Complex Organic Spectral Pointers to Life on Five Solar System Worlds

by Craig Carmichael (independent researcher) May 2007
 
 

1. Unusual Spectral Readings on Five Worlds

There seem to be five worlds in our solar system whose surface has been reported as being abundantly covered with complex organic "tholins" compounds:

* Earth
* Ganymede
* Callisto (especially the leading hemisphere)
* Iapetus (leading hemisphere only)
* Titan
AFAIK, complex tholins have not been reported as being present even in small quantities on any other worlds. (If any trace of such organics had been found on Mars, it would probably be front page news!)
Without successfully looking up Earth in such obscure terms of reference, I presume the "tholins" of Earth are unique in the solar system, just as are those of Titan. Earth and Titan are mid-atmospheric worlds, though otherwise having considerably different natures. Allowing for differences of equipment aboard Galileo and Cassini, and for differences of what the authors of the various unconnected writings thought was worth reporting about the results found, the tholins of Ganymede, Callisto and Iapetus would appear likely to be similar. (For example, sulfur is mentioned on Callisto but not Ganymede or Iapetus, but there is reason to believe at least for Ganymede that the omission is probably in the reporting rather than in the actual findings.) On the other hand, the albedos of the surfaces differ, perhaps with tholin density. The general albedo of Ganymede is .4, Callisto is .2 and Iapetus's dark side is darkest of all at just .05.

It was a surprise that the Galileo found tholins on Ganymede and Callisto - unexpected and unpredicted. Others have supposed that they should also be present on Europa, yet there is no sign of them there. Some of the tholin compounds have not been identified. Having found tholins on Ganymede and Callisto, scientists were not so surprised when they were also found on Saturn's moon Iapetus. Still, they are unexplained. Several worlds show simpler organic molecules. There are organic readings on Saturn's odd moonlet Phoebe, but these differ spectrographically and I expect they are probably fairly simple molecules.It seems improbable to me that these complex and doubtless fragile compounds should have persisted on planetary surfaces through their meteoric accretion stages with the attendant heating and geological morphology, even if they had existed in cometary material supposed to be "abundant in the solar nebula". I propose that, as on Earth, it is living organisms that form complex organic compounds. It seems to me life is the obvious and simple interpretation of the spectralfindings.

There is more evidence:

Analysis of spectral data from the Voyager probes found that the temperature profiles of Ganymede and Callisto were best explained by a two-layer surface with the top layer having a very low thermal inertia[1]. This would seem consistent with a covering of vegetation over the ground.

On Iapetus, "the dark material appears to lie on top of other geologic features seen on Iapetus thus far, implying that the event which formed the dark coating occurred later in Iapetus' history."[2] Again, this and the idea that the dark material is "a relatively thin layer"[2] is consistent with vegetation on the surface.

On Titan, the tholins found are said to be "the building blocks of life", and compounds such as ammonia, found on the surface but not in the atmosphere, are thought to be "the end products of a complex organic chemistry". There is "an unidentified blue slope in the near infrared". If life on Titan seems incredible, is it not even more incredible that, in the absence of life, there should be complex and unidentified organic compounds "unique in the solar system", and complex organic chemical reactions occurring on the surface? Cassini and Huygens findings indicate no UV or other energetic radiation, lightning hasn't been detected, and there are low wind speeds and gentle conditions. What but life would stir the elements to these unique organizing activities?

2. Visual Aspects: The Face of Life

Interpretation of spectrographic results as being indicative of life is not without support from the imaging. Scrutiny of the nearest images from both Ganymede and Titan indicate, at least to some viewers, that they both appear to be covered with vegetation. It's not very clear, but it is as clear as the space probes sent could be expected to show such things. It would doubtless be much more clear (or else counterindicated) if any of the closest images had been taken in color, but unfortunately, neither Galileo, Cassini nor Huygens was (is) capable of taking color images of nearby planetary surfaces. The best views of vegetation on Ganymede are the images of regions 30 - 45 degrees north latitude at about 50 meters per pixel, taken obliquely from Galileo passing by over the equator. Finer scale views of Titan, especially the Cassini SAR RADAR images and the Huygens images, appear to disclose lush vegetation both on land and in the liquid methane.On both Ganymede and Titan, the scale of the vegetation is gigantic compared to Earth, allowing us to see it even from space and making it hard to believe. If there were large scale human works such as Earth's cities on Ganymede or Titan, they should have been seen, so we may infer that there are no advanced civilizations comparable to Earth's on these worlds. Animal life, unless seen by the Huygens probe after landing or unless incredibly huge, should definitely have been too small to image with any certainty of identification, so the presence or status of animal life, and human life, on either sphere is, predictably, undetermined.

