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February 26, 2004
If you take a look at some of the orbital imagery of Meridiani, you will see that there appears to be quite a bit of reef and outcroppings around, but if you look very carefully, you notice that most of these are the eroded away circular remnants of earlier cratering. Eroded as in melted, slumped or subsided, as in ice and water. http://www.msss.com/moc_gallery/e13_...8/E1801275.jpg Now think about what a putative or hypothetical 'porifera jonathanii' would have to deal with in surviving. Not only would it have to deal with extreme environmental fluctuations, melting and thawing of ice sheets, runoff etc., but it would also have to deal with the occasional incoming impacts. A better way to propagate itself *and* deal with random impacts in such an environment, is to leave millions of hardened, impact resistant, aerodynamically stable gemmules laying around, ready to ride the (shock) waves into the next quadrant. If you choose the water and ice hypothesis then you have to start thinking about life, and fossils. If you choose the fossil hypothesis, you have to start thinking about natural selection and biology, in addition to planetary geology. Here is a modern paper on gemmulation and oogenesis. It describes the 'launch pad' very nicely. I propose that many large, robust, spherical gemmules could be a result of natural selection. http://www.bio.pu.ru/win/embryo/art/haplosclerida.pdf Just a thought. Thomas Lee Elifritz http://elifritz.members.atlantic.net |
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