1
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Espinoza N, Steinrueck ME, Kirk J, MacDonald RJ, Savel AB, Arnold K, Kempton EMR, Murphy MM, Carone L, Zamyatina M, Lewis DA, Samra D, Kiefer S, Rauscher E, Christie D, Mayne N, Helling C, Rustamkulov Z, Parmentier V, May EM, Carter AL, Zhang X, López-Morales M, Allen N, Blecic J, Decin L, Mancini L, Molaverdikhani K, Rackham BV, Palle E, Tsai SM, Ahrer EM, Bean JL, Crossfield IJM, Haegele D, Hébrard E, Kreidberg L, Powell D, Schneider AD, Welbanks L, Wheatley P, Brahm R, Crouzet N. Inhomogeneous terminators on the exoplanet WASP-39 b. Nature 2024; 632:1017-1020. [PMID: 39009005 PMCID: PMC11357994 DOI: 10.1038/s41586-024-07768-4] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 09/01/2023] [Accepted: 07/01/2024] [Indexed: 07/17/2024]
Abstract
Transmission spectroscopy has been a workhorse technique used over the past two decades to constrain the physical and chemical properties of exoplanet atmospheres1-5. One of its classical key assumptions is that the portion of the atmosphere it probes-the terminator region-is homogeneous. Several works from the past decade, however, have put this into question for highly irradiated, hot (Teq ≳ 1,000 K) gas giant exoplanets, both empirically6-10 and through three-dimensional modelling11-17. While models have predicted clear differences between the evening (day-to-night) and morning (night-to-day) terminators, direct morning and evening transmission spectra in a wide wavelength range have not been reported for an exoplanet so far. Under the assumption of precise and accurate orbital parameters for the exoplanet WASP-39 b, here we report the detection of inhomogeneous terminators on WASP-39 b, which has allowed us to retrieve its morning and evening transmission spectra in the near-infrared (2-5 μm) using the James Webb Space Telescope. We have observed larger transit depths in the evening, which are, on average, 405 ± 88 ppm larger than the morning ones, and also have qualitatively larger features than the morning spectrum. The spectra are best explained by models in which the evening terminator is hotter than the morning terminator by 17 7 - 57 + 65 K, with both terminators having C/O ratios consistent with solar. General circulation models predict temperature differences broadly consistent with the above value and point towards a cloudy morning terminator and a clearer evening terminator.
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Affiliation(s)
- Néstor Espinoza
- Space Telescope Science Institute, Baltimore, MD, USA.
- Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA.
| | - Maria E Steinrueck
- Max Planck Institute for Astronomy (MPIA), Heidelberg, Germany
- Department of Astronomy & Astrophysics, University of Chicago, Chicago, IL, USA
| | - James Kirk
- Department of Physics, Imperial College London, London, UK
| | - Ryan J MacDonald
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Arjun B Savel
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Kenneth Arnold
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Eliza M-R Kempton
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Matthew M Murphy
- Department of Astronomy and Steward Observatory, University of Arizona, Tucson, AZ, USA
| | - Ludmila Carone
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - Maria Zamyatina
- Department of Physics and Astronomy, Faculty of Environment, Science and Economy, University of Exeter, Exeter, UK
| | - David A Lewis
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
- Institute for Theoretical Physics and Computational Physics, Graz University of Technology, Graz, Austria
| | - Dominic Samra
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - Sven Kiefer
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
- Institute of Astronomy, KU Leuven, Leuven, Belgium
- Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
- Fakultät für Mathematik, Physik und Geodäsie, TU Graz, Graz, Austria
| | - Emily Rauscher
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Duncan Christie
- Max Planck Institute for Astronomy (MPIA), Heidelberg, Germany
| | - Nathan Mayne
- Department of Physics and Astronomy, Faculty of Environment, Science and Economy, University of Exeter, Exeter, UK
| | - Christiane Helling
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
- Institute for Theoretical Physics and Computational Physics, Graz University of Technology, Graz, Austria
| | - Zafar Rustamkulov
- Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - Vivien Parmentier
- Observatoire de la Côte d'Azur, Université Côte d'Azur, CNRS, Nice, France
| | | | - Aarynn L Carter
- Department of Astronomy & Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Xi Zhang
- Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, CA, USA
| | | | - Natalie Allen
- Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - Jasmina Blecic
- Department of Physics, New York University Abu Dhabi, Abu Dhabi, UAE
- Center for Astro, Particle, and Planetary Physics (CAP3), New York University Abu Dhabi, Abu Dhabi, UAE
| | - Leen Decin
- Institute of Astronomy, KU Leuven, Leuven, Belgium
| | - Luigi Mancini
- Max Planck Institute for Astronomy (MPIA), Heidelberg, Germany
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | - Karan Molaverdikhani
- University Observatory Munich, Ludwig Maximilian University, Munich, Germany
- Exzellenzcluster Origins, Garching, Germany
| | - Benjamin V Rackham
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
| | - Shang-Min Tsai
- Department of Earth Sciences, University of California, Riverside, Riverside, CA, USA
| | - Eva-Maria Ahrer
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
| | - Jacob L Bean
- Department of Astronomy & Astrophysics, University of Chicago, Chicago, IL, USA
