Draft of my presentation for the think tank this summer on the value to science and implications of exploration of Enceladus and Europa for signs of life.
This talk is about the science value and implications of searching for life in the oceans of Europa and Enceladus.
Enceladus particularly is such an interesting place for exobiology, especially with the new results published in March of this year.
As well as that it gives us a wonderful opportunity to search for life with the minimal of planetary protection issues, which is an issue close to my heart.
So why is Enceladus so interesting?
Here is a photograph of two of its geysers. It is not an artist's impression:

Cassini first discovered them in 2005. Since then it's taken many photographs and flown through them several times. This is what we know about them
[youtube https://www.youtube.com/watch?v=Vd1oLAetEPI]
3D model of the geyser basin of Enceladus showing location and tilt of 98 of the 101 geysers identified in 2014. Dotted lines show five jets with images taken too close together to determine the tilt precisely.
- 101 geysers counted in 2014
- Typical vent is a hot spot of about 10 square meters.
- Geysers occur along fracture lines
- They contain ice crystals, methane, ammonia, and silica
- The silica tells us an astonishing amount about the conditions
From the silica we can deduce (Gabriel Tobie, March 2015 Nature):
- Enceladus subsurface sea has at most 4% salt - so not too salty for life
- It's pH is between 8.5 and 10 so moderately alkaline.
- Originates at an interface between rock and water at temperatures of 90 C
- pH on formation is greater than 8.5
- The silica particles probably get to the surface within a few months of formation at the vents, or at most years.
These conditions are almost identical to those in the "Lost City" hydrothermal vent in the mid Atlantic..
Exposed mantle rock (layer below the Earth's crust). This suggests that we may learn about abiogensis as this habitat may have been common in Early Earth.
Serpentization: olivine + H2O + CO2 → serpentine + magnetite + brucite + CH4 + H2 + hydrocarbons
Sulfate in seawater reduced by hydrogen to produce hydrogen sulfide
Microbes may be using anaerobic methane oxidation so methane consumers (methanotropes)
Simultaneously there may methane producers (methanogens)
Temperatures of the interoir: 20-90°C and pH 9-11 (the water is emitted at 300°C but rapidly cools down).
Interior dominated by biofilms of - Lost City Methanosarcinales (LCMS)
Microbial community to a large extent independent of surface conditions
So it is an ecosystem, one of several now known, that's for the most part not dependent on sunlight in any way. This community could most likely survive on Enceladus.
It's also been suggested as a possible place for abiogenesis, where life may have originated in the early Earth.
Mystery of the heat sources of Enceladus
Originally then there was a mystery about how Enceladus obtained enough heat for the geysers. Back in 2012, then the heat source was still unknown, with some suggestions of ways the heat budget could add up.
It seems that research is gradually converging towards a solution that may lead eventually to a model for a permanent Enceladus ocean.
I'm mainly summarizing the discussion section of the 2014 paper, TIDALLY MODULATED ERUPTIONS ON ENCELADUS: CASSINI ISS OBSERVATIONS AND MODELS with some more background information.
See also Hugh Platt's blog post on these results.
Heat map taken by Cassini in 2008 and later in 2009
Zooming in on Heat at Baghdad Sulcus
Temperatures measured at up to 180 Kelvin at the hottest parts, confined to an area of a few square meters. No internal heat in violet coloured areas. Most of the heat from the warm flanks of the fractures, and the interior of the fractures may be warmer than that, possibly warm enough for liquid water just below the surface.
Plumes wax and wane with the tides. But with a 5.7 hour delay which is a challenge for the models. It may be due to a lag in response of the ice to the tidal effects amongst other suggestions.
This is the latest model of the surface processes. Vapour and salty liquid droplets rise and condense near the surface. Latent heat of condensation helps heat up the geysers. This also suggests there may be liquid water near the surface.
At first it was a major challenge to explain the heat sources. However recent models are able to obtain this amount of heat by making various assumptions.
One way is through eccentricity tides with a time delay.
Another way, favoured by the 2014 paper, is due to longtitudinal libration of the crust over a global ocean.
Shows libration of our Moon, both latitudinally and longtitudinally.Small longtitudinal librations of 0.8 degrees (beyond the resolution of studies so far) of its ice crust over a subsurface global ocean may be a source of heat for Enceladus, but this is a prediction of a theoretical model not yet confirmed.
Is the ocean temporary or long term?
Some time back the consensus was that it was likely to be a temporary ocean, because the heat budget. But with these newer models, then they seem to favour idea of a long term ocean.
