George Lebo 24 October 2012 AST 2037

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Presentation transcript:

George Lebo 24 October 2012 AST 2037 Life: What Do We Expect? George Lebo 24 October 2012 AST 2037 1

Life Needs Need energy source and reproductive code Likely energy sources: light, chemical energy Reproductive code: likely chemical, and requires complex molecules/chains A little weaker: May have a preference for liquid phase? Probably need a powerful solvent 2

Complex Molecules Abundant elements in the Universe: H (can only bond with one electron) He (noble gas) C O Ne (noble gas) N Si Fe 3

Other Options? Oxygen only makes two stable molecules with hydrogen: water (H2O) and hydrogen peroxide (H2O2) Nitrogen only makes two also: ammonia (NH3) and hydrazine (N2H2) Fe also relatively limited in its bonding Carbon makes a nearly endless number of molecules/isomers with H Si also makes lots of molecules too 4

Si vs. C Both C and Si can make complex chains and diverse molecules But … C-C bond is about as strong as C-H and C-O bonds Si-Si bond is about ½ as strong as Si-H and Si-O bond Carbon can make long C-C-C chains Silicon unstable for long chains; Si-O can form chains (silicone), but they don’t like to attach other elements (often used as lubricants) If oxygen present, Si forms SiO2 preferentially (while many C molecules about equal – CH4, CO, CO2, alcohol, sugars, etc.) SiO2 (quartz/sand) is a solid at most reasonable temperatures for complex chemical reactions; only soluble in hydroflouric acid 5

Si Life? Develops elsewhere, comes to Earth “Skin” must be resistant to oxidation  SiO2 (rock) “armor” Digestion might produce silane SiH4 (analogy to CH4 methane) Belch silane into oxygen atmosphere  preference for Si-O bonds creates rapid chemical reaction in the gas  ignites into flame What would that look like? Rock for skin  impervious Breathes fire 6

Solvent Issues Want broad temperature range for liquid state Common molecules High thermal capacity Can “move” heat around for temperature regulation (important for complex life – probably …) High heat of vaporization Evaporative cooling Lower heat of vaporization means less efficient cooling 7

Possible Solvents H2O is most common molecule in the Universe, after H2 Other contenders: Ammonia Methyl alcohol Ammonia has only ~45C temp range as liquid Methyl alcohol has OK temp range but ~1/2 heat capacity of water Water has about x2 higher heat of vaporization These others can work (esp., liquid at lower temps than water); but, we expect water to be better 8