| | - Ian J M Crossfield
- Department of Physics & Astronomy, University of Kansas, Lawrence, KS, USA
| | - David Haegele
- Max Planck Institute for Astronomy (MPIA), Heidelberg, Germany
| | - Eric Hébrard
- Department of Physics and Astronomy, Faculty of Environment, Science and Economy, University of Exeter, Exeter, UK
| | - Laura Kreidberg
- Max Planck Institute for Astronomy (MPIA), Heidelberg, Germany
| | - Diana Powell
- Department of Astronomy & Astrophysics, University of Chicago, Chicago, IL, USA
| | - Aaron D Schneider
- Institute of Astronomy, KU Leuven, Leuven, Belgium
- Centre for ExoLife Sciences, Niels Bohr Institute, Copenhagen, Denmark
| | - Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Peter Wheatley
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
| | - Rafael Brahm
- Facultad de Ingeniería y Ciencias, Universidad Adolfo Ibáñez, Santiago, Chile
- Millennium Institute for Astrophysics, Santiago, Chile
- Data Observatory Foundation, Santiago, Chile
| | - Nicolas Crouzet
- Leiden Observatory, Leiden University, Leiden, The Netherlands
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2
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Fu G, Welbanks L, Deming D, Inglis J, Zhang M, Lothringer J, Ih J, Moses JI, Schlawin E, Knutson HA, Henry G, Greene T, Sing DK, Savel AB, Kempton EMR, Louie DR, Line M, Nixon M. Hydrogen sulfide and metal-enriched atmosphere for a Jupiter-mass exoplanet. Nature 2024; 632:752-756. [PMID: 38977019 DOI: 10.1038/s41586-024-07760-y] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 10/01/2023] [Accepted: 06/26/2024] [Indexed: 07/10/2024]
Abstract
As the closest transiting hot Jupiter to Earth, HD 189733b has been the benchmark planet for atmospheric characterization1-3. It has also been the anchor point for much of our theoretical understanding of exoplanet atmospheres from composition4, chemistry5,6, aerosols7 to atmospheric dynamics8, escape9 and modelling techniques10,11. Previous studies of HD 189733b have detected carbon and oxygen-bearing molecules H2O and CO (refs. 12,13) in the atmosphere. The presence of CO2 and CH4 has been claimed14,15 but later disputed12,16,17. The inferred metallicity based on these measurements, a key parameter in tracing planet formation locations18, varies from depletion19,20 to enhancement21,22, hindered by limited wavelength coverage and precision of the observations. Here we report detections of H2O (13.4σ), CO2 (11.2σ), CO (5σ) and H2S (4.5σ) in the transmission spectrum (2.4-5.0 μm) of HD 189733b. With an equilibrium temperature of about 1,200 K, H2O, CO and H2S are the main reservoirs for oxygen, carbon and sulfur. Based on the measured abundances of these three main volatile elements, we infer an atmospheric metallicity of three to five times stellar. The upper limit on the methane abundance at 5σ is 0.1 ppm, which indicates a low carbon-to-oxygen ratio (<0.2), suggesting formation through the accretion of water-rich icy planetesimals. The low oxygen-to-sulfur and carbon-to-sulfur ratios also support the planetesimal accretion formation pathway23.
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Affiliation(s)
- Guangwei Fu
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA.
| | - Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Drake Deming
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Julie Inglis
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Michael Zhang
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | | | - Jegug Ih
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | | | | | - Heather A Knutson
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Gregory Henry
- Center of Excellence in Information Systems, Tennessee State University, Nashville, TN, USA
| | | | - David K Sing
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - Arjun B Savel
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Eliza M-R Kempton
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Dana R Louie
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Michael Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Matt Nixon
- Department of Astronomy, University of Maryland, College Park, MD, USA
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3
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Alatoom D, Ibrahim MTI, Furtenbacher T, Császár AG, Alghizzawi M, Yurchenko SN, Azzam AAA, Tennyson J. MARVEL analysis of high-resolution rovibrational spectra of 16O 12C 18O. J Comput Chem 2024. [PMID: 38997238 DOI: 10.1002/jcc.27453] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 12/23/2023] [Revised: 05/30/2024] [Accepted: 06/14/2024] [Indexed: 07/14/2024]
Abstract
Empirical rovibrational energy levels are presented for the third most abundant, asymmetric carbon dioxide isotopologue, 16O12C18O, based on a compiled dataset of experimental rovibrational transitions collected from the literature. The 52 literature sources utilized provide 19,438 measured lines with unique assignments in the wavenumber range of 2-12,676 cm-1. The MARVEL (Measured Active Rotational-Vibrational Energy Levels) protocol, which is built upon the theory of spectroscopic networks, validates the great majority of these transitions and outputs 8786 empirical rovibrational energy levels with an uncertainty estimation based on the experimental uncertainties of the transitions. Issues found in the literature data, such as misassignment of quantum numbers, typographical errors, and misidentifications, are fixed before including them in the final MARVEL dataset and analysis. Comparison of the empirical energy-level data of this study with those in the line lists CDSD-2019 and Ames-2021 shows good overall agreement, significantly better for CDSD-2019; some issues raised by these comparisons are discussed.
