My World of Moisture

Tag: Mars

A Question of Moisture and Space

On October 4th somebody from my past got in touch through LinkedIn. We used to work at Delta Biotechnology in Nottingham, didn’t really know each other that well and not had any contact since about 1990. After exchanging messages, a few weeks later I asked my newly reintroduced contact if there was any topic on moisture he would like to see written as an article. That has led me to write this today because something that is interesting for one person is probably relevant and worth writing about for other people.

Before I get started on the topic, let me introduce Michael Geisow, a protein chemist who has reinvented himself as an author. Michael’s first novel is a modern psychological drama around social networking and artificial intelligence: a data expert, a healthcare evangelist, a dodgy psychologist and others including the devious Tuula Pippi. Available on Amazon.

The first thing Michael asked about was condensation on the outside of double glazed windows but dry inside. An easy one really and it’s all about temperature. Condensation like this occurs when high humidity air immediately above the glass surface is cooled taking the relative humidity to 100%. At this point water vapour in the air turns to liquid and forms droplets on the glass. Warmer air around the inner glass pane of the double glazing keeps the moisture in the air as a gas.

Michael’s second question on condensation is trickier. He described outside balustrade panels only having condensation on one side even though both sides are exposed to the same air conditions. I can see his scientific brain at work on this question. Something does not add up! No easy answer this time without further investigation. One unlikely possibility is that one side of the panels is warmer for some reason, but in the open air, natural circulation should be redistributing the temperature. Balustrade panels are made with reinforced glass for safety reasons. Perhaps one side of the glass is coated preventing water droplets forming. Even though a very thin layer of moisture will be present on the coated side, from casual observation, condensation on the other side will be all that is seen. A case where more information is needed to solve this one.

A day later after the condensation questions arrived, a question from Michael about looking for moisture on other planets. I’m not quite sure what Michael had in mind, but this gives me an opportunity to talk about life on other planets and their moons.

Starting in Autumn 2020 I signed up for the Open University course S283 Planetary science and the search for life. The course was split into two parts, one on our Solar System and the other on Astrobiology. I thoroughly enjoyed the whole experience even when having to attend online tutorials and complete assignments that were continuously assessed.

Moisture is present in vast quantities throughout our Solar System. Space scientists and astrobiologists generally work from what we understand about our Earth. Life in the form of microorganisms is found in the most extreme conditions on Earth. Logically we use our planet as a model system to look for life on other planets and moons in our Solar System. One of the driest places on Earth is the Atacama Desert in Chile.

Microbiologists have studied the bacteria and fungi from this region since the 1960’s. But in 2003, NASA published a paper describing Atacama as a model for Mars. That kicked off intense interest in engineering and scientific activity to mimic how to perform tests on the Martian terrain. Let’s start with “Is there water on Mars?” Pictures from the Mars missions compared to geographical features on Earth, indicate strongly that liquid water once flowed on the surface of Mars. Features that look just like riverbeds and erosion by water. We know for sure that water in the form of ice sits at the North and South poles of Mars. Also, there may be water deep underground. Future missions are planned to provide some answers.

As far As far as we know, water is a prerequisite for life. On Earth no life exists that does not rely on water. Back to the arid Atacama Desert. Engineers and scientists have designed machines and testing techniques to detect the presence of microbes in this desolate part of our world. The technology will be placed on board Mars missions and the data from the tests will be beamed back to Earth.

Related to this is a fact that has been known for many years. Microbes do not grow when the relative humidity of the air gets below 60%. In my eBook A Wetter Look At Climate Change and the section related to food, there is a table that shows the lowest %RH for the organisms is 61%. Recent studies on the microbes from Atacama and other arid parts of our planet have shown that there appears to be an absolute limit of 60.5 %RH for growth. For example, a paper published in 2014 with the title: Multiplication of microbes below 0.690 water activity: implications for terrestrial and extraterrestrial life and written as an international collaboration. One of the groups is the Institute for Global Food Security, School of Biological Sciences, Queen’s University Belfast and another is the UK Centre for Astrobiology, School of Physics and Astronomy, University of Edinburgh. So, you can see how things are interrelated. The other co-authors come from NASA, Germany, The Netherlands Italy and France. By the way, you have to multiply the “water activity” in the title of the paper by 100 to get the %RH for growth.