Why should we be surprised by giant vegetation on low gravity worlds? The theoretical limit to tree height on Earth has been calculated as being 120 meters, and the tallest actual trees are about 140 meters. This is related to the ability of plant cells to push sap from the base of the tree to the top against gravity by cellular capillary action. Ganymede and Titan both have 1/7th of Earth's gravity. All else being equal (for purposes of gross estimation), one might expect trees could grow 7 times as tall, or 120 * 7 = 840 meters. One thing that's not equal on Titan is that the liquid is methane, density .8, instead of water, 1.0, so it's lighter to push up the stalk: 840 meters / .8 = 1050 meters. That's trees a kilometer tall, and it's why forest canopies are visible on Titan in radar images from space even at 30 meters per pixel rez, and why individual branches and tree trunks (the "poles") can be discerned on Ganymede. Something that throws a wild card into vegetation heights on Ganymede is that in a vacuum there really ought to be no liquids. The vegetation must either create its own internal pressure to where liquid can exist, or else Ganymedean "sap" is a gas going up the stalks. Obviously, gas could be pushed up any conceivable height of stalk and wouldn't be the limiting height factor. A thick skin that holds in gas or liquid could perhaps account for the 'gelatinous', 'globby' appearance of certain forms of Ganymedean vegetation.Callisto discloses no plant forms large enough to be discerned in the closest Galileo probe images. However, its entire surface besides icy slopes and other bare ice areas appears to have a "blanket" which obscures smaller surface features, and which has been variously described as "dark", "gritty" and "fluffy". Indeed it looks so little geological that an electrostatic charge holding "grit" aloft has been proposed (seems absurd - whence cometh this charge?), as well as sublimation of ice from flatter areas, leaving the darker material. (and why, and where does the ice sublimate to?) Whatever it is, this happens also to be the appearance one would expect from dense vegetation too small to image. Iapetus has only been imaged at many hundreds of meters per pixel, and there are no plans to view it from close enough to certainly discern even very huge plants.


Colorized version of Galileo image of Ganymede. (@2x)
(Image #359946139, 35 degrees North, 186 degrees West, 45 x 73 meters per pixel, imaged from Galileo, flying over the equator. This geometry has provided a fine perspective view.)
The colorizations, while they doubtless misinterpret some of the forms and details, highlight many amazing image features people appear to have paid little attention to. Some other interesting features are not colored. On inspection, the majority of the short vertical lines do not appear to be image artifacts. What are they if not trees?
 
 

3. Migration and Distribution of Ganymedean Life

Why these worlds, and no others? It is my belief that the life which seems to exist according by the spectral readings on Callisto and Iapetus, originated on Ganymede. Meteors occasionally spew up debris including seeds, spores or living roots from Ganymede's surface. Some exceed Ganymede's escape velocity and some (evidently) eventually fell onto other acceptable airless worlds and grew.So, why should Ganymedean life flourish on two other worlds but no others? It isn't hard to start eliminating worlds as possibilities. Io is so hostile to life it can be immediately dismissed. (No human will ever go near it!) Likewise, anything that hit Europa would soon die of radiation poisoning if it didn't en route. The same might perhaps apply to Saturn's small inner moons (Rhea, Dione and Tethys) as well as Mars (unfiltered UV there). Mars is also probably too hot and has an atmosphere that may well be inimical to Ganymedean life (and would fry it during landing). Dione and Tethys may be simply too small. (I thought Iapetus would have been too, and also that the Saturn environs would have been too far from the sun for Ganymedean life... but the Iapetus spectral readings are there.) An alternative reason nothing is found on Rhea may be simply that nothing from Ganymede has ever landed alive on its leading hemisphere. Or, its geology may provide little but hard ice for soil. Jupiter's magnetic field sends charged particles bombing into the trailing hemispheres of its satellites, but Ganymede has its own magnetic field to deflect these. Callisto has a weak and varying magnetic field that is electromagnetically induced by Jupiter's field in liquid water deep under the crust. This is protection of a sort but not very good protection, so Callisto's trailing hemisphere is somewhat unfriendly to life and a lower density of tholins is seen there than on the front half. Iapetus is much too small to have any magnetic field, so its trailing hemisphere is freely bombarded by Saturn's magnetic field, making it relatively uninhabitable to life, while the leading hemisphere has grown dark with migrated Ganymedean plants, which could, perhaps, in Iapetus's 1/40th gravity, possibly grow very huge indeed.