This next graph may not seem that interesting, just some dots on a straight line, but it is potentially quite huge in its implications.
This is from a paper which charted the growth in complexity in DNA. The author's insight was to measure only the "non redundant" DNA. So leaving out junk DNA and also duplicates such as extra redundant chromosones. They got a nice straight line and you'd expect it to hit the origin at 4.5 billion years.
But instead, this is what they found:

So, there are two ways to take this. One is to use the now respectable theory of Panspermia.
Perhaps life on Earth originated around another star. If asked to guess, you might suggest, perhaps the much more common orange dwarfs. It's a puzzle that life started on such a rare and short lived star as a yellow dwarf when it could have started on the much more numerous and equally habitable and longer lived and more stable orange dwarf stars.
So, what if it did start on a planet around an orange dwarf (or any other precursor star). Which passed through a collapsing gas cloud when the solar system was forming.
Or maybe later on, it passed through the forming solar system in a stellar nursery, when there was still a lot of material to bombard our orange dwarf's planets and transfer material to the young Earth?
TW Hydra disk - a protoplanetary nebula imaged with evidence of a gap where a giant planet may be forming. Perhaps life could be transferred to the early solar system by another star system passing close to one of these protoplanetary nebulae in a stellar nursery.
One way or another, it may be possible that ancient life in our solar system could have a common origin with Earth life from a previous star like this.
The other way to take it though, is that it could just be that the evolution proceeds far more slowly once DNA is involved and all the error correction machinery etc of the modern cell.
Perhaps all that billions of years of evolution can happen in just a billion years or so, with the precursors to modern life, or due to special conditions that prevailed then.

Either way, the diagram helps us to see the huge gap in our understanding of biology.
Presumably the missing first half of this diagram has as many stages as the second half. Events as momentous as the development of cells with a nucleus (Eukaryotes), and creatures with a backbone, and of fish, of mammals and of ourselves. But we have no idea what they were.
Our experiments in laboratories only just edge in a bit from the left of this diagram. In between you have the vast area of "Don't know". Many theories, no data.
Another thing that suggests the same conclusion is the immense complexity of the modern cell, with its million chemicals all coming together in a complex dance. There is no way that could just form from chemicals without many intermediate steps.
RNA polymerase used to decode DNA to mRNA, present in all living cells.
Ribosome translating mRNA into a protein
Every cell of our body, and every cell of every living creature is using exactly the same process, and same DNA, same bases, same amino acids.
It's all rather "Heath Robinson" or "Rube Goldberg".
It works, and presumably is a good solution to the problems, but it is surprisingly complex, with details piled on details, parts of the "machinery" error correcting other parts, until you get something that works.
Also DNA is unstable at high temperatures, and doesn't form easily either. Most researchers think that early life went through a stage when it used RNA only. Or possibly, some other helix structure such as PNA which has a different backbone from DNA (or a whole alphabet soup" of other possible precursors such as TNA).
PNA

So what were the earliest cells like? What are the simplest possible cells?
Many experiments and researches but no hard data to ground any of it.ells
Some researchers are working with Butschli droplets, a complex mixture of oils and other chemicals that behave rather like cells. Not suggesting that they are precursors of evolution, but just simple examples that work like protocells
Or more complex "behaviour"
[youtube https://www.youtube.com/watch?v=abb9R_JvZ5k]
That includes Rachel Armstrong and Martin Hanczyc:
Or there is the idea of an RNA world.
So general basic approaches of metabolism first or replication first. The protocells can "reproduce" in a way but imperfectly, just grow and then split.
So what could we find on Enceladus?
Well if the ocean is just a few tens of millions of years old, as originally suggested, or if life has not yet evolved there, it could be right at the start of the graph, in the area of protocells or the simplest forms of life, maybe just a few tens of nanometers accross. Or it could be an RNA or PNA world in there. No metabolism but replicating chemicals. Or a primitive form of life.
So, then it is right towards the left of our diagram, helping fill in the huge gap in our understanding of abiogenesis.

But then - it could be way to the right. It might be a billions of years old ecosystem that has evolved through as many stages as our own. Or even beyond the graph to the right.
There is nothing, actually, to rule out creatures in the ocean of Europa or Enceladus as intelligent as octopuses, dolphins, or even ourselves. A civilization in these oceans would be unable to use fire. Under conditions of high pressure, sealed from the surface by ice, they would probably be unaware of us and us of them, so far, anyway
That is not a serious suggestion, but it's possible. Just to highlight our lack of knowledge here. These oceans could be anywhere from the far left all the way to the far right. Or even beyond the far right, evolved to some future possibility Earth life hasn't encountered yet.
