You Must First Invent the Universe…

By Rich Feldenberg

This year Carl Sagan Day is being celebrated Saturday, November 14th. Sagan, who was born on November 9th, 1934 has been an inspiration to generations of scientists and science enthusiasts. Unfortunately, he passed away on December 20th, 1996 at the age of 62. Way too young, and certainly way too soon for a world that desperately needed his carefully measured dose of rationality, skepticism, and his poetic style of revealing the awe of the cosmos we inhabit together.

There are many great and inspiring Sagan quotes, or Saganisms as they’ve come to be known, but one of my favorites is, “If you want to make and apple pie from scratch, you must first invent the universe”. The meaning, of course, gets one to think deeper about where the origin for all the things we take for granted actually came from. The ingredients for an apple pie may include things like apples, flour, sugar, eggs, salt, etc. But where to these ingredients come from? To get these ingredients you must first invent a universe with laws like our own, that can lead to the formation of galaxies full of stars, which can fuse hydrogen atoms into heavier elements, which can then form planets. Some of these planets must have conditions that allow life to arise, which can evolve into things like apple trees and chickens (for the apples and eggs respectively) and for the evolution of intelligent beings that can put them together to make an apple pie. Some of the ingredients, like the salt (NaCl) and water (H2O), are relatively easy to produce, and just require the hundreds of millions of years necessary for stars to produce the heavy elements oxygen, sodium, and chloride (the hydrogen for the water was produced in the Big Bang itself). The other ingredients require billions of years in the making, for life forms and their evolution to take place. How brilliant and wonderful and simple a statement to make. Many people around the globe, that continue to honor and remember Carl make it a tradition to eat a slice of apple pie on Carl Sagan day. I know I plan to have a piece this year!

Sagan was an Astronomer, and one of the first astrobiologists. He was involved in important scientific research on the atmospheric composition of Venus and Mars. He played a major role in the Viking mission to Mars and the Voyager probes to the outer solar system. And, of course, he made communicating scientific findings to the public, and demonstrating the importance of the scientific process, a priority.

When I was growing up, the book Cosmos and the mini-series, by the same name, came out. Both were inspiring, thought provoking, and in some ways life altering, and Sagan tackled everything from Astronomy, evolution, the brain, and the importance of being skeptical of pseudoscientific claims. He had a mesmerizing way of delivering his message with intelligence and passion. The TV series was recently redone by Astrophysicist and science communicator, Neil Degrasse Tyson, who didn’t attempt to remake the original episodes, but who did an excellent job of continuing on where Sagan left off.

Sagan also wrote quite a few other excellent books. These included, “The Dragons of Eden”, “Broca’s Brain”, “The Demon Haunted World”, and “Billions and Billions”. These books really fueled my scientific curiosity growing up, as I’m sure they have done for many others who grew up to love science. After all these years, his books are still worth reading, if you haven’t done so already. He also wrote the science fiction novel, “Contact” that was made into a motion picture in 1997 with actress Jodie Foster. In the novel he attempted to show what first contact with an advanced alien species might be like.

I did have the opportunity to see Carl Sagan in person on one occasion. At the time I was a chemistry major in the mid-1980s at The University of Missouri – St. Louis. Sagan came to deliver a lecture to our university on the dangers of nuclear war and the importance of nuclear disarmament. He was a great dynamic speaker and the lecture hall was completely full. I think, at the time I was hoping he was going to talk about astronomy, but in retrospect I now understand the importance of his social concerns for our future and continued existence.

Sagan also introduced me to the concept of scientific skepticism, at a relatively early age. He was critical of how to tell the difference between science and pseudoscience (something now called the demarcation problem). He showed us that there are no beliefs that should be immune to skeptical inquiry, including religious belief. He came up with the “Baloney Detection Kit” that everyone should have in their skeptical toolbox.

Carl passed away right when the first exoplanets were just being discovered. Now we know of more than 1000 planets that circle other stars. We have made a much more thorough exploration of Mars and the moons of the outer solar system. We have strong evidence for liquid water deep under the crust of the moons Europa, Enceladus, and Ganymede. There is liquid methane on Saturn’s moon Titan. These discoveries make the possibility for life in our outer solar system a little more likely, and for life outside of our solar system very likely, by the sheer number of planets in our galaxy alone. At the same time the skeptical movement has gained momentum and is going strong. We have learned more about cognitive psychology and our innate biases and predisposition towards distortions of memory and perception. Flaws we must recognize in ourselves if we are to take the first steps to learn to become a more rational species and rise out of our superstitious past. I believe Carl would find all this fascinating and exciting. We could really use Carl’s wisdom now, but at the very least we still have him with us in the form of his writing and video.     

