A new study indicates that some exoplanets may have better conditions for life to thrive than Earth itself has. “This is a surprising conclusion,” said lead researcher Dr. Stephanie Olson, “it shows us that conditions on some exoplanets with favorable ocean circulation patterns could be better suited to support life that is more abundant or more active than life on Earth.”
The first exoplanet was discovered in 1992, and currently, more than 4000 have been confirmed so far. The nearest known exoplanet is Proxima Centauri b, which is 4.25 light-years away.
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Currently, much of the search for life on exoplanets focuses on those in the habitable zone, which is the range of distances from a star where a planet’s temperature allows liquid water oceans, critical for life on Earth.
The discovery of exoplanets has accelerated the search for life outside our solar system. The huge distances to these exoplanets mean that they are effectively impossible to reach with space probes, so scientists are working with remote sensing tool such as telescopes, to understand what conditions prevail on different exoplanets. Making sense of these remote observations requires the development of sophisticated models for planetary climate and evolution to allow scientists to recognize which of these distant planets that might host life.
Dr. Stephanie Olson from the University of Chicago describes the search to identify the best environments for life on exoplanets:
“NASA’s search for life in the Universe is focused on so-called Habitable Zone planets, which are worlds that have the potential for liquid water oceans. But not all oceans are equally hospitable–and some oceans will be better places to live than others due to their global circulation patterns.”
Olson’s team modeled a variety of possible exoplanets using the ROCKE-3D software*, developed by NASA’s Goddard Institute to simulate the climates and ocean habitats of different types of exoplanets. In the end, they were able to define which exoplanet types stand the best chance of developing and sustaining thriving biospheres.
“Our work has been aimed at identifying the oceans which have the greatest capacity to host globally abundant and active life. Life in Earth’s oceans depends on upwelling (upward flow) which returns nutrients from the dark depths of the ocean to the sunlit portions of the ocean where photosynthetic life lives. More upwelling means more nutrient resupply, which means more biological activity. These are the conditions we need to look for on exoplanets”.
“We have used an ocean circulation model to identify which planets will have the most efficient upwelling and thus offer particularly hospitable oceans. We found that higher atmospheric density, slower rotation rates, and the presence of continents all yield higher upwelling rates. A further implication is that Earth might not be optimally habitable–and life elsewhere may enjoy a planet that is even more hospitable than our own.
There will always be limitations to our technology, so life is almost certainly more common than “detectable” life. In our search for life in the Universe, we should target the habitable planets that will be most favorable to large, globally active biospheres because those are the planets where life will be easiest to detect–and where non-detections will be most meaningful”.
Dr Olson notes that we don’t yet have telescopes which can identify appropriate exoplanets and test this hypothesis, but says that “Ideally this work this will inform telescope design to ensure that future missions, such as the proposed LUVOIR or HabEx telescope concepts, have the right capabilities; now we know what to look for, so we need to start looking”.
Commenting, Professor Chris Reinhard from Georgia Institute of Technology said: “We expect oceans to be important in regulating some of the most compelling remotely detectable signs of life on habitable worlds. Dr. Olson’s work represents a significant and exciting step forward in our understanding of exoplanet oceanography”.