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Affiliation(s)
- Dunia Alatoom
- AstroJo Institute, Amman, Jordan
- Department of Physics and Astronomy, University College London, London, UK
- Department of Physics, The University of Jordan, Amman, Jordan
| | - Mohammad Taha I Ibrahim
- AstroJo Institute, Amman, Jordan
- Department of Physics and Astronomy, University College London, London, UK
| | | | - Attila G Császár
- HUN-REN-ELTE Complex Chemical Systems Research Group, Budapest, Hungary
- Institute of Chemistry, Eötvös Loránd University, Budapest, Hungary
| | - M Alghizzawi
- AstroJo Institute, Amman, Jordan
- Department of Physics and Astronomy, University College London, London, UK
| | - Sergei N Yurchenko
- Department of Physics and Astronomy, University College London, London, UK
| | - Ala'a A A Azzam
- AstroJo Institute, Amman, Jordan
- Department of Physics, The University of Jordan, Amman, Jordan
| | - Jonathan Tennyson
- Department of Physics and Astronomy, University College London, London, UK
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4
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Welbanks L, Bell TJ, Beatty TG, Line MR, Ohno K, Fortney JJ, Schlawin E, Greene TP, Rauscher E, McGill P, Murphy M, Parmentier V, Tang Y, Edelman I, Mukherjee S, Wiser LS, Lagage PO, Dyrek A, Arnold KE. A high internal heat flux and large core in a warm Neptune exoplanet. Nature 2024; 630:836-840. [PMID: 38768634 DOI: 10.1038/s41586-024-07514-w] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/15/2024] [Accepted: 05/02/2024] [Indexed: 05/22/2024]
Abstract
Interactions between exoplanetary atmospheres and internal properties have long been proposed to be drivers of the inflation mechanisms of gaseous planets and apparent atmospheric chemical disequilibrium conditions1. However, transmission spectra of exoplanets have been limited in their ability to observationally confirm these theories owing to the limited wavelength coverage of the Hubble Space Telescope (HST) and inferences of single molecules, mostly H2O (ref. 2). In this work, we present the panchromatic transmission spectrum of the approximately 750 K, low-density, Neptune-sized exoplanet WASP-107b using a combination of HST Wide Field Camera 3 (WFC3) and JWST Near-Infrared Camera (NIRCam) and Mid-Infrared Instrument (MIRI). From this spectrum, we detect spectroscopic features resulting from H2O (21σ), CH4 (5σ), CO (7σ), CO2 (29σ), SO2 (9σ) and NH3 (6σ). The presence of these molecules enables constraints on the atmospheric metal enrichment (M/H is 10-18× solar3), vertical mixing strength (log10Kzz = 8.4-9.0 cm2 s-1) and internal temperature (>345 K). The high internal temperature is suggestive of tidally driven inflation4 acting on a Neptune-like internal structure, which can naturally explain the large radius and low density of the planet. These findings suggest that eccentricity-driven tidal heating is a critical process governing atmospheric chemistry and interior-structure inferences for most of the cool (<1,000 K) super-Earth-to-Saturn-mass exoplanet population.
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Affiliation(s)
- Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA.
| | - Taylor J Bell
- Bay Area Environmental Research Institute, NASA's Ames Research Center, Moffett Field, CA, USA
- Space Science and Astrobiology Division, NASA's Ames Research Center, Moffett Field, CA, USA
| | - Thomas G Beatty
- Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA
| | - Michael R Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Kazumasa Ohno
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
- Division of Science, National Astronomical Observatory of Japan (NAOJ), Tokyo, Japan
| | - Jonathan J Fortney
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | | | - Thomas P Greene
- Space Science and Astrobiology Division, NASA's Ames Research Center, Moffett Field, CA, USA
| | - Emily Rauscher
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Peter McGill
- Space Science Institute, Lawrence Livermore National Laboratory, Livermore, CA, USA
| | - Matthew Murphy
- Steward Observatory, University of Arizona, Tucson, AZ, USA
| | - Vivien Parmentier
- Laboratoire Lagrange, Observatoire de la Côte d'Azur, Université Côte d'Azur, Nice, France
| | - Yao Tang
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Isaac Edelman
- Bay Area Environmental Research Institute, NASA's Ames Research Center, Moffett Field, CA, USA
| | - Sagnick Mukherjee
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Lindsey S Wiser
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Pierre-Olivier Lagage
- Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France
| | - Achrène Dyrek
- Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France
| | - Kenneth E Arnold
- Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA
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5