Atacama gets less than 2mm annual rain and has an average %RH of 10, classifying this desert as the driest place on Earth. Fog drifting in from the coast and around the coastal range of mountains into the desert provides microbes with the necessary moisture to keep them alive. These highly specialised organisms live in rocks containing salt. The salt in the rocks attracts moisture that is scavenged by the microbes. The interaction between salt and moisture is also a section in my eBook.

I’ll finish this article with one of my ‘mad’ ideas! On board a future exploratory mission to Mars a humidifier-dehumidifier should be set up to adjust the %RH around soil samples. Based on what we know from Earth, exposing soil to above 60%RH should encourage any viable microbes to grow. A range of temperatures and relative humidity would be needed to discover the growth requirements of these organisms. Soil samples will need to be taken from depths below the Martian surface as Solar radiation has most likely destroyed any past living entity on the surface.  Rock is a good shield against penetrating radiation.

Why is this simple idea ‘mad’? There are protocols in place for limiting risk of Why is this simple idea ‘mad’? There are protocols in place for limiting risk of contamination of extra-terrestrial bodies from space missions known as COSPAR which is a committee of scientists (Committee on Space Research). In Category IV, the second most stringent, covers a mission for “studying chemical evolution and/or origin of life, or for which scientific opinion provides a significant chance of contamination that could jeopardize a future biological experiment”. Perhaps transporting water, even though sterile, and encouraging growth of microbes is against the protocol.

The idea is so simple that it must have been thought about, yes?

I write about how humidity and moisture effects everything around us. If you would like to hear more on the impact of moisture, various topics on moisture and humidity are discussed in my eBook “A Wetter Look At Climate Change”.

Life on Mars

Being old enough to remember when David Bowie brought out “Life on Mars” and watching him on Top Of The Pops, it’s great to see the renewed fascination with this planet. We get headlines about the findings from the various missions circling around and landing on the Mars surface. Behind those headlines there’s a fantastic amount of science going on that we don’t hear about unless you’re really into space exploration. Astrobiology is the area of science I’m drawing from to write this blog post. Especially about the limits for microbes to grow and how they get their water…….

A fact that has been known for many years is that microbes do not grow when the relative humidity of the air gets below 60%. In the FOOD section of my eBook A Wetter Look At Climate Change there is a table that shows the lowest %RH for one of the organisms is 61%. The two organisms at the bottom of the table are Xerophilic, which means, high tolerance and able to survive in dry conditions. This is where “Life on Mars” is relevant.

Atacama Desert https://en.wikipedia.org/wiki/File:Atacama.png

In South America there is an area that is the most “arid” place on Earth. An area defined as arid has little or no rain and is too dry or barren to support vegetation. The Atacama Desert, located in northern Chile, is accepted as being the driest and oldest part of our planet. Microbiologists have studied the bacteria and fungi from this region since the 1960’s. But in 2003, NASA published a paper describing Atacama as a model for Mars. That kicked off intense interest in engineering and scientific activity to mimic how to perform tests on the Martian terrain.

The big question “Is there life on Mars?”

Let’s start with “Is there water on Mars?” Pictures from the Mars missions compared to geographical features on Earth, indicate strongly that liquid water once flowed on the surface of Mars. Features that look just like riverbeds and erosion by water. We know for sure that water in the form of ice sits at the North and South poles of Mars. Also, there may be water deep underground. Future missions are planned to provide some answers.

Mars showing the ice capped poles https://en.wikipedia.org/wiki/Mars

Does water always mean life?

As far as we know, water is a prerequisite for life. On Earth no life exists that does not rely on water. Back to the arid Atacama Desert. Engineers and scientist have designed machines and testing techniques to detect the presence of microbes in this desolate part of our world. The technology will be placed on board Mars missions and the data from the tests will be beamed back to Earth.

All very exciting and high tech this stuff. In my reading of the published papers on the microbiology and molecular biology of the Atacama organisms, I went looking for evidence of microbial growth in an environment that is predominantly below 60%RH. I thought, if anybody can find such Xerophiles, these guys might.