But as well as that, it doesn't need to be on a linear progression with Earth life. Since DNA is so very particular, and "Rube Goldberg" or "Heath Robinson" in the way it works.
Imagine that you have been brought up in the African savannah - with its grasses and trees and elephants and antelopes. You've never seen a marsh or a forest, or a beach. All your life you've lived in a hut in the African Savannah, never traveled more than a few miles from your hut, and that's the only thing you've ever known.
Then one day someone takes you to the sea shore, with its fish, shellfish, seaweeds, and sea anemones, and perhaps they take you on a dive to see a coral reef.
A Blue Starfish (Linckia laevigata) resting on hard Acropora coral. Lighthouse, Ribbon Reefs, Great Barrier Reef. Photo by Richard Ling
XNA based life could be as different from DNA based life as the African Savannah is different from a coral reef. And imagine the new perspectives we might get if we can study it.
So - I see both of those possibilities as immensely interesting for exobiology. But they have major planetary protection issues. The life, if so very different from Earth life - could it be hazardous for us, or vice versa? How can we explore Enceladus without risking destroying the very thing we want to find out about?
So that's where the Enceladus geysers come in. But to frame this discussion, first we need the precautionary principle
Precautionary principle
When an activity raises threats of harm to human health or the environment, precautionary measures should be taken even if some cause and effect relationships are not fully established scientifically.
In this context the proponent of an activity, rather than the public, should bear the burden of proof.
The process of applying the Precautionary Principle must be open, informed and democratic and must include potentially affected parties. It must also involve an examination of the full range of alternatives, including no action
This clearly applies to a sample return. And the affected parties there are everyone on the Earth because it could, potentially, impact on the habitability of the Earth.
The main point there is it has to involve examination of the full range of alternatives including no action.
Suggestion for a precautionary principle approach for forward contamination.
What would we think, if in the future, that we knew that a few decades, or centuries, or a few thousand years earlier, in their very first exploration of the solar system, that humans introduced Earth life to an Enceladus ocean of protocells or XNA life? And so completely ruined it for study of these processes for later generations?
For those reasons I suggest we take an equally precautionary approach for forward contamination.
For every site we study in the solar system, until we know more, it may be the most precious thing in our solar system, outside Earth. It might require interstellar flight to find another analogue, and even that might not be sufficient, for all we know.
So, discussions of precautions needed for planetary protection should in both directions, in my view, always consider "the full range of alternatives including no action."
This would probably work like researchers not drilling into Blood Falls until they are ready - a case of "no action for now, because we need to know more, or need improved technology".
Decision tree
So I see a progression here. Each step requires either a higher level of understanding, and confidence, or more elaborate precautions.
If your understanding is good, and you have high confidence levels in your results, you may not need much by way of precautions, and what precautions you take will be addressed to a known situation and will be proportional and effective.
If your understanding is not so good, or your confidence levels for your results are low, you need many precautions and even elaborate precautions may not always be enough.
For Enceladus and Europa I see the stages here as
- Clipper mission, collects at 7 km /sec
- Orbiter, down to 100 meters / sec (why I'm so enthusiastic about the proposal).
- Sample return, sterilized before return
- Surface mission, drilling into the ice
- Sample return unsterilized.
Europa Clipper
Planetary protection issues seem very low. Main one, to make sure it can't impact into the target body.
Enceladus Orbiter
Launches Jan 28 2023. (21 day launch window). Flies past Venus twice and Earth twice, reaches Saturn July 29th 2031. Enters Saturn with a six month orbit. Biggest delta v is the insertion into Saturn orbit.
Then it uses a sequence of flybys of the inner moons of Saturn to work its way in to Enceladus. First flies past Titan, Then Rhea, then Dione, then Tethys and finally Enceladus.
Several close encounters with each one. So a very interesting science mission on its own.
- "The Titan tour would include three flybys of Titan and would end with an encounter with Rhea.
- The Rhea tour would include 15 flybys of Rhea and would end with an encounter with Dione
- The Dione tour would include 10 flybys of Dione and would end with an encounter with Tethys.
- The Tethys tour would include 12 flybys of Tethys and would end with an encounter with Enceladus
- The Enceladus tour would include 12 engineering flybys and 10 science flybys of Enceladus and would end with Enceladus orbit insertion
Zero chance of back contamination of Earth and very small chance of contamination of Enceladus to work through.