Earth of course has its own magnetic and other protections from the energies of space, and no doubt atmospheric Titan has its own shields -- some have been identified. For example, elements of its upper atmosphere reflect UV rays back the way they came!
 

Since on Iapetus the dark "life area" geography is well defined and there are images of it, here is some detail. The same could perhaps be done for Ganymede (presumably showing latitude differences only) and Callisto (latitudes and longitudes) if there are images and if the regions are defined well enough.

First let me say the idea that Iapetus's dark coating came from material blasted off the distant moonlet Phoebe has so many flaws that in the interests of brevity I won't discuss it. It is just one of a number of impossible ideas that attempt to explain the images of life on these various worlds in terms of non-living phenomena.

The boundaries of Iapetus's dark area and the constancy of the darkness within that area are relatively convincing as describing the region where vegetation seems plausible. It is distributed throughout the lower latitudes without notable gaps, and comes to faily well defined northern and southern limits at 45 to 50 degree latitudes:


And it ceases on the trailing face, exposed to Saturn's magnetosphere, first in the temperate regions, and more gradually in the tropics in a semicircular shape, at both ends. I suppose it doesn't end very suddenly because Iapetus essentially orbits beyond Saturn's field except when it passes through the magnetotail. Iapetus thus only receives very modest doses of ionic radiation compared to Saturn's inner moons:


Especially at its eastern extremity near the equator (facing Saturn), vegetation appears to spread a fair ways onto the trailing hemisphere within what I presume are sloped areas somewhat sheltered from the magnetosphere's ionic particle impacts. One sees a somewhat dark ring in an impact basin, "the moat", on the right above as being relatively flat and dark; a higher resolution image gives the possible impression of steep terrain with smaller dark areas sheltered westward of various hills and scarps. But it is difficult to tell shadows from darker terrain in monochrome images of Iapetus.

There is an excellent color image (PIA06167) in which shadows are quite distinct from terrain brightness.  Though it doesn't extend across an east-west boundary, in this small excerpt the dark brown coating can be seen to gradually thin to light grey towards the north pole. Again appropriate to the vegetation model, northern walls of craters, facing south and thus simulating lower latitudes in small selected areas, have the dark coating. Some whispy darker streaks of higher latitudes also appear to disclose southerly oriented slopes.

4. Conclusions and Forecast

The first conclusions are of human factors: Excellent spectrographic and visual evidence for life on other worlds in our own solar system appears to have been overlooked, evidently through simple disbelief that life could possibly exist on any of these spheres. We tend to look for conditions where Earth life could perhaps thrive, even to saying "there must be liquid water", and we ignore environments that don't meet Earth life conditions. But we know life on Earth thrives under many unusual conditions, one of the most unusual of which is perhaps the microbes living in liquid carbon dioxide (a non-polar molecule I expect) trapped under solid carbon dioxide hydrate in deep ocean trenches. If our Earth biased criteria of factors like liquid water, air pressure and temperature aren't met, we don't relate to other important life conditions, such as a world having a magnetic field and an ozone layer and orbiting in a quiet space zone. More direct conclusions: Interpreting the presence of complex organic tholins on a planetary surface as indicative of life can explain: (a) why they are either abundant, seeming to blanket a planetary surface, or completely absent, never simply "present but rare" on any world (b) why they occur uniformly all over Ganymede but are more abundant on Callisto's leading hemisphere than the trailing one and why they are present only on the leading hemisphere of Iapetus (c) Why they avoid polar regions, especially on cold Iapetus (d) why they appear to exist in a geologically thin layer blanketing a planet's surface[1,2] (e) why they don't occur on worlds with radioactive environments and (f) why they weren't broken down into simpler compounds by heat and pressure during the formation of the sphere: ie, because they grew later.Finally, forecasts: Look for vegetation on the dark leading hemisphere in the images returned from the upcoming Iapetus flyby by Cassini. The flyby is to be regrettably quite distant and thus the resolution will be poor, so failure to identify stems and trunks does not mean it isn't present. Of course, if huge vegetation is indisputably seen, it will pretty much validate this thesis. Some may believe they see vegetation, but as on Ganymede if it isn't crystal clear this will be ignored as there is no possibility of satisfactory proof. On the other hand, as on Callisto plants may be too small to resolve even at "just" a few meters per pixel resolution.If we aren't interested enough today about the weird, alien stuff we're seeing on Ganymede to go back for another look, or even to image Iapetus closely while Cassini is there, it will be left for some future generation. Maybe by 2150 or 2200 mankind will return to Ganymede with a color camera - as there are no plans (with the demise of the absurdly complex JIMO project) even tentative at this point for a return it certainly won't happen within anybody's current lifetime. Titan is more hopeful for a return in the upcoming decades as it has unexpectedly interesting features even without acknowledging that there is life there. Exploration of Callisto and Iapetus - and other, seemingly lifeless, worlds - would of course be interesting and would expand our knowledge of the universe, but they don't hold a candle to exploring Ganymede and Titan, where there are almost undoubtedly animals, and perhaps even people, though if so they don't appear to have built any cities on either world.
 