Happy Carl Sagan Day. Have some Apple Pie and be sure to learn something new today!
References and other items of interest:
1. Carl Sagan Wikipedia article: https://en.wikipedia.org/wiki/Carl_Sagan
2. Article detailing the “Baloney Detection Kit”: https://www.brainpickings.org/2014/01/03/baloney-detection-kit-carl-sagan/
3. Trailer for the movie “Contact” based on the book by Carl Sagan: https://www.youtube.com/watch?v=jl7Xe80_0MY
4. The Demarkation Problem on the Rationally Speaking Blog.
http://rationallyspeaking.blogspot.com/2013/08/philosophy-of-pseudoscience.html
Also check out the excellent “Rationally Speaking” podcast. The current host is Julie Galef, and excellent skeptic and teacher of all things rational! The previous host was Massimo Piglucci and scientist and philosopher and all around brilliant guy. Well worth checking out!
5. The Rationally Speaking Podcast with Julia Galef: http://rationallyspeakingpodcast.org
6. Some great Julia Galef youtube videos on rationality: https://www.youtube.com/user/measureofdoubt
7. Massimo Piglucci’s homepage: https://platofootnote.wordpress.com/massimo-central/
8. My contemplations on the possibility of what it would take for life to evolve on Titan:
http://darwinskidneys-science.com/2015/08/05/musings-on-the-biochemistry-on-saturns-moon-titan-part-i/

Part II: Musings on the Biochemistry of Saturn’s Moon Titan

Part II: How can we envision solutions to the challenges for life on Titan?

By Rich Feldenberg
Titan_and_rings

Definitions:
Non-Polar Liquid Solution – NPLS
Polar Non-Aqueous Liquid Solution – PNAL
Titanoids – terpenoid-like molecules used by life on Titan. They provide the subunits (monomers) necessary to make large molecules (polymers), the way amino acids make proteins on earth.
Protiteins – These molecules are build up from the smaller titanoid subunits, and serve the role of proteins for Titan life forms.
Genoids – steroid-like molecules that have been naturally selected by life on Titan to store the genetic information, similar to nucleotides on earth. They can “base pair”, based on complementary physical fit with another specific form of genoid.
Titanite – life forms found on Titan.
Reverse lipid bilayer – a molecular membrane on Titan in the PNAL scheme that has its hydrophobic tail facing the methane solution outside the cell, and its polar head facing the cell interior to remain in contact with the polar solvent concentrated in the cell.

In Part I of this article we discussed the special properties of water that makes it so important for life on earth, and the properties of liquid methane on Titan that make it a poor substitute for life as we know it. So while in Part I we focused on what the problems are for Titan biochemistry to exist, Part II will look at some theoretical solutions to those problems. For methane to be the fluid of life, would require life to take on an entirely different character from what we know. Methane’s non-polar physical character presents major hurdles that may prevent interesting biochemistry from taking place in a such a non-polar liquid solvent (NPLS). While liquid methane is abundant on the surface of Titan, and undergoes a methane cycle, similar to the water cycle on Earth, a non-polar solvent for life would seem problematic at best, and impossible at worst. For that reason we will also consider some other options for life on Titan. We’ll look at the possibility of a Polar Non-Aqueous Liquid Solution (PNAL), that might provide a way for Titanites to survive and evolve by creating an internal environment friendly to polar chemical reactions, like those seen in Earthly life forms. As I said in part I of the article, “We will stick, as much as possible, to the rules of organic chemistry, but Warning, wild speculation ahead”. Ready to jump into a lake of liquid methane? Here we go!

The Non-Polar Liquid Solution (NPLS):
Lets start with the Non-Polar liquid solution (NPLS) possibilities. If we accept methane as our solvent because it is the liquid that happens to be flowing on Titan’s surface, then we’re faced with a difficult dilemma. Methane is a non-polar compound. It’s dipole moment is zero, zip, nadda, in other words, it has no permanent charge separation within the molecule itself – unlike water which has a relatively large dipole moment of 1.85 D. So just like the adage, water and oil don’t mix, on Titan we’re dealing with oil so the things that will dissolve in methane are also going to be non-polar substances or hydrophobic. The kinds of biomolecules that make life possible on earth would not do well in that “hateful” environment. In fact, the very thing that makes life interesting on Earth is that the molecules of life are very reactive, have groups of atoms in the molecules themselves, that are polar and therefore reactive with other polar molecules. This provides the basis of most of the biochemistry of Earth life. So on Titan, in the NPLS scenario we would not expect to find things like Earth-like DNA or proteins. So how could it work?

alkane

We would need non-polar molecules so that they could remain in a methane solution. Due to the extreme cold on Titan, any polar molecules would have too stable of an interaction with each other and precipitate out of solution as a solid. In other words, DNA, and other similar molecules would crystalize out. Not really a very good way for life to get started. On Earth we do have lots of non-polar biomolecules in the form of waxes, oils, and fats. The biochemistry on Titan, in the NPLS would have to be made of something like that. Life also seems to need small building block materials (monomers) that can be polymerized together to make large biomolecules. We need to find non-polar compounds that can, in principle function that way. Two possibilities could be substances similar to terpenoids or steroids.

