The organic speck methanol was once thought to be a possible index number there was life under the surface of Saturn ’s icy moon Enceladus . But we ’ve just find a ton of methanol elsewhere around Saturn – suggesting it is not   as important as we thought .

A few month ago , NASA confirmedthat under the ice of Enceladus there ’s hydrothermal activity that propels complex molecule into infinite . The Cassini investigation detected atomic number 1 , atomic number 6 dioxide , and wood alcohol , among other substances , and now a study indicate that we might have been wait at only part of the picture .

In a subject field presented at theNational Astronomy Meetingat the University of Hull in the UK this week , researchers foretell the uncovering of a smashing amount of methanol in the Saturnian system than the previous detection made by Cassini as it flew through plumage ejected by Enceladus . This suggests that methanol output might be happening aside from this icy Sun Myung Moon but still driven by the moon itself .

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" [ O]ur finding suggest that that methanol is being create by further chemic reaction once the feather is turn out into space , make it improbable it is an denotation for lifespan on Enceladus , ” Dr. Emily Drabek - Maunder , who is   submit the research , articulate in a statement .

These observance were conducted by Dr. Jane Greaves of Cardiff University and Dr. Helen Fraser of the Open University ,   using the IRAM 30 - meter wireless scope in Spain .

The plume of Enceladus fuel material in the E - ring of Saturn , and in the squad ’s observation , they short found a very promising emission of methyl alcohol . The detection of this complex molecule ( made of carbon , hydrogen , and O ) was not expected , and when they see such a unmortgaged key signature , they knew something odd was happening .

This point at   two possible account for the substantial sign . Either the methanol from the plumes interpenetrate deep into the E - ring than thought , or a large cloud was trammel by Saturn ’s magnetized field . Either option though ca n’t explain the more abundant methanol unless it ’s take shape in distance .

While organic molecules like wood alcohol can be produce by lifeforms , they can be produced by chemical cognitive process too . This inquiry suggests that the latter is more potential to be the case for Enceladus . But the detection is important by itself , both for the method acting and its implications .

" This observation is incredibly important because it is the first espial of a molecule in Enceladus ' vicinity from a priming - based scope , " Dr. Drabek - Maunder told IFLScience .

" The   Cassini ballistic capsule   is coming to an end towards the end of the yr , and   in - situ [ direct ] observations from future   space missions wo n’t be possible for another decade or so . The only way for us to carry on studying this environs in the lag is by using outside telescopes . "

Cassini is now in the last few calendar month of its commission before it takes a last plunge into Saturn at the end of September . A new Saturn mission is presently in the works , but until that come about basis instrument are the best we have . And there ’s plenty more scientific discipline that they can do .

" One really interesting thing ground - establish observatories can do in the meantime is to study how Enceladus ' plume deviate in time , " enounce Dr. Drabek - Maunder . " In past flybys , Cassini find that Enceladus ' huffs and puffs ' , intend the plumes seem to be brighter when Enceladus is furthest aside from Saturn . However , we do n’t know if the molecules being ejected from Enceladus vary over time and if variability is also found within the E - hoop . "

We learned so much about Saturn in the 13 old age Cassin explore it . But it seems there ’s a lot more to con .