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 by Staff Writers Heidelberg, Germany (SPX) Nov 23, 2022
Observations of the exoplanet WASP-39b with the James Webb Space Telescope (JWST) have yielded a wealth of information about the planet's atmosphere - a whole new level of observational data, and a harbinger of how JWST will shape the study of exoplanet atmospheres in the future. The detailed infrared spectra taken with three of JWST's four instruments contain information about atmospheric chemistry of unprecedented accuracy, allow deductions about the planet's cloud cover, and include the first signs of photochemistry in exoplanet atmospheres. Data about the chemical composition is so accurate as to allow for deductions about the planet's formation. Information about clouds, first data about photochemistry, and a near-complete chemical inventory that hints at the planet's formation history - those are some highlights from the recently published observations of the exoplanet WASP-39b with the James Webb Telescope (JWST). "Data like these are a game changer," is the verdict of Natalia Batalha (University of California at Santa Cruz), who coordinated the observing program that yielded the new results. The new results, by a group of astronomers that includes MPIA director Laura Kreidberg, also showcase methods that, eventually, should allow astronomers to detect life on distant planets, although that will be a job for one of the successors of JWST.
Putting JWST through its paces But for astronomers planning their own observations, the information contained in those first pictures was of course not nearly enough. For them, JWST started to be put through its paces immediately afterwards, during the first five months of JWST's science operations, in the shape of the "Early Release Science Programs": 13 observational programs covering a representative sample of targets from solar-system objects to the most distant galaxies, chosen specifically so as to give observational astronomers all the information they would need to make optimal use of JWST's instruments themselves later on. Data from those programs is released to the astronomical community directly after the observations are complete. They are complemented by "guide books" and additional analysis aimed at making future observational planning as effective as possible.
All eyes on WASP-39b Crucial for the observations in this case are so-called exoplanet transits. Such a transit happens when from the point-of-view of observers here on Earth, a planet orbiting a distant star passes between that star and us. Exoplanets are typically too far away for us to see in detail how the little dark disk of the planet passes in front of the bright disk of the star. What can be observed are brightness variations. After all, the planet moves in front of the star and, in doing so, blocks some of the starlight. The astronomers made use of JWST to observe four different transits from mid to late July 2022, using three of the space telescope's four science instruments: NIRCam and NIRISS for one transit each, and two transits observed with two different operational modes of NIRSpec, respectively. MPIA has a direct connection to the hardware in use here, as well: as part of a European consortium, the institute supplied the mechanisms of the filter and grating wheels that NIRSpec uses to split the light into the various wavelengths.
Transit spectroscopy This means that the dimming of starlight is now color-dependent, or in terms of the underlying physics: it depends on the wavelength of light at which we observe the system. If the detailed view (which we do not, in reality, have) were to show a dark disk surrounded by a thin blue ring of planetary atmosphere, that means blue light could pass through the atmosphere, but red light could not - hence, when observed through a red filter, the starlight's dimming would be more pronounced than through a blue filter. JWST does not, in studies like the present one, observe the transit through filters, but instead uses spectroscopy to observe the transit in each elementary color, in each wavelength region, separately, with the degree of dimming ("transit depths"). The results are recorded for a broad range of infrared wavelengths.
A wealth of atmospheric information The papers published now add a number of crucial additional pieces of the puzzle. A back-then somewhat mysterious spectral feature in the spectrum turned out to represent sulfur dioxide - once more, the first such detection in an exoplanet atmosphere. This opens up the exciting new field of exoplanet photochemistry: Sulfur dioxide molecules, similar to ozone in Earth's atmosphere, are formed as the upper reaches of the exoplanet's atmosphere interact with high-energy photons from the host star. The fact that WASP-39b is so close to its host star (one eighth the distance from Mercury to our Sun!) makes it an ideal laboratory for exploring these reactions.
Hints of planet formation The comparison of observations and models also yielded information about the planet's cloud cover: a broken-up collection of clouds - not water clouds, though, but clouds made of substances like sulphides and silicates - rather than a single, uniform blanket over the planet.
Helping those who come next MPIA director Laura Kreidberg, who is a member of the Transiting Exoplanet Community Early Release Science Program, emphasizes that this is indeed just the beginning: "These early observations are a harbinger of more amazing science to come with JWST. We put the telescope through its paces to test the performance, and it was nearly flawless - even better than we hoped." The long-term relevance for the search for life on other planets The current observations are also relevant for one of the greatest future goals of observational astronomy: detecting traces of life on exoplanets. As currently envisioned, the discovery of life on an exoplanet would proceed along very similar lines as the research described here: detailed transit observations by some space telescope that is a successor to JWST would be used to extract data about the exoplanet's atmosphere. A comparison with atmospheric models would eventually show that a certain combination of properties - an excess of atmospheric oxygen, say - strongly indicates the presence of specific kinds of living organisms on that planet. The observations described here provide a test run for the observational techniques that will need to be employed in this kind of search for life on other planets. They also add important pieces of information to the more complete understanding of exoplanet atmospheres that is needed for future to be able to distinguish between chemistry in exoplanets with and without the involvement of living organisms.
Research Reports
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