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Powell D, Feinstein AD, Lee EKH, Zhang M, Tsai SM, Taylor J, Kirk J, Bell T, Barstow JK, Gao P, Bean JL, Blecic J, Chubb KL, Crossfield IJM, Jordan S, Kitzmann D, Moran SE, Morello G, Moses JI, Welbanks L, Yang J, Zhang X, Ahrer EM, Bello-Arufe A, Brande J, Casewell SL, Crouzet N, Cubillos PE, Demory BO, Dyrek A, Flagg L, Hu R, Inglis J, Jones KD, Kreidberg L, López-Morales M, Lagage PO, Meier Valdés EA, Miguel Y, Parmentier V, Piette AAA, Rackham BV, Radica M, Redfield S, Stevenson KB, Wakeford HR, Aggarwal K, Alam MK, Batalha NM, Batalha NE, Benneke B, Berta-Thompson ZK, Brady RP, Caceres C, Carter AL, Désert JM, Harrington J, Iro N, Line MR, Lothringer JD, MacDonald RJ, Mancini L, Molaverdikhani K, Mukherjee S, Nixon MC, Oza AV, Palle E, Rustamkulov Z, Sing DK, Steinrueck ME, Venot O, Wheatley PJ, Yurchenko SN. Sulfur dioxide in the mid-infrared transmission spectrum of WASP-39b. Nature 2024; 626:979-983. [PMID: 38232945 PMCID: PMC10901732 DOI: 10.1038/s41586-024-07040-9] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 08/11/2023] [Accepted: 01/05/2024] [Indexed: 01/19/2024]
Abstract
The recent inference of sulfur dioxide (SO2) in the atmosphere of the hot (approximately 1,100 K), Saturn-mass exoplanet WASP-39b from near-infrared JWST observations1-3 suggests that photochemistry is a key process in high-temperature exoplanet atmospheres4. This is because of the low (<1 ppb) abundance of SO2 under thermochemical equilibrium compared with that produced from the photochemistry of H2O and H2S (1-10 ppm)4-9. However, the SO2 inference was made from a single, small molecular feature in the transmission spectrum of WASP-39b at 4.05 μm and, therefore, the detection of other SO2 absorption bands at different wavelengths is needed to better constrain the SO2 abundance. Here we report the detection of SO2 spectral features at 7.7 and 8.5 μm in the 5-12-μm transmission spectrum of WASP-39b measured by the JWST Mid-Infrared Instrument (MIRI) Low Resolution Spectrometer (LRS)10. Our observations suggest an abundance of SO2 of 0.5-25 ppm (1σ range), consistent with previous findings4. As well as SO2, we find broad water-vapour absorption features, as well as an unexplained decrease in the transit depth at wavelengths longer than 10 μm. Fitting the spectrum with a grid of atmospheric forward models, we derive an atmospheric heavy-element content (metallicity) for WASP-39b of approximately 7.1-8.0 times solar and demonstrate that photochemistry shapes the spectra of WASP-39b across a broad wavelength range.
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Affiliation(s)
- Diana Powell
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA.
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA.
| | - Adina D Feinstein
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
- Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, USA
| | - Elspeth K H Lee
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - Michael Zhang
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Shang-Min Tsai
- Department of Earth Sciences, University of California, Riverside, Riverside, CA, USA
| | - Jake Taylor
- Department of Physics, University of Oxford, Oxford, UK
- Institut Trottier de Recherche sur les Exoplanètes, Université de Montréal, Montréal, Quebec, Canada
- Département de Physique, Université de Montréal, Montréal, Quebec, Canada
| | - James Kirk
- Department of Physics, Imperial College London, London, UK
| | - Taylor Bell
- Bay Area Environmental Research Institute, NASA Ames Research Center, Moffett Field, CA, USA
- Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, CA, USA
| | - Joanna K Barstow
- School of Physical Sciences, The Open University, Milton Keynes, UK
| | - Peter Gao
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Jacob L Bean
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Jasmina Blecic
- Department of Physics, New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
- Center for Astro, Particle, and Planetary Physics (CAP3), New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
| | - Katy L Chubb
- Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
| | - Ian J M Crossfield
- Department of Physics & Astronomy, University of Kansas, Lawrence, KS, USA
| | - Sean Jordan
- Institute of Astronomy, University of Cambridge, Cambridge, UK
| | - Daniel Kitzmann
- Laboratory for Atmospheric and Space Physics, University of Colorado Boulder, Boulder, CO, USA
| | - Sarah E Moran
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | - Giuseppe Morello
- Department of Space, Earth and Environment, Chalmers University of Technology, Gothenburg, Sweden
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- INAF - Palermo Astronomical Observatory, Palermo, Italy
| | | | - Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Jeehyun Yang
- Planetary Sciences Section, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Xi Zhang
- Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Eva-Maria Ahrer
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Aaron Bello-Arufe
- Astrophysics Section, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Jonathan Brande
- Department of Physics & Astronomy, University of Kansas, Lawrence, KS, USA
| | - S L Casewell
- School of Physics and Astronomy, University of Leicester, Leicester, UK
| | - Nicolas Crouzet
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
| | - Patricio E Cubillos
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - Brice-Olivier Demory
- Center for Space and Habitability, University of Bern, Bern, Switzerland
- Space and Planetary Sciences, Institute of Physics, University of Bern, Bern, Switzerland
| | - Achrène Dyrek
- Université Paris-Saclay, CEA, CNRS, AIM, Gif-sur-Yvette, France
| | - Laura Flagg
- Department of Astronomy, Cornell University, Ithaca, NY, USA
- Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - Renyu Hu