References


1. http://adsabs.harvard.edu/abs/1987PhDT........81S

Title: The Surfaces of Europa, Ganymede, and Callisto: an Investigation Using Voyager IRIS Thermal Infrared Spectra
Authors: Spencer, John Robert
Affiliation: AA(THE UNIVERSITY OF ARIZONA.)
Publication: Thesis (PH.D.)--THE UNIVERSITY OF ARIZONA, 1987.Source: Dissertation Abstracts International, Volume: 48-03, Section: B, page: 0793.
Publication Date: 00/1987
Category: Physics: Astronomy and Astrophysics
Origin: UMI
Keywords: JUPITER
Bibliographic Code: 1987PhDT........81S

Abstract

In 1979, the IRIS infrared spectrometers on the two Voyager spacecraft obtained over 1000 disk-resolved thermal emission spectra of Europa, Ganymede, and Callisto, Jupiter's three large icy satellites. This dissertation describes the first detailed analysis of this data set. Ganymede and Callisto subsolar temperatures are 10(DEGREES)K and 5(DEGREES)K respectively below equilibrium values. Equatorial nighttime temperatures are between 100(DEGREES)K and 75(DEGREES)K, Callisto and Europa being colder than Ganymede. The diurnal temperature profiles can be matched by 2-layer surfaces that are also consistent with the eclipse cooling observed from earth, though previous eclipse models underestimated thermal inertias by about 50%. Substrate thermal inertias in the 2-layer models are a factor of several lower than for solid ice. These are 'cold spots' on Ganymede and Callisto that are not high-albedo regions, which may indicate large thermal inertia anomalies. All spectra show a slope of increasing brightness temperature with decreasing wavelength, indicating local temperature contrasts of 10-50(DEGREES)K. Callisto spectra steepen dramatically towards the terminator, a trend largely matched with a laterally-homogeneous model surface having lunar-like roughness, though some lateral variation in albedo and/or thermal inertia may also be required. Subsolar Ganymede spectra are steeper than those on Callisto, but there is no steepening towards the terminator, indicating a much smoother surface than Callisto's. The spectrum slopes on Ganymede may indicate large lateral variations in albedo and thermal inertia. A surface with similar areal coverage of dark, very low thermal inertia material, and bright material with thermal inertia a factor of 2 -3 below solid ice, fits the diurnal and eclipse curves, and (less accurately) the IRIS spectrum slopes. Europa spectra have very small slopes, indicating a smooth and homogeneous surface. Modelling of surface water ice migration gives a possible explanation for the inferred lateral inhomogeneities on Ganymede. Dirty ice surfaces at Jupiter are subject to segregation into high-albedo ice-rich cold spots and ice-free regions covered in lag deposits, on decade timescales. Ion sputtering and micrometeorite bombardment are generally insufficient to prevent the segregation. The reflectance spectra of Ganymede and Callisto may be consistent with this type of segregated surface.
 

2. http://ciclops.org/view.php?id=708