In orbit around Enceladus with 100 meters / second impact of ice particles not just onto the aerogel, but onto the spacecraft itself. Could that dislodge microbes that still attached to the outside of the spacecraft - given that the plume itself falls back to Enceladus? What is the chance they could be viable and hit the planetary surface?
Lander on Enceladus
Here I differ from COSPAR and the "orthodox view" on this matter.
So, COSPAR's recommendation is of a 1 in 10,000 chance of contaminating the ocean of Enceladus for each mission.
And that's figured using a calculation from the initial bioload,
I argue we may need to be concerned even about dead DNA if it makes contact with an Enceladus ocean of protocells or very early life. And for living organisms, I'm not at all sure myself that the 1 in 10,000 is sufficient.
That's an ethical decision. You can't make that decision using the scientific method.
In case of Mars decision has already made, we have to accept a chance that we have already contaminated Mars, and hope that it is around the 1 in 1,000 level which was Carl Sagan's original aim when he chose his 1 in 10,000 per mission.
That's where the figure comes from, Carl Sagan having the aim that after 30 or 40 missions the chance should be less than 1 in 1,000 of contaminating Mars.
And it's just become a benchmark figure that is used in this topic area - with no scientific justification. Can't have because it is an ethical question.
For Enceladus we have not yet done any actions that could contaminate it. And I would argue myself that 1 in 10,000 is not enough. We shouldn't risk contaminating Enceladus for all future generations unless at a lower probability than that. Others will have other views. So that's an ethical judgement. Shouldn't be presented as anything else in my view.
What can we do.
So I think that there are two things we can do to greatly reduce the chance, maybe to the extent it is acceptable to everyone, even the likes of me.
So first idea is to completely sterilize the exterior of the ice mole so that it is 100% free of organics in any form. If we put it in an enclosure, then seems only the drill at the front and the nose of the icemole needs to protrude beyond it.
So is that possible?
Deep cleaning with super critical CO2 and CO2 snow
I don't know if this is an answer but gives an example for the sort of thing I'd be looking for here. Ref 1, ref 2
- CO2 a liquid at 100 atmospheres and 50 C.
- And then on release of pressure turns to snow and takes the dirt, organics, everything away leaving the surface dry.
- Mixed with Hydrogen peroxide and other chemical to increase effectiveness.
- Can be used even with sensitive electronics. Was used to clean usb drives in testing and they functioned afterwards.
- Surface is left with no trace of organics, not just with dead micro-organisms. Major plus!
End of mission IceMole sterilization with ionizing radiation
So this is the idea, after the mission is over, exterior sterilized, but the interior and electronics, especially the computer, protected by a protective layer.
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In case of Enceladus, with our mole next to a geyser, a new geyser might erupt or the vent shift or widen, and our mole ends up in the ocean. And it could plunge tens of kilometers and rupture.
So I suggest just as a concept for discussion, that we could have a mission end sterilization cobalt60 ionizing radiation source or similar. Shielded from the mole - and the orbiter of course. But the shielding need not be that heavy because it just needs to prevent radiation in the direction of the mole itself, not in all directions. Just a plate in between of sufficient thickness, maybe on a boom if necessary to reduce the cross section and give some extra attenuation. Then at end of mission, to remove the shielding, and the mole then remains there, but irradiated by several thousand Grays a week or whatever is feasible. The most radioresistant life can withstand around 50,000 Grays. So to be safe, ensure that that amount of radiation is received in a short enough time so that there is no risk that it lands in the ocean with viable life. But it might need to be more than that if you also have to make sure that it doesn't include even dead fragments of life. Eventually ionizing radiation would break most of the bonds of any complex molecule until all you have left are gases. So just leave it to sterilize itself for all future time. Sample return with sterilized sampleThen that's the same, after you receive the sample, use an ionizing radiation source, to sterilize it. So we will get material back that is split up into many pieces by the radiation. But still, we can detect biosignatures even after a lot of radiation damage. And as well, we have in situ measurement to inform our analysis. Potentially, if totally sure it is adequately sterilized, can return to the Earth. Sample return with unsterilized sampleYou'd think this was easy, but it turns out to be surprisingly complex and difficult. I'm going to suggest it is best to find a way to just bypass all these issues. But first let's see what the issues are. Back in the 1990s then the general idea was that we can just return samples to a glove box facility in a biohazard 4 laboratory. But as studies were undertaken, the precautions needed got more and more complex. Ending with ideas that need hundreds of millions of dollars facilities with capabilities never tested before. The problem is that it is easy to contain a known pathogen, say smallpox, or anthrax, or the Ebola virus etc. And that's the general situation for a biohazard laboratory. But what can you do when you don't know what is in the sample, what its capabilities are, what size it is, or even what biochemistry it has? Quite possibly doesn't use DNA? XNA based life in the sample return may be sub optical resolution as well. Smallest size for cells not containing all the machinery of modern DNA generally estimated as about 40 nm. (But depends on advances of science, like all of this, and see the 3 nm theoretical example above). So successive studies by the National Research Council (NRC), USA (two studies) then the European Science Foundation (ESF) (one study) gradually lead to more and more stringent requirements. First, reduction to 200 nm by the NRC after discovery of the ultramicrobacteria Then reduced to 10 nm by the ESF. as a result of discovery of the profligate way that archaea can share their DNA through the tiny Gene Transfer Agents (GTAs)
So if the life is at all related to Earth life, you have the possibility of this exchange of DNA bringing new capabilities to Earth microbes from space. Even if the microbes themselves don't survive. Recommendations of the ESF:
This is one of the designs they came up with in 2008, the one with the telerobotics.
