Lecture 30: Life on Exoplanets Flashcards
(7 cards)
explain how atmospheric chemistry is complex and many gases have nothing to do with biology
volcanic gases, lighting, and atmospheric photochemistry all interact
explain how some gases can be used as biosignature gases such as oxygen
oxygen highly reactive, so without constant production, it would quickly combine with other elements and disappear
so, detecting large amounts of oxygen in an exoplanets atmosphere could suggest ongoing biological activity
why do we have to be careful of ‘false-positive’ detection of biosignature gases
abiotic production of oxygen by photolysis of water
the O2 so produced tends to react with rocks and become consumed
but, higher concentrations can be produced if there is lots of water or geological activity is not so great so that oxygen builds up
when might it be hard to see a biosignature?
clouds etc
presence of gaseous biosignature
- gaseous biosignature can be seen (oxygen), but no surface signature exists
why was it once hard to tell if there was life on earth?
because oxygen biosignatures have only existed for about 2.4 million years
what have some people considered looking for when in search of extraterrestrial intelligence?
technosignatures
signs or evidence of technological activity by intelligent extraterrestrial civilisation
what are the required characteristics of a biosignature?
- produced by life
- produced in negligible amounts by abiotic processes
- clearly detectable signature