Hans Blaster
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- Mar 11, 2017
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The paper itself mentions "life" three times.On the subject of exoplanets, the pop-sci press generally deviate from the scientific publications by focusing more on the sensationalist aspect of looking for life forms.
As this thread has revealed, the scientific objective is to have a confidence level the so called biosignatures are real and not some statistical anomaly.
In the introduction (on background):
"The Hycean paradigm developed in recent years has
the potential to significantly expand and accelerate the
search for life elsewhere."
And referencing other studies:
"Another potential indication of
biological activity was suggested by a weak (≲2-σ) infer-
ence of dimethyl sulfide (DMS) in K2-18 b with previous
JWST observations (Madhusudhan et al. 2023b).
The tentative inference of DMS in K2-18 b opens an
important debate on the possible presence of life on K2-
18 b. "
And in the discussion at the end:
"The spectrum shows multiple spectral features between
∼6-11 μm which are best explained
by a combination of DMDS and DMS in the atmosphere,
both molecules uniquely produced by life on Earth and
predicted as promising biosignatures in habitable exo-
planets".
"Their [DMDS and DMS] identification [in theory papers] as robust
biosignatures is due to the fact that on Earth, both
molecules are uniquely produced by life (particularly
marine biota) in small quantities of ≲1 ppb by volume
and are not supplied by abiotic photochemistry. Never-
theless, here we explore some potential alternatives."
This was a transmission spectroscopy study.The direction technology needs to take are straightforward to go from a three sigma to a five sigma level or reveal the anomaly.
A current limitation is the light reaching the spectrometers is polluted with starlight combined with light reflected from the exoplanets or passing through their atmospheres.
There is some planet exploring mission that is now at risk due to proposed budget cuts, but I don't remember the name of it.To alleviate this limitation is to build larger telescopes which are in the pipeline. Larger telescopes not only collect more light but are theoretically able to resolve stars into disks which appear as point sources in smaller telescopes. This allows starlight to be filtered out before it reaches the spectrometer.
The two methods being researched are using coronagraphs which are smaller telescopes built inside the earth or space based telescope.
The other is the use of starshades which are spacecraft placed thousand of kilometres in front of the telescope and use petal shaped obstructions designed to minimise diffraction and to create a deep shadow on the telescope optics.
Both methods will greatly increase the S/N ratio.
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