- Astrophysics Section, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Julie Inglis
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Kathryn D Jones
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | | | | | | | | | - Yamila Miguel
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
- SRON Netherlands Institute for Space Research, Leiden, The Netherlands
| | - Vivien Parmentier
- Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, French Riviera, France
| | - Anjali A A Piette
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Benjamin V Rackham
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Michael Radica
- Institut Trottier de Recherche sur les Exoplanètes, Université de Montréal, Montréal, Quebec, Canada
- Département de Physique, Université de Montréal, Montréal, Quebec, Canada
| | - Seth Redfield
- Astronomy Department, Wesleyan University, Middletown, CT, USA
- Van Vleck Observatory, Wesleyan University, Middletown, CT, USA
| | - Kevin B Stevenson
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA
| | | | | | - Munazza K Alam
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Natalie M Batalha
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | | | - Björn Benneke
- Institut Trottier de Recherche sur les Exoplanètes, Université de Montréal, Montréal, Quebec, Canada
- Département de Physique, Université de Montréal, Montréal, Quebec, Canada
| | - Zach K Berta-Thompson
- Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Boulder, CO, USA
| | - Ryan P Brady
- Department of Physics and Astronomy, University College London, London, UK
| | - Claudio Caceres
- Instituto de Astrofisica, Facultad Ciencias Exactas, Universidad Andres Bello, Santiago, Chile
- Centro de Astrofisica y Tecnologias Afines (CATA), Santiago, Chile
- Núcleo Milenio de Formación Planetaria (NPF), Valparaíso, Chile
| | - Aarynn L Carter
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Jean-Michel Désert
- Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, The Netherlands
| | - Joseph Harrington
- Planetary Sciences Group, Department of Physics and Florida Space Institute, University of Central Florida, Orlando, FL, USA
| | - Nicolas Iro
- Institute of Planetary Research, German Aerospace Center (DLR), Berlin, Germany
| | - Michael R Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | | | - Ryan J MacDonald
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Luigi Mancini
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
- Max Planck Institute for Astronomy, Heidelberg, Germany
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy
| | - Karan Molaverdikhani
- Universitäts-Sternwarte, Ludwig-Maximilians-Universität München, München, Germany
- Exzellenzcluster Origins, Garching, Germany
| | - Sagnick Mukherjee
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Matthew C Nixon
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Apurva V Oza
- Astrophysics Section, Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
| | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
| | - Zafar Rustamkulov
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
| | - David K Sing
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
- Department of Physics and Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | | | - Olivia Venot
- Université de Paris Cité and Université Paris-Est Creteil, CNRS, LISA, Paris, France
| | - Peter J Wheatley
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Sergei N Yurchenko
- Department of Physics and Astronomy, University College London, London, UK
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6
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Bell TJ, Welbanks L, Schlawin E, Line MR, Fortney JJ, Greene TP, Ohno K, Parmentier V, Rauscher E, Beatty TG, Mukherjee S, Wiser LS, Boyer ML, Rieke MJ, Stansberry JA. Methane throughout the atmosphere of the warm exoplanet WASP-80b. Nature 2023; 623:709-712. [PMID: 37993572 DOI: 10.1038/s41586-023-06687-0] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 06/21/2023] [Accepted: 09/27/2023] [Indexed: 11/24/2023]
Abstract
The abundances of main carbon- and oxygen-bearing gases in the atmospheres of giant exoplanets provide insights into atmospheric chemistry and planet formation processes1,2. Thermochemistry suggests that methane (CH4) should be the dominant carbon-bearing species below about 1,000 K over a range of plausible atmospheric compositions3; this is the case for the solar system planets4 and has been confirmed in the atmospheres of brown dwarfs and self-luminous, directly imaged exoplanets5. However, CH4 has not yet been definitively detected with space-based spectroscopy in the atmosphere of a transiting exoplanet6-11, but a few detections have been made with ground-based, high-resolution transit spectroscopy12,13 including a tentative detection for WASP-80b (ref. 14). Here we report transmission and emission spectra spanning 2.4-4.0 μm of the 825 K warm Jupiter WASP-80b taken with the NIRCam instrument of the JWST, both of which show strong evidence of CH4 at greater than 6σ significance. The derived CH4 abundances from both viewing geometries are consistent with each other and with solar to sub-solar C/O and around five times solar metallicity, which is consistent with theoretical predictions15-17.
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Affiliation(s)
- Taylor J Bell
- Bay Area Environmental Research Institute, NASA Ames Research Center, Moffett Field, CA, USA.
- Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, CA, USA.
| | - Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | | | - Michael R Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Jonathan J Fortney
- Department of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA, USA
| | - Thomas P Greene
- Space Science and Astrobiology Division, NASA Ames Research Center, Moffett Field, CA, USA
| | - Kazumasa Ohno
- Department of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA, USA
- Division of Science, National Astronomical Observatory of Japan, Tokyo, Japan
| | - Vivien Parmentier
- Laboratoire Lagrange, Observatoire de la Côte d'Azur, Université Côte d'Azur, Nice, France
| | - Emily Rauscher
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Thomas G Beatty
- Department of Astronomy, University of Wisconsin-Madison, Madison, WI, USA
| | - Sagnick Mukherjee
- Department of Astronomy and Astrophysics, University of California Santa Cruz, Santa Cruz, CA, USA
| | - Lindsey S Wiser
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | | | - Marcia J Rieke
- Steward Observatory, University of Arizona, Tucson, AZ, USA
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7
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Zieba S, Kreidberg L, Ducrot E, Gillon M, Morley C, Schaefer L, Tamburo P, Koll DDB, Lyu X, Acuña L, Agol E, Iyer AR, Hu R, Lincowski AP, Meadows VS, Selsis F, Bolmont E, Mandell AM, Suissa G. No thick carbon dioxide atmosphere on the rocky exoplanet TRAPPIST-1 c. Nature 2023; 620:746-749. [PMID: 37337068 PMCID: PMC10447244 DOI: 10.1038/s41586-023-06232-z] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 03/21/2023] [Accepted: 05/17/2023] [Indexed: 06/21/2023]
Abstract
Seven rocky planets orbit the nearby dwarf star TRAPPIST-1, providing a unique opportunity to search for atmospheres on small planets outside the Solar System1. Thanks to the recent launch of the James Webb Space Telescope (JWST), possible atmospheric constituents such as carbon dioxide (CO2) are now detectable2,3. Recent JWST observations of the innermost planet TRAPPIST-1 b showed that it is most probably a bare rock without any CO2 in its atmosphere4. Here we report the detection of thermal emission from the dayside of TRAPPIST-1 c with the Mid-Infrared Instrument (MIRI) on JWST at 15 µm. We measure a planet-to-star flux ratio of fp/f⁎ = 421 ± 94 parts per million (ppm), which corresponds to an inferred dayside brightness temperature of 380 ± 31 K. This high dayside temperature disfavours a thick, CO2-rich atmosphere on the planet. The data rule out cloud-free O2/CO2 mixtures with surface pressures ranging from 10 bar (with 10 ppm CO2) to 0.1 bar (pure CO2). A Venus-analogue atmosphere with sulfuric acid clouds is also disfavoured at 2.6σ confidence. Thinner atmospheres or bare-rock surfaces are consistent with our measured planet-to-star flux ratio. The absence of a thick, CO2-rich atmosphere on TRAPPIST-1 c suggests a relatively volatile-poor formation history, with less than [Formula: see text] Earth oceans of water. If all planets in the system formed in the same way, this would indicate a limited reservoir of volatiles for the potentially habitable planets in the system.
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Affiliation(s)
- Sebastian Zieba
- Max-Planck-Institut für Astronomie, Heidelberg, Germany.
- Leiden Observatory, Leiden University, Leiden, The Netherlands.
| | | | - Elsa Ducrot
- Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France
| | - Michaël Gillon
- Astrobiology Research Unit, University of Liège, Liège, Belgium
| | - Caroline Morley
- Department of Astronomy, University of Texas at Austin, Austin, TX, USA
| | - Laura Schaefer
- Department of Earth and Planetary Sciences, Stanford University, Stanford, CA, USA
| | - Patrick Tamburo
- Department of Astronomy, Boston University, Boston, MA, USA
- The Institute for Astrophysical Research, Boston University, Boston, MA, USA
| | - Daniel D B Koll
- Department of Atmospheric and Oceanic Sciences, Peking University, Beijing, People's Republic of China
| | - Xintong Lyu
- Department of Atmospheric and Oceanic Sciences, Peking University, Beijing, People's Republic of China
| | - Lorena Acuña
- Max-Planck-Institut für Astronomie, Heidelberg, Germany
- Aix-Marseille Université, CNRS, CNES, Institut Origines, LAM, Marseille, France
| | - Eric Agol
- Astrobiology Program, Department of Astronomy, University of Washington, Seattle, WA, USA
