AP Biology class blog for discussing current research in Biology

Have There Ever Been Oceans on Earth’s Sister Planet?

Venus, commonly referred to as the volcanic planet, also known as Earth’s sister planet, is the second closest planet to the sun. The planet’s surface is currently known to be the hottest in the solar system due to its dense atmosphere which traps in an immense amount of heat. This characteristic of Venus is actually very similar to how Earth’s greenhouse effect traps in warm air, keeping our planet warm; however, Earth also has oceans that cool the atmosphere, thus allowing for life to flourish.  Recently, research has been conducted to get to the bottom of whether or not Venus has actually ever had oceans.

Venus dome 3D

From a distance, Earth and Venus are strikingly similar: both around the same size, with a rocky surface and an atmosphere. As mentioned previously, Venus’ atmosphere traps in far more heat than Earth’s. In addition to having a very thick CO2 atmosphere, Venus also has sulphuric acid clouds which Earth does not. Life simply cannot exist on Venus due to the intense atmospheric pressure and the extreme temperatures created by the trapped heat. An article by Charles Q. Choi and Chelsea Gohd entitled “Venus: The hot, hellish & volcanic planet” gives more information about the nature of Venus’s surface. Choi and Gohd stated that Venus has the heaviest atmosphere out of all the planets in the solar system which causes its pressure to be about 90 times that on Earth. They mentioned a similar study also exploring the possibility of oceans on Venus. It concludes that the ultraviolet radiation, from the sun, as it grew closer, caused the water vapor molecules in the atmosphere to split apart, thus allowing for the hydrogen molecules to escape into space. This was the cause of the build-up of CO2 in the atmosphere that then lead to the current-day conditions of the planet. Unlike Earth, Venus has very strong winds and is primarily a dry desert land with many active volcanoes. Contrastingly, Earth’s surface is 70% water and is covered with dirt and plants. We can understand the similarities between Earth and Venus when we dig underneath all that dirt and ocean. Earth happens to have the same rocky surface that Venus has that came from cooled lava billions of years ago. To learn more about Earth’s surface, click here.

Venus Earth Comparison Horizontal

Theories have formed that Venus was once a far more inviting planet with potential for life. The National Centre of Competence in Research (NCCR) PlanetS and the University of Geneva (UNIGE), leading a team of astrophysicists, thoroughly explored whether Venus could have actually experienced milder days. Unfortunately, according to the results of the study posted in the journal Nature, this was not the case. Martin Turbet and his team of astrophysicists used the tools available on Earth to come to a conclusion.  They created a three-dimensional simulation of both Earth and Venus in their early stages when their surfaces were still molten and any present-day water would have been vaporized. They used the simulation to then evaluate how the evolution of the plants would play out. By examining how the atmospheres evolved, they can determine whether or not it was possible for oceans to have formed in the process. Marcus Turbet concluded that “Thanks to our simulations, we were able to show that the climatic conditions did not allow water vapour to condense in the atmosphere of Venus.” Due to the level of heat in the planet’s atmosphere, the water vapor was never able to cool to the point where it would form water droplets and fall to the surface; therefore; it remained in the gaseous state and never formed oceans.

As we learned in AP Biology this year, water (H2O) plays a huge role in life on Earth and it makes sense that other planets, such as Venus, that lack liquid water, would not be able to support life. We discussed that one of water’s main properties moderating temperature. Due to water’s unusually high specific heat,  its temperature changes less when it loses or absorbs a certain amount of heat. Life can exist on Earth because Earth’s oceans are able to moderate and control any temperature fluctuations that happen on land to keep the atmosphere in ideal condition for life. Water also has a high heat of vaporization which, again, aids life on Earth. Oceans absorb heat, and as some water evaporates, it condenses and then falls back to Earth in the form of rain, thus cooling the surface. On a much smaller scale, this can be related to how humans sweat (sweat representing the oceans and humans representing a planet). I run a lot, which means that I also sweat a lot, especially in the summertime when the temperature starts to rise. The sweat being 99% water means that it offers the same cooling effects that pure water does. The liquid on the surface of my skin allows my body temperature to be lowered so I can still feel cool enough to continue on my run. Hopefully, this aids our understanding of how oceans could never have existed on Venus because the water vapor was unable to become cool enough to transform into its liquid state and moderate the temperature of the planet. Venus’s surface is left to be rocky and full of volcanoes while Earth’s surface is able to support an immense amount of life.

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1 Comment

  1. clalvincycle

    Very interesting fertilivization. The idea of water proving that there is life on other planets is very exciting to think about. Another planet which shares such similarities to Earth is Mars. An article by EarthSky details their discovery——. The joint European-Russian Trace Gas Orbiter (TGO), part of the ExoMars mission has discovered subsurface water ice in Valles Marineris on Mars, the largest canyon system in the solar system. The TGO identifies neutrons rather than using light because drier soils emit more neutrons than wetter ones. The subsurface ice on Mars is similar to the Earths Permafrost regions. Who knows; maybe there was life on mars in the past.

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