これには、James Webb Space Telescopeなどの大きなミラーが必要です。将来の大型宇宙望遠鏡は、K2-18bの観測を継続することにより、この手法に従うことができます。これは、他の大気ガスを発見し、太陽系に存在しないこのタイプの惑星を少しよく理解する機会になるかもしれません。私たち全員が期待する発表は、明らかに、その星の居住可能ゾーンにある岩だらけの太陽系外惑星の大気中の水の発見です。楽観的になりましょう、これは次の10年になりそうです。
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