Let’s look at terpenoids first. Terpenoids are a class of lipids that are made out of multiples of 5 carbon units. Their precursor molecule is isopentenyl diphosphate – a 5 carbon compound attached to a diphosphate group. By using this as the basic building block, you can build up a larger sized molecule with the isopentenyl as the basic unit. Since Titan’s oceans are methane with some ethane, we might imagine our basic building block to be a 2 carbon unit – made from the ethane. That way our biomolecules would be large with an even number of carbons because they are built up from multiples of two. Instead of terpenoids, we’ll call these molecules titanoids, and they could perhaps function in the role of amino acids, being used to build larger biomolecules, the equivalent of proteins – we’ll call these protiteins (pronounced Pro-Tie-Teens). There could be different titanoids used – like the 20 different amino acids on Earth – each with a different non-polar side chain.

Next lets look at the steroids. These are a diverse class of molecules which all have a basic 4 part ring structure. All steroids are themselves derived from a terpenoid compound called lanosterol. The rings, which are labeled A, B, C, and D, can themselves be altered in many ways to give the wide variety of steroids found in plants and animals. Having a hydrocarbon ring system, like in the steroids found on Earth, produces an essentially non-polar and hydrophobic compound. Like terpenoids, they could mix easily in the liquid methane environment found in the cells of Titan organisms. The rings themselves can be boat-shaped if saturated, but flat if aromatic (meaning they have double bonds like benzene that provide an aromatic resonance).

We might imagine the non-polar and very cold environment on Titan to favor a kind of stacking of these rings. They might be produced to fit neatly on top of one in other, so that instead of have a linear molecule composed of many monomers, like Earth protein or DNA, on Titan we might have layers or thick sheets of molecules that are stacked on top of each other, held in place by their Van der Waals forces, to provide the structure. The weak Van der Waals forces would keep the molecules, essentially glued together. This would provide a very different and alien kind of molecular structure than earth organisms which put molecules together with covalent bonding.

We also need some type of information storage molecule to allow a Darwinian type of evolution to take place. We might also imagine steroid-like molecules serving the function of information storage that DNA and RNA can serve on earth. There would not be hydrogen bonding between nucleotide bases possible in the cells hydrophobic methane protoplasm. Instead several different steroid types (lets call these genoids to indicate they form the genetic material based on a steroid structure) might have been chosen in which one molecule seems to make a very good physical fit with one of the other chosen genoid molecules – essentially a lock and key type of interaction based on complementary shape. No hydrogen bonding would be necessary, just the close fitting together of genoid 1 with genoid 2, and genoid 3 with genoid 4. That way there is a template for copying the genetic material, and way to store information in the genoid 1, 2, 3, and 4 code. The back side of the genoids might contain functional groups, such a methyl groups, that would create a steric hindrance so that they can only fit together in the desired base-pairing way.

There could be only 2 genoids, although that would not allow for much coding information, or there could be more than 4. So for example, a “codon” with the genoid sequence 111, might code for titanoid A, and the codon with genoid sequence 112, might code for titanoid B, and so on. The genoids might stack on top of one another but fit together with their complementary sheet, which forms the template for replication. Because dispersion forces, which are terribly weak, are holding the works together, this would only be possible at the extremely low temperatures, like those found on Titan. If the temperature was raised the molecules would fall apart and the organism would essentially melt away. Even the temperature of dry ice (solid carbon dioxide) with a temperature of -109F, would be hot as hell for our friendly little Titanites.

genoid A&B

genoid base pair

Somehow we would have to have a mechanism that allowed the genoid code to be translated into the titanoids to make some sort of polymer structure. Since hydrophobic chemistry is rather boring – I mean only in the sense of being unvaried, not that it is stuffy in any way – because there is no nucleophilic substitutions or eliminations, or so forth, molecular reactions other than simple dipole-dipole and dispersion interactions, would probably have to take place through radical reactions, using some energy source to produce the free radicals.

methane

Polar-Non Aqueous Solution (PNAL):
The PNAL scenario would work by allowing the cells on Titan to essentially evolve to become containers of weakly polar solvent, which keep the polar solvent inside the cell membrane, and the non-polar methane on the outside. There would have to be a way to pump in the polar solvent from the environment and concentrate it in the cell, preventing it from leaking back out. The advantage here is that we then can allow the much more interesting types of chemistry to occur in the cell, with reactions like the nucleophilic substitutions, additions, and eliminations, which can be used to build interesting molecules and metabolize others. This type of life might seem slightly more familiar than the NPLS, that we considered above, but would still be a very alien “life as we don’t know it” variety. We might have to imagine the cell membrane to be a kind of reverse lipid layer, instead of the lipid bilayer found in Earthly cell membranes. The lipid bilayer of Earthly cells has the lipid tails in contact with each other, sandwiched in, while the hydrophilic phosphate heads are facing outward on each side, making contact with the aqueous environment of the interior cell on one side and the water external to the cell on the other side. The reverse lipid layer would have the hydrophobic tail sticking on the outside to interact with the methane environment, but the polar head region (like a phosphate group) on the inside to interact with the polar solvent concentrated in the cell.