I was encouraged when I found this statement in a review paper: “This work definitively validated the Atacama Desert as a Mars analogue and also as an unparalleled place to pursue studies on the dry limit for life.” In my mind, coloured by my quest for an explanation for the 60%RH microbial growth limit, I read this as a search for organisms that can scavenge in low moisture conditions. By low moisture conditions, I mean at a humidity below 60 %RH.

A problem with doing science outside of the laboratory is the things going on that are not under your control. Looking at the weather conditions for Atacama with less than 2mm annual rain and average %RH of 10, it is easy to classify this desert as the driest place on Earth. So, what can get in the way of looking for life in such a low moisture environment? Fog for one. Drifting in from the coast and around the coastal range of mountains into the desert this moisture can provide organisms with the necessary moisture to keep them alive. What the scientists observed is a fall off in the total number and different types of organisms as they went from the edges of the desert towards its middle.

Fog advancing over the coastal range on the Pacific Ocean side of the Atacama Desert
From: Life at the dry edge: Microorganisms of the Atacama Desert Armando Azua-Bustos, Catalina Urrejola, Rafael Vicuña

After my initial excitement of maybe getting an answer to the 60 %RH growth limit for microbes, I was becoming disillusioned. Seemed like the microbes were simply scavenging moisture when it was carried across parts of the desert by fog. Frustrated by not making progress on the 60 %RH growth limit question I contacted one of the authors of a review paper “Life at the dry edge: Microorganisms of the Atacama Desert”. His name is Armando Azua-Bustos, an Astrobiologist working in Spain. We had a Skype call in which, at last, I saw hope on the horizon.

Armando told me about controlled laboratory experiments where he studied the Xerophiles from the Atacama Desert. Under low %RH conditions mimicking the Atacama Desert he detected one of the key signs of a living organism. All living creatures must have an active metabolism to live and certain molecules are produced and used within living cells. Using sensitive probes for the molecules of life, activity was seen in the Xerophiles at 10% and 30% humidity. Well below the 60% limit.

My chat with Armando got even better. He told me about how cells can protect themselves against dehydration. Certain types of sugar molecules and proteins are produced by the Xerophiles. One of the key sugars is called Trehalose that can substitute for water molecules within the cell by interacting with other key molecules. I knew about Trehalose from my past where I used it to protect yeast from freezing when storing at -20°C. Another type of molecule mentioned by Armando is Dehydrins. These are small proteins that can also substitute for water molecules within the cell. Both Trehalose and Dehydrins are produced in cells that are under stress from dehydration. Armando described the inside of the cell becoming more like a gel rather than a watery soup.

Trehalose

The picture we now have of Xerophiles is that, when the environment gets drier, the protective molecules, Trehalose and Dehydrins, allow the cell to continue to metabolise with less water. However, further dehydration would stop metabolism completely, which means cell death. Armando suggested that Xerophiles have evolved biochemical pathways to counteract dehydration by producing within the cell a small amount of water for metabolism. This is what Armando and his colleagues are detecting using their probe for metabolic activity. In other words, the Xerophiles respond to drought by protecting themselves and then turn on a water production mechanism.

So, with my question answered about the 60% growth limit, what about the Big question, Life on Mars? Science is telling us that a key sign of life, metabolism, is looking feasible under the dry conditions present on Mars. Does that mean there could be the possibility of organisms growing in that environment? We don’t know yet.

Earth and Mars were created around the same time, about 4.6 billion years ago. Mars started to lose its atmosphere and ability to support liquid water about 4 billion years ago. But it took a further 0.5 billion years (3.5 billion years ago) for life to evolve on Earth. This raises the question of would there have been a sufficient time for life to have evolved on Mars before it became too dry? If life had evolved, is it possible that Martian Xerophiles would be able to sustain low level metabolic activity over the billions of years since it became dry? Armando and his fellow Astrobiologists will one day let us know.

NASA have discovered large underground lakes of water on Mars. One of these is frozen and is the size of Lake Superior, another is liquid. Also, it is possible that underground water could be warmed by the sun and trapped in caves where it could support life. This all adds to the thrill of there being Martians out there, albeit most likely micro-ones!

Welcome to my world of moisture

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