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2. Atmosphere of Venus - Wikipedia

   en.wikipedia.org/wiki/Atmosphere_of_Venus

   The early Earth during the Hadean eon is believed by most scientists to have had a Venus-like atmosphere, with roughly 100 bar of CO 2 and a surface temperature of 230 °C, and possibly even sulfuric acid clouds, until about 4.0 billion years ago, by which time plate tectonics were in full force and together with the early water oceans, removed ...

3. The discovery of a possible sign of life in Venus’ clouds ...

   www.aol.com/venus-atmosphere-shows-potential...

   Researchers’ detection of two gases, phosphine and ammonia, in the clouds of Venus raises speculation about possible life forms in the planet’s atmosphere.

4. Atmospheric super-rotation - Wikipedia

   en.wikipedia.org/wiki/Atmospheric_super-rotation

   The initial observations of Venus' super rotation were Earth-based. Modern GCM models and observations are often enhanced by looking at past ancient climates. In a model where Venus is assumed to have an atmospheric mass similar to Earth, SS-AS circulation could have dominated over super-rotation in an ancient thinner atmosphere. [2]

5. Scientists detect oxygen in noxious atmosphere of Venus - AOL

   www.aol.com/news/scientists-detect-oxygen...

   Its thick and noxious atmosphere is dominated by carbon dioxide - 96.5% - with lesser amounts of nitrogen and trace gases. In fact, with Venus getting far less scientific attention than other ...

6. Water on Venus - Wikipedia

   en.wikipedia.org/wiki/Water_on_Venus

   This means the habitable zone was stretched from Venus to Earth (and possibly to Mars), before eventually Solar maxima began creating greenhouse gases in Venus’ atmosphere, making the atmosphere thicker, evaporating away all liquid water on the planets surface. Studies have proven that Venus needed liquid water three billion years ago to be ...

7. Why isn’t Venus like Earth? New space mission aims to find out

   www.aol.com/space-missions-probe-mysteries-venus...

   The EnVision Venus explorer will study that planet in unprecedented detail, from inner core to the top of its atmosphere, to help astronomers understand why the hot, toxic world didn’t turn out ...

8. Water on terrestrial planets of the Solar System - Wikipedia

   en.wikipedia.org/wiki/Water_on_terrestrial...

   The current Venusian atmosphere has only ~200 mg/kg H 2 O(g) in its atmosphere and the pressure and temperature regime makes water unstable on its surface. Nevertheless, assuming that early Venus's H 2 O had a ratio between deuterium (heavy hydrogen, 2H) and hydrogen (1H) similar to Earth's Vienna Standard Mean Ocean Water of 1.6×10 −4, [7] the current D/H ratio in the Venusian atmosphere ...

9. The Plan to Look for Life on Venus—Without NASA

   www.aol.com/news/plan-look-life-venus-without...

   Photo Illustration by Elizabeth Brockway/The Daily Beast/NASAVenus is a nasty planet. Thick layers of high-pressure, sulfuric clouds cover a very hot volcanic surface, which can rise up to as high ...