The solvent here would still need to be an almost non-polar substance with a very low dipole moment. Any truly polar substance – one having a high dipole moment – would have too much molecular interactions with other molecules of its kind, and would solidify at the temperatures found on Titan’s lakes and rivers. Water has a dipole moment of 1.85D, which is way too high for this environment. In fact, water on Titan’s surface forms rock hard geological structures. One substance that might work would be Arsine (AsH3) which has a dipole moment of 0.20. Arsine, with one Arsenic atom and three hydrogen atoms, might conceivably be a substance that could be found or produced on Titan since Arsenic (As) and Hydrogen (H) are both common elements. The freezing point of Arsine is -168.16F, which is pretty cold but Titan is -291.1F, so this would only work if there were some warmer spots on Titan where there is geothermal energy reaching the surface. If true though, Titanites would drink arsenic the way we drink water! The reverse would be equally true, water would be a deadly poison to their delicate machinery of life.

Arsine-underside-3D-vdW

Arsine

Perhaps a better choice of polar solvent would be Perchloryl fluoride, with a dipole moment of only 0.023D and a freezing point of -234F. This is still a little short of the -291.1F of Titans Lakes, but fairly close so perhaps there could be some “hot spots” where the temperature is a balmy -234F, and the perchloryl fluoride would flow free! Perchloryl fluoride is a molecule made of one chloride, one fluoride, and three oxygen atoms, so it may be something that life on Titan could find or produce and concentrate in their cells. The low dipole moment might still mean that other polar molecules would not react well with it, and there would be the risk of other polar biomolecules freezing out of solution. Getting caught in a slightly cooler zone for PNALs would spell disaster for these little Titan cells, as they would crystalize, whereas the NPLS would seem well suited for the extreme cold of a world far from it’s star.

Since the temperatures are so cold we might also need to consider molecules that are extremely reactive – even too reactive for Earth life. We might consider acid halides in place of the usual functional groups like carboxylic acids, alcohols, esters, and so on. On earth acid halides are too reactive – the halide (such as chloride) would be too good of a leaving group – and they would therefore have no stability. On Titan, however, where the temperatures are so cold the acid halides, like acid chloride for example, might be longer lived so that they might have more stability and could be controlled by cellular process to take part in chemical reactions at the appropriate times.

acyl_chloride

Whether any of this could really play out on Titan or a similar world, I don’t know. This is the fun of pure arm-chair astrobiology. Perhaps some of these ideas could be tested to some degree in the lab. Our only real way of knowing if Titan could support some form of life is to send robotic probes that can go there and conduct the right experiments. I sure hope that a mission like that will happen sometime in our lifetimes. Certainly finding life as we don’t know it would increase our understanding about what life is, and would ultimately mean that life must be very common in the universe if it can manage to find ways to exist on worlds as different as Earth and Titan.

References:

1. Titan: Wikipedia; https://en.m.wikipedia.org/wiki/Titan_(moon)

2. Freezing and Melting Points of some common liquids:
http://www.engineeringtoolbox.com/freezing-points-liquids-d_1261.html

3. “Selected values for electric dipole moments for molecules in the gas phase”, United States Department of Commerce; http://www.nist.gov/data/nsrds/NSRDS-NBS-10.pdf

4. Organic Chemistry; John E. McMurry, 8th edition. ISBN-13: 978-0840054449
5. See my article on Silicon Based Life forms (another variety of life as we don’t know it):
In this case it would presumably be water dependent but not based on carbon.
“Why the Horta would not have looked like a rock monster”;
http://darwinskidneys-science.com/2015/06/18/why-the-horta-would-not-have-looked-like-a-rock-monster/

6. See Part I of this article. “Musings on the Biochemistry of Saturn’s moon Titan, Part I”.
http://darwinskidneys-science.com/2015/08/05/musings-on-the-biochemistry-on-saturns-moon-titan-part-i/

7. McLendon, Christopher, et al. “Solubility of Polyethers in Hydrocarbons at Low Temperatures. A model for Potential Genetic Backbones on Warm Titans”. Astrobiology, Volume 15, Number 3, 2015.