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Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H

Authors: Alderson, Lili; Wakeford, Hannah R.; Alam, Munazza K.; Batalha, Natasha E.; Lothringer, Joshua D.; Redai, Jea Adams; Barat, Saugata; +85 Authors

Early Release Science of the exoplanet WASP-39b with JWST NIRSpec G395H

Abstract

AbstractMeasuring the abundances of carbon and oxygen in exoplanet atmospheres is considered a crucial avenue for unlocking the formation and evolution of exoplanetary systems1,2. Access to the chemical inventory of an exoplanet requires high-precision observations, often inferred from individual molecular detections with low-resolution space-based3–5 and high-resolution ground-based6–8 facilities. Here we report the medium-resolution (R ≈ 600) transmission spectrum of an exoplanet atmosphere between 3 and 5 μm covering several absorption features for the Saturn-mass exoplanet WASP-39b (ref. 9), obtained with the Near Infrared Spectrograph (NIRSpec) G395H grating of JWST. Our observations achieve 1.46 times photon precision, providing an average transit depth uncertainty of 221 ppm per spectroscopic bin, and present minimal impacts from systematic effects. We detect significant absorption from CO2 (28.5σ) and H2O (21.5σ), and identify SO2 as the source of absorption at 4.1 μm (4.8σ). Best-fit atmospheric models range between 3 and 10 times solar metallicity, with sub-solar to solar C/O ratios. These results, including the detection of SO2, underscore the importance of characterizing the chemistry in exoplanet atmospheres and showcase NIRSpec G395H as an excellent mode for time-series observations over this critical wavelength range10.

Countries
United Kingdom, United Kingdom, Italy, United States, Austria, Belgium, United Kingdom, United Kingdom, United Kingdom, United States, United Kingdom, France, Netherlands, United States
Keywords

550, Extraterrestrial Environment, ISOTOPOLOGUES, [SDU.ASTR.EP]Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], Planets, [SDU.ASTR.EP] Sciences of the Universe [physics]/Astrophysics [astro-ph]/Earth and Planetary Astrophysics [astro-ph.EP], 5109 Space Sciences, [PHYS.PHYS.PHYS-AO-PH] Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph], CHEMISTRY, QB Astronomy, ROTATION-VIBRATION SPECTRUM, 103004 Astrophysics, MOLECULAR LINE LISTS, QC, QB, Earth and Planetary Astrophysics (astro-ph.EP), Multidisciplinary, Exoplanets, article, 3rd-DAS, /639/33/34/862, 103004 Astrophysik, 520, Multidisciplinary Sciences, Saturn, GIANT PLANETS, Astrophysics - Solar and Stellar Astrophysics, 5101 Astronomical Sciences, /639/33/34/2810, Science & Technology - Other Topics, METALLICITY, Astrophysics - Instrumentation and Methods for Astrophysics, 51 Physical Sciences, MODEL ATMOSPHERES, General Science & Technology, SULFUR, FOS: Physical sciences, Settore FIS/05 - ASTRONOMIA E ASTROFISICA, DWARF, Astronomical instrumentation, Article, /140, ABUNDANCES, Instrumentation and Methods for Astrophysics (astro-ph.IM), Solar and Stellar Astrophysics (astro-ph.SR), [PHYS.PHYS.PHYS-AO-PH]Physics [physics]/Physics [physics]/Atmospheric and Oceanic Physics [physics.ao-ph], MCC, Science & Technology, Atmosphere, 500, Oxygen, QC Physics, 627, Astrophysics - Earth and Planetary Astrophysics

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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
239
Top 0.1%
Top 10%
Top 0.1%
Green
hybrid