This is for just a less than 1 kg of samples returned most likely, yet you have to build something like this, Also their conclusions have to be reviewed continually, based on new research, as they conclude at the end. For instance there is much active research at present into into a semi synthetic minimal living cell or an artificial minimal cell. Does the 40 nm size limit still apply based on the recent research? And it doesn't address at all issues of human error, accidents, terrorism, a plane crashing into the facility etc (as they also say in the study). So that needs to be considered as well. Meteorite extinctionsYou might think that we don't need to worry, because so much material arrives on Earth from outer space through meteorites. However
And how do we know that meteorites don't cause extinctions over timescale of many millions, even hundreds of millions of years? The NRC looked into it in assessment of a Mars sample return, and they concluded:
What do we need to concern ourselves with?Most science fiction scenarios are implausible and wouldn't work. E.g. a virus able to infect humans. But there are things we should be concerned about
On the first possibility, Joshua Lederberg who first characterized the Archaea said:
Not saying at all that it is going to happen, or is inevitable. As Carl Sagan said once for Mars,it could be that you can ingest kilograms of Enceladus life without any ill effects. But if you don't know what is in it, you have to be prepared for anything Legal complexitiesMargaret Race covered these in an excellent paper, there's far more to it than you'd think. Back in days of Apollo, then the quarantine rules for the Apollo 11 return were only published on the day that they launched to the Moon. That would simply not be permitted today. And the Apollo regulations have lapsed BTW. And there are many domestic and international regulations to be negotiated and new laws to be passed. She considered the whole process likely to take ten years or more, and it can also potentially involve the domestic laws of nations that are not receiving the sample, because of the potential effect of the worst case scenario could impact on all nations. First idea to bypass all this - characterize before returnSo this whole baroque complexity can be bypassed completely if we simply don't return it to Earth quite yet. So the simplest solution is to characterize the sample before you return it. If we start with in situ missions first, then by the time we do a sample return, we may know what is in it so well that we don't need to do anything much. Either we know it is harmless, or we know it is hazardous but know what needs to be done to prevent harm. Second idea, to return to HEOIf we do return and are unsure, then I think safest return is to High Earth Orbit. Above geostationary, or geostationary. With L1 or L2 it could potentially spiral out and then after flybys of Earth and Moon leave the Earth and enter independent orbit around the sun and eventually return and impact Earth. In HEO then it's orbit is stable for the indefinite future. So we have plenty of time to decide what to do. If so that could be a low cost sample return from Enceladus. We don't need to build a receiving facility in orbit. The capsule needs to be returned with trajectory biasing, obviously not aerobraking in LEO, and need a way for it to get into HEO without close approaches to the Earth that endanger collision with the Earth. Once there in a stable orbit, we may enclose it in a larger "holding" spacecraft. Then anyone can send their own robotic missions up there to study it. This is for the 2030s. So by then we can send up equipment far more capable than our current Mars rovers to study it. Also with the sample so close to Earth we have near to real time telepresence.. By then probably already be using telerobotics routinely for repairing satellites I think. Dextre is gradually step by step working towards satellite repair capabilities, as is Darpa, involved in an initiative for repair of civilian spacecraft in GEO And by then with heavy lift we'll be able to send hundreds of tons into HEO. And telerobotics surely much advanced. We already have telerobotic surgery as routine.
So that should completely safe for planetary protection so long as material is only transferred one way. And no chance of impact with Earth. So that then would simplify everything. No need to convince general public and ourselves that we have everything covered and that nothing can possibly escape containment. Because it is in a stable orbit at GEO, or just above, obviously can't impact on the Earth.
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