Mars, life on
Has there been life on Mars in the past? If so, does it exist there still today? These questions remain open and of keen interest to the astrobiologist. Conditions on the surface of Mars would once hve been much more conducive to the survival of life as we know it. The average temperature was higher, the atmospheric pressure was greater, and there was plenty of surface water – though exactly how much and how long it remained are important unresolved issues. Given the ability of hardy microorganisms known as extremophiles to thrive in what appear to us to be very harsh conditions on Earth, the possibility of present-day Martian microbes certainly can't be ruled out. Such creatures could have evolved several billion years ago, when Mars was more similar in its climate to Earth, and then gradually adapted as the environment turned less friendly. In particular, microbial survivors on the Red Planet may have retreated underground where it is warmer, probably wetter, and better shielded from the Sun's harsh ultraviolet rays. The prospects for residual life on Mars appear to have been raised by the announcement, in 2004, of the discovery by the Mars Express orbiter of trace amounts of methane and ammonia in the Martian atmosphere.
Although advocates of pluralism from the 17th century on had built a case for Martian life on purely philosophical and theological grounds, it was William Herschel who first made astronomical observations of the planet that were detailed enough to be relevant to the debate. From his telescopic studies in 1783, Herschel concluded:1
The analogy between Mars and the earth is, perhaps, by far the greatest in the whole solar system. The diurnal motion is nearly the same; the obliquity of their respective ecliptics, on which the seasons depend, not very different; of all the superior planets the distance of Mars from the sun is by far the nearest alike to that of the earth ... If, then, we find that the globe we inhabit has its polar regions frozen and covered with mountains of ice and snow, that only partly melt when alternately exposed to the sun, I may well be permitted to surmise that the same causes may probably have the same effect on the globe of Mars ... I have often noticed occasional changes of partial bright belts ... and also once a darkish one, in a pretty high latitude... And these alterations we can hardly ascribe to any other cause than the variable disposition of clouds and vapors floating in the atmosphere of that planet.
Writing in 1870, Richard Procter 2 took Herschel's Mars-Earth parallels further and argued vehemently for advanced Martian life based on the assumption that Mars was well supplied with both water and atmosphere:
Shall we recognize in Mars all that makes our own world so well fitted for our wants – land and water, mountain and valley, cloud and sunshine, rain and ice, and snow, rivers and lakes, ocean currents and wind currents, without believing further in the existence of those forms of life without which all of these things would be wasted? ... it is yet to speculate ten thousand times more rashly to assert ... that Mars is a barren waste, either wholly untenanted by living creatures, or inhabited by beings belonging to the lowest orders of animated existence.
The astronomical evidence seemed to continue to favor life following Giovanni Schiaparelli's announcement that he had seen regular linear markings on the surface, though no one could have imagined how far speculation over his canali would lead. By 1892, Camille Flammarion 3 had leapt to the conclusion that:
[T]he present inhabitation of Mars by a race superior to ours is very probable... The considerable variations observed in the network of waterways testify that this planet is the seat of an energetic vitality ... [We] may hope that, because the world of Mars is older than ours, mankind there will be more advanced and wiser.
In the fertile imagination of Percival Lowell, this portrait of an intelligently-populated planet attained its most elaborate form. Though Lowell's Mars was far less hospitable than Procter's, this was seen by him as no barrier to its habitation. On the contrary, the difficulties imposed by the environment had led the Martians to engage in such heroic hydrological schemes that evidence of them was visible from Earth. By the early years of the twentieth century, professional opinion was shifting inexorably away from the notion of advanced life on Mars. Increasingly, Mars seemed too dry, airless, and cold to support anything more than primitive vegetation. Yet, as late as 1936, one of the founders of the British Interplanetary Society, felt able to write: 4
On Mars, the crumbling remains of ancient civilizations may be found, mutely testifying to the one-time glory of a dying world.
Indeed, in the very decade that the Space Age began, Willy Ley and Wernher von Braun's The Exploration of Mars 5 contained a haunting illustration by Chesley Bonestell of the ruins of a Martian temple. That dream, of finding the remnants of a long-dead race, quickly vanished as close-up pictures arrived in 1964 from the first successful Mars probe, Mariner 4, of a crater-strewn wilderness seemly not unlike that of our own Moon. However, in 1971, Mariner 9 brought renewed hope of finding past and even extant biological activity, with its images of what appeared to be dried-up river channels. Such was the revival of optimism that only a few weeks before the first Viking landing, Carl Sagan and Joshua Lederberg went so far as to suggest 6 that: "Large organisms, possibly detectable by the Viking lander cameras, are not only possible on Mars; they may be favored." In the event, nothing so spectacular was found, although the Viking result's are still open to a variety of interpretations, both chemical and biological.
The discovery on Earth of a number of meteorites from Mars has opened up a couple of extraordinary possibilities. One is that some of these rocks actually contain evidence of past Martian life in the form of fossils and biogenic chemical signatures. The other possibility, which remains valid whatever the final verdict on the fossils claim, is that microorganisms could travel between worlds aboard material shot into space during asteroids collisions. Life may have been seeded on Mars from Earth. Or, more extraordinarily, it has been suggested that life may have evolved first on Mars and then come to Earth by the process of ballistic panspermia.7 According to this idea, Mars afforded a safer haven for primitive life during the early, violent bombardment phase of the Solar System, between about 4.6 and 3.8 billion years ago. Whereas the Earth was probably hit repeatedly by objects up to 500 kilometers across which would have vaporized the oceans and created a deadly steam atmosphere, fewer giant impacts would have taken place on Mars (because it is a smaller target) and the absence of large amounts of surface water would have saved the planet from being as severely steam-sterilized. Any Martian thermophiles living just a few hundred meters below the surface, it has been suggested, would have been able to survive the trauma of collision with a 500-km-wide object. Furthermore, because of Mars' relatively cool interior and low gravity (allowing cracks, in which microbes could reside, to extend further down into the planet's interior) thermophilic subterranean organisms may have existed in a wide habitable zone extending to depths of several thousand meters. On Earth, by comparison, although thermophiles 1 km below the surface might have survived an ocean-boiling impact this would have left an uncomfortably narrow habitable zone – much below 1 km and microbes would probably be cooked by the planet's hot interior.8, 9
Herschel, W., "On the Remarkable Appearances at the Polar Regions of the Planet Mars, the Inclination of its Axis, the Position of its Poles, andf its spheroidal Figure; with a few Hints relating to its real Diameter and Atmosphere," Philosophical Transactions of the Royal Society of London, 74, 233 (1784).
Procter, Richard. Other Worlds Than Ours. New York: P. F. Collier (1900) (first published 1894).
Flammarion, Camille. La planÃ¨te Mars et ses conditions d'habitabilitÃ©. Paris: Gautheir Villars et Fils (1892).
Cleator, P. E. Rockets Through Space, p. 195. New York: Simon & Schuster (1936).
Ley, Willy, von Braun, Wernher. The Exploration of Mars, New York: Viking (1956).
Sagan, C., and Lederberg, J. "The Prospects for Life on Mars: A Pre-Viking Assessment," Icarus, 28, 291 (1976).
Sleep, N. H., and Zahnle, K. "Refugia from Asteroid Impacts on Early Mars and the Early Earth," Journal of Geophysical Research, 103, no. E12, 28529 (1998).
Goldsmith, Donald. The Hunt for Life on Mars, New York: Penguin Books (1997).
Hansson, Anders. Mars and the Development of Life, 2nd ed. New York: John Wiley & Sons (1997).