A Look at the Case for Moon Life

Science in the News
by Hugh Ross

Fervently optimistic about life's existence elsewhere in the cosmos, some scientists have abandoned the old notion that life requires an Earth-like home. A satellite (moon) orbiting a giant planet that in turn orbits a star resembling our sun at a distance nearly identical to Earth’s distance from the sun could be, they say, a life site. 1-3

How feasible is such a suggestion, and, if feasible, how would it impact our conclusions about God’s design of the solar system? The following three considerations, among others, shape my response:

First, while planets outside our solar system do exist, and while they may (though it is unlikely) orbit their stars at appropriate-for-life distances,4-5 their orbits would likely be too unstable to accommodate a moon-life scenario. Giant planets do not (in fact, cannot) form close to their stars. They either drift there or are bounced there under the influence of gravity and other physical forces. The likelihood that such a planet would end up a habitable distance from its star and with a stable, nearly circular orbit is miniscule.6-11 The extra-solar (outside our solar system) planets we do see anywhere close to life-habitable distances from their stars have such highly elongated orbits as to make life on any of their moons impossible.12 Their seasonal temperature differences would be far too extreme. An important and yet unanswered question is whether or not giant planets can even hold onto their satellites as they (the planets) migrate.

Second, a moon orbiting far enough away from its planet to avoid "tidal locking" (sticking by gravity with the same face always toward the planet) will at one point in its orbit be too close to its star (thus too hot) and at the opposite point too far from its star (too cold) for life to survive. Ameliorating the temperature extreme through a very dense atmosphere will not work as the accompanying article by Guillermo Gonzalez demonstrates.13 On the other hand, a moon in close orbit about a planet like Jupiter would be bombarded by speeding charged particles (accelerated by the planet’s magnetosphere). These energetic particles would sputter away the satellite’s atmosphere, making the place uninhabitable. Wind from the parent star also would contribute significantly to the sputtering of the satellite's atmosphere. Escape from this catastrophe would be possible only if the moon were to possess a strong magnetic field. However, just a few solar system bodies have strong magnetic fields: the sun, Jupiter, and Earth. Ganymede, the largest solar system moon and the only one with an undisputed magnetic field, has a very weak one, less than one percent as strong as Earth’s.14, 15 It is too weak to prevent sputtering in Ganymede’s polar regions, and this sputtering would inhibit life-essential cloud formation.16

Third, a life-supporting moon would need enough mass to hang onto (by gravity) an appropriate atmosphere. On that basis alone, such a moon would have to possess at least 12% the mass of Earth.17 Other factors beyond mass and gravity, however, affect a body's capacity to sustain an adequate atmosphere. 18 The long list sounds like "The House that Jack Built," but it ends with the carbonate-silicate cycle, which requires a just-right balance of dry land, plants on the dry land, the right ratio between dry land and ocean surfaces to permit sufficient weathering, and plate tectonic activity.19, 20 These factors add up to the need for a moon that's nearly one-fourth as massive as Earth. In that case, it would be eight times more massive than Ganymede, which orbits Jupiter, and more than twice as massive as Mars, which is the seventh largest planet in our solar system—not a satellite we're likely to find anywhere in the cosmos. Incidentally, this need for dry land and plate tectonics eliminates the totally ice-water environments such as Jupiter's moon Europa as long-term life sites. More reasons than these could be cited for skepticism about moons as life sites.21, 22 No doubt even more reasons will be discovered in the next few years. While I cannot yet say that research has sealed the case, evidence strongly suggests that a long-term home for life requires divine engineering.

References:
1. J. F. Kasting, D. P. Whitmire, and R. T. Reynolds, "Habitable Zones Around Main Sequence Stars," Icarus 101 (1993), pp. 108-128.
2. Darren M. Williams, James F. Kasting, and Richard Wade, "Habitable Moons Around Extrasolar Giant Planets," Nature 385 (January 16, 1997), pp. 234-236.
3. Darren M. Williams, "Habitable Moons Around Extrasolar Giant Planets," in The Stability of Habitable Planetary Environments, a Ph.D. Thesis in Astronomy and Astrophysics, Pennsylvania State University (May 1998), pp. 111-120.
4. Ron Cowen, "Scientists Puzzle Over Extrasolar Planets," Science News 154 (August 8, 1998), pp. 88-90.
5. URL: wwwusr.obspm.fr/departement/darc/planets/encycl.html.
6. Frederic A. Rasio and Eric B. Ford, "Dynamical Instabilities and the Formation of Extrasolar Planetary Systems, Science 274 (November 8, 1996), pp. 954-958.
7. N. Murray, B. Hansen, M. Holman, and S. Tremaine, "Migrating Planets," Science 279 (January 2, 1998), pp. 69-72.
8. D. N. C. Lin, P. Bodenheimer, and D. C. Richardson, "Orbital Migration of the Planetary Companion of 51 Pegasi to Its Present Location," Nature 380 (April 18, 1996), pp. 606-607.
9. Stuart J. Widenschilling and Francesco Marsari, "Gravitational Scattering As a Possible Origin for Giant Planets at Small Stellar Distances," Nature 384 (December 19/26, 1996), pp. 619-621.
10. Gregory Laughlin and Fred C. Adams, "The Modification of Planetary Orbits in Dense Open Clusters," Astrophysical Journal Letters 508 (December 1, 1998), in press.
11. Stuart Ross Taylor, Destiny or Chance: Our Solar System and Its Place in the Cosmos (Cambridge, UK: Cambridge University Press, 1998).
12. Ron Cowen, p. 88.
13. Guillermo Gonzalez, "How Wide the Life Zone?" Facts & Faith, v. 12, n. 4 (1998), pp. 5-6.
14. D. A. Gurnett, et al, "Evidence for a Magnetosphere at Ganymede from Plasma-wave Observations by the Galileo Spacecraft," Nature 384 (December 12, 1996), pp. 535-537.
15. M. G. Kivelson, et al, "Discovery of Ganymede’s Magnetic Field by the Galileo Spacecraft," Nature 384 (December 12, 1996), pp. 537-541.
16. M. G. Kivelson, et al, p. 541.
17. Darren M. Williams, pp. 115-117.
18. Hugh Ross, The Creator and the Cosmos, second edition (Colorado Springs: NavPress, 1995), pp. 134-135.
19. Katherine L. Moulton and Robert A. Berner, "Quantification of the Effect of Plants on Weathering: Studies in Iceland," Geology 26 (October, 1998), pp. 895-898.
20. Darren M. Williams, pp.119-120.
21. Hugh Ross, pp. 143-144.
22. Hugh Ross, Big Bang Refined by Fire (Pasadena, Calif.: Reasons To Believe, 1998), pp. 27-29.