Tag: deep-sea hydrothermal vents

New Evidence for Methane a Sign of Extraterrestrial Life

Article by Sarah Kahle                                       February 10, 2021                                       (dailyuw.com)

• Scientists know that methane is produced two ways: first by living biological microbes converting carbon monoxide into methane, and second by volcanos and deep sea hydrothermal vents. A biologically active exoplanet – the kind that astronomers search star systems for – could be detected by its abundance of methane.

• The James Webb Space Telescope (pictured above) is set to launch October 2021, and will replace the aging Hubble telescope in space. The Webb telescope is particularly adept at detecting atmospheric methane on distant exoplanets.

• A team led by UW postdoctoral student Nick Wogan set out to determine whether volcanic gas emissions on terrestrial exoplanets were abundant enough to disguise any biologically produced methane, and why an abundance of methane might be a potential indication of life. “We wanted to understand whether if we look at another planet, if we see methane there, is that because of life, or is that because of some weird volcano that also produces methane?” Wogan said. The team ran many combinations of simulations that modeled a wide range of volcanic chemistries possible for a terrestrial planet.

• The researchers found that while volcanic activity did produce methane, they weren’t capable of producing abundances anywhere near the level of biogenic methane. Further, if an abundance of methane in an atmosphere did come from volcanic activity, it would be indicated by an abundance of carbon monoxide as well, which the telescopes can detect.

• Therefore, the detection of proportionately large amount of methane in an exoplanet’s atmosphere might indeed be an indication that Earth-like organisms exist there. Large amounts of oxygen-rich gases, such as carbon dioxide and water vapor, alongside the methane would strengthen the possibility of a life-supporting biosignature. Says Wogan, “Really, our best shot of finding evidence of life on another planet is probably seeing the combination of methane and carbon dioxide.”

• Another indication of methane-producing bacteria or other similar lifeforms would be a proportionately low level of carbon monoxide which is consumed and converted by bacteria.

• The research group’s findings will be particularly helpful to astronomers analyzing exoplanetary atmospheres with the James Webb Space Telescope, and may be instrumental in finding extraterrestrial methane biosignatures.

 

                 Nick Wogan

A team led by UW postdoctoral student Nick Wogan has published a paper explaining why an abundance of methane in the atmosphere of an exoplanet (any planet orbiting a star other than the Sun) might be a potential indication of life.

Scientists typically search for molecular oxygen as an indication of life (or of conditions favorable to life) on other planets, but unfortunately, the James Webb Space Telescope, set to launch October 2021, isn’t well equipped to detect it in the atmospheres of faraway planets. The new telescope, however, intended to replace the aging Hubble, is particularly adept at detecting atmospheric methane and carbon dioxide abundances.

During the Archean, an eon early in Earth’s history, the first microbes developed and began to convert carbon monoxide into methane. This process continues today. As a result, methane began to build up in the atmosphere and has remained as an indication of biologic activity on Earth ever since.

However, life is not the only process we know of that can produce methane. Volcanism, deep sea hydrothermal vents, and meteor impacts can all generate methane as well. Wogan set out to determine whether volcanic gas emissions on terrestrial exoplanets were abundant enough to disguise any biologically produced methane.

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Ariel’s Search For Extraterrestrial Life

Article by Giovanni Mussini                                 November 30, 2020                                      (oxfordstudent.com)

• The European Ariel space telescope (Atmospheric Remote-sensing Infrared Exoplanet Large-survey) has been given the go-ahead for launch in 2029. Intended to map the atmospheres and chemical environments of distant exoplanets, the Ariel spacecraft’s search range will target hundreds of planets in the hotter Goldilocks zones in order to build a standard model of atmospheres based on the attributes of its host star and planetary environments.

• Different atmospheric components imprint distinctive patterns on the starlight beaming through. While not conducive to life itself, planets having an “atmospheric cauldron” that can circulate freely allows Ariel to capture more representative spectral signatures to create a standard model.

• The presence of unique ‘biosignatures’ arise due to the unique self-organizing properties of life. But at the same time, anomalies are unlikely to be spectacular or self-evident. Take Venus for example. Venus is a planetary inferno bathed in sulphuric acid rains, with a mean surface temperature high enough to melt lead. The biosignature of phosphine – a chemical created by living organisms – was detected in the cooler high-altitude Venusian clouds. But it is uncertain whether the presence of phosphine is due to biological activity, exotic abiotic chemistries, or a blip in the data.

• Time and again, attempts to map molecular pathways to life from simple organics have failed. Promising places – such as deep-sea hydrothermal vents – have proven an unlikely starting point for biology. The necessary interdependence of proteins, membranes, and nucleic acids may require simultaneous assembly, rather than in a stepwise fashion. Across the cosmos, the least unlikely places for spontaneous life to occur might be mineral-rich ephemeral pools bombarded by UV radiation. This is bad news for life. Temperate gas giants, oceanic super-Earths, and promising icy moons would all be ruled out. Perhaps biology really needs a planet like ours to get started: rocky, temperate, and tectonically active, with emerging landmasses. Places like these probably do exist, dotting the spiral arms of our galaxy.

• If the history of the Earth is any guide, evolution may rise to the challenges of alien worlds where there is living material to work from in the first place. Even on Venus, where balmy oceans existed as recently as 700 million years ago, life may have escaped the planet’s descent into a greenhouse nightmare by migrating to the higher atmosphere. As robotic emissaries and telescopic eyes return troves of data on far-flung worlds, sensational discoveries may come. But we are probably in for a long wait.

 

After years in the pipeline, the Ariel space telescope has been given the go-ahead for launch in 2029. This spacecraft is the brainchild of a cooperative European endeavour to map the atmospheres and chemical environments of far-flung worlds. If all goes well, Ariel will bring planetary science out of the solar system, and into uncharted territory. However, alien hunters may have to keep their enthusiasm in check – for now.

Ariel will peer at a range of exoplanets, but its focus will be on worlds baked by their home stars at over 320 ºC. By all measures, these are extremely unlikely abodes for life. Even so, the detection technique available to Ariel makes them attractive targets.

The telescope will search for faint chemical fingerprints as planets transit in front of their star. By only soaking up particular wavelengths, different atmospheric components imprint distinctive patterns on the starlight beaming through. The closer a planet is to its star, the more frequent the transits and the opportunities to carry out observations. Another perk of closely orbiting hellish worlds is that they wear their atmospheric makeup on their sleeve. Whereas gases may sink or coalesce into clouds on cooler planets, in an atmospheric cauldron they can circulate freely, allowing Ariel to capture more representative spectral signatures.

Ariel’s predecessors had to split their focus between probing exoplanetary atmospheres and other tasks. Instead, the ESA spacecraft will be solely dedicated to this endeavour, broadening the search to an unprecedented number of targets – hundreds of them. This is a cause for excitement. By gathering data en masse, Ariel will build towards something that has been sorely lacking in the quest for living worlds: a standard model of how atmospheres arise based on their host star and planetary environments. Understanding what is in line with this model, and what is not, may help scientists home in on genuine anomalies.

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