- NASA Nexus for Exoplanet System Science, Virtual Planetary Laboratory Team, University of Washington, Seattle, WA, USA
| | - Aishwarya R Iyer
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Renyu Hu
- Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA, USA
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Andrew P Lincowski
- Astrobiology Program, Department of Astronomy, University of Washington, Seattle, WA, USA
- NASA Nexus for Exoplanet System Science, Virtual Planetary Laboratory Team, University of Washington, Seattle, WA, USA
| | - Victoria S Meadows
- Astrobiology Program, Department of Astronomy, University of Washington, Seattle, WA, USA
- NASA Nexus for Exoplanet System Science, Virtual Planetary Laboratory Team, University of Washington, Seattle, WA, USA
| | - Franck Selsis
- Laboratoire d'Astrophysique de Bordeaux, Université de Bordeaux, CNRS, B18N, Pessac, France
| | - Emeline Bolmont
- Observatoire Astronomique de l'Université de Genève, Versoix, Switzerland
- Centre Vie dans l'Univers, Université de Genève, Geneva, Switzerland
| | - Avi M Mandell
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
- Sellers Exoplanet Environments Collaboration, NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Gabrielle Suissa
- Astrobiology Program, Department of Astronomy, University of Washington, Seattle, WA, USA
- NASA Nexus for Exoplanet System Science, Virtual Planetary Laboratory Team, University of Washington, Seattle, WA, USA
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8
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Coulombe LP, Benneke B, Challener R, Piette AAA, Wiser LS, Mansfield M, MacDonald RJ, Beltz H, Feinstein AD, Radica M, Savel AB, Dos Santos LA, Bean JL, Parmentier V, Wong I, Rauscher E, Komacek TD, Kempton EMR, Tan X, Hammond M, Lewis NT, Line MR, Lee EKH, Shivkumar H, Crossfield IJM, Nixon MC, Rackham BV, Wakeford HR, Welbanks L, Zhang X, Batalha NM, Berta-Thompson ZK, Changeat Q, Désert JM, Espinoza N, Goyal JM, Harrington J, Knutson HA, Kreidberg L, López-Morales M, Shporer A, Sing DK, Stevenson KB, Aggarwal K, Ahrer EM, Alam MK, Bell TJ, Blecic J, Caceres C, Carter AL, Casewell SL, Crouzet N, Cubillos PE, Decin L, Fortney JJ, Gibson NP, Heng K, Henning T, Iro N, Kendrew S, Lagage PO, Leconte J, Lendl M, Lothringer JD, Mancini L, Mikal-Evans T, Molaverdikhani K, Nikolov NK, Ohno K, Palle E, Piaulet C, Redfield S, Roy PA, Tsai SM, Venot O, Wheatley PJ. A broadband thermal emission spectrum of the ultra-hot Jupiter WASP-18b. Nature 2023; 620:292-298. [PMID: 37257843 PMCID: PMC10412449 DOI: 10.1038/s41586-023-06230-1] [Citation(s) in RCA: 1] [Impact Index Per Article: 1.0] [Reference Citation Analysis] [Abstract] [Key Words] [MESH Headings] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/18/2023] [Accepted: 05/16/2023] [Indexed: 06/02/2023]
Abstract
Close-in giant exoplanets with temperatures greater than 2,000 K ('ultra-hot Jupiters') have been the subject of extensive efforts to determine their atmospheric properties using thermal emission measurements from the Hubble Space Telescope (HST) and Spitzer Space Telescope1-3. However, previous studies have yielded inconsistent results because the small sizes of the spectral features and the limited information content of the data resulted in high sensitivity to the varying assumptions made in the treatment of instrument systematics and the atmospheric retrieval analysis3-12. Here we present a dayside thermal emission spectrum of the ultra-hot Jupiter WASP-18b obtained with the NIRISS13 instrument on the JWST. The data span 0.85 to 2.85 μm in wavelength at an average resolving power of 400 and exhibit minimal systematics. The spectrum shows three water emission features (at >6σ confidence) and evidence for optical opacity, possibly attributable to H-, TiO and VO (combined significance of 3.8σ). Models that fit the data require a thermal inversion, molecular dissociation as predicted by chemical equilibrium, a solar heavy-element abundance ('metallicity', [Formula: see text] times solar) and a carbon-to-oxygen (C/O) ratio less than unity. The data also yield a dayside brightness temperature map, which shows a peak in temperature near the substellar point that decreases steeply and symmetrically with longitude towards the terminators.
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Affiliation(s)
- Louis-Philippe Coulombe
- Department of Physics, Université de Montréal, Montréal, Quebec, Canada.
- Trottier Institute for Research on Exoplanets, Université de Montréal, Montréal, Quebec, Canada.
