form
- The addition of breathable oxygen to the atmosphere.
These three changes are closely interrelated because Venus's extreme temperature is due to the high pressure of its dense atmosphere and the greenhouse effect.