| | - Björn Benneke
- Department of Physics, Université de Montréal, Montréal, Quebec, Canada
- Trottier Institute for Research on Exoplanets, Université de Montréal, Montréal, Quebec, Canada
| | - Ryan Challener
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Anjali A A Piette
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Lindsey S Wiser
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | | | - Ryan J MacDonald
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
- Department of Astronomy, Cornell University, Ithaca, NY, USA
- Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - Hayley Beltz
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | - Adina D Feinstein
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Michael Radica
- Department of Physics, Université de Montréal, Montréal, Quebec, Canada
- Trottier Institute for Research on Exoplanets, Université de Montréal, Montréal, Quebec, Canada
| | - Arjun B Savel
- Department of Astronomy, University of Maryland, College Park, MD, USA
- Center for Computational Astrophysics, Flatiron Institute, New York, NY, USA
| | | | - Jacob L Bean
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Vivien Parmentier
- Université Côte d'Azur, Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Nice, France
| | - Ian Wong
- NASA Goddard Space Flight Center, Greenbelt, MD, USA
| | - Emily Rauscher
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
| | | | - Eliza M-R Kempton
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Xianyu Tan
- Tsung-Dao Lee Institute, Shanghai Jiao Tong University, Shanghai, People's Republic of China
- School of Physics and Astronomy, Shanghai Jiao Tong University, Shanghai, People's Republic of China
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
| | - Mark Hammond
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
| | - Neil T Lewis
- Department of Mathematics and Statistics, Faculty of Environment, Science and Economy, University of Exeter, Exeter, UK
| | - Michael R Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Elspeth K H Lee
- Center for Space and Habitability, University of Bern, Bern, Switzerland
| | - Hinna Shivkumar
- Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, The Netherlands
| | - Ian J M Crossfield
- Department of Physics & Astronomy, University of Kansas, Lawrence, KS, USA
| | - Matthew C Nixon
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Benjamin V Rackham
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | | | - Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Xi Zhang
- Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Natalie M Batalha
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Zachory K Berta-Thompson
- Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Boulder, CO, USA
| | - Quentin Changeat
- European Space Agency, Space Telescope Science Institute, Baltimore, MD, USA
- Department of Physics and Astronomy, University College London, London, UK
| | - Jean-Michel Désert
- Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, The Netherlands
| | | | - Jayesh M Goyal
- School of Earth and Planetary Sciences (SEPS), National Institute of Science Education and Research (NISER), Homi Bhabha National Institute (HBNI), Jatni, India
| | - Joseph Harrington
- Planetary Sciences Group, Department of Physics, University of Central Florida, Orlando, FL, USA
- Florida Space Institute, University of Central Florida, Orlando, FL, USA
| | - Heather A Knutson
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | | | | | - Avi Shporer
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - David K Sing
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
- Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | | | | | - Eva-Maria Ahrer
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Munazza K Alam
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Taylor J Bell
- Bay Area Environmental Research Institute, NASA Ames Research Center, Moffett Field, CA, USA
| | - Jasmina Blecic
- Department of Physics, New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
- Center for Astro, Particle, and Planetary Physics (CAP3), New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
| | - Claudio Caceres
- Instituto de Astrofisica, Universidad Andrés Bello, Santiago, Chile
- Núcleo Milenio de Formación Planetaria (NPF), Valparaíso, Chile
- Centro de Astrofisica y Tecnologias Afines (CATA), Santiago, Chile
| | - Aarynn L Carter
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Sarah L Casewell
- School of Physics and Astronomy, University of Leicester, Leicester, UK
| | - Nicolas Crouzet
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
| | - Patricio E Cubillos
- INAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - Leen Decin
- Institute of Astronomy, Department of Physics and Astronomy, KU Leuven, Leuven, Belgium
| | - Jonathan J Fortney
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Neale P Gibson
- School of Physics, Trinity College Dublin, Dublin, Ireland
| | - Kevin Heng
- Department of Physics, University of Warwick, Coventry, UK
- Universitäts-Sternwarte München, Ludwig-Maximilians-Universität München, München, Germany
- ARTORG Center for Biomedical Engineering Research, University of Bern, Bern, Switzerland
| | | | - Nicolas Iro
- Institute of Planetary Research (PF), German Aerospace Center (DLR), Berlin, Germany
| | - Sarah Kendrew
- European Space Agency, Space Telescope Science Institute, Baltimore, MD, USA
| | - Pierre-Olivier Lagage
- Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France
| | - Jérémy Leconte
- Laboratoire d'Astrophysique de Bordeaux, Université de Bordeaux, Pessac, France
| | - Monika Lendl
- Département d'Astronomie, Université de Genève, Sauverny, Switzerland
| | | | - Luigi Mancini
- Max Planck Institute for Astronomy, Heidelberg, Germany
- INAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy
| | | | - Karan Molaverdikhani
- Max Planck Institute for Astronomy, Heidelberg, Germany
- Universitäts-Sternwarte München, Ludwig-Maximilians-Universität München, München, Germany
- Exzellenzcluster Origins, Garching, Germany
| | | | - Kazumasa Ohno
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
| | - Caroline Piaulet
- Department of Physics, Université de Montréal, Montréal, Quebec, Canada
- Trottier Institute for Research on Exoplanets, Université de Montréal, Montréal, Quebec, Canada
| | - Seth Redfield
- Astronomy Department, Van Vleck Observatory, Wesleyan University, Middletown, CT, USA
| | - Pierre-Alexis Roy
- Department of Physics, Université de Montréal, Montréal, Quebec, Canada
- Trottier Institute for Research on Exoplanets, Université de Montréal, Montréal, Quebec, Canada
| | - Shang-Min Tsai
- Department of Earth and Planetary Sciences, University of California, Riverside, Riverside, CA, USA
| | - Olivia Venot
- Université Paris Cité and Université Paris-Est Creteil, CNRS, LISA, Paris, France
| | - Peter J Wheatley
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
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9
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Hochman A, Komacek TD, De Luca P. Analogous response of temperate terrestrial exoplanets and Earth's climate dynamics to greenhouse gas supplement. Sci Rep 2023; 13:11123. [PMID: 37429911 PMCID: PMC10333385 DOI: 10.1038/s41598-023-38026-8] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 04/05/2023] [Accepted: 06/30/2023] [Indexed: 07/12/2023] Open
Abstract
Humanity is close to characterizing the atmospheres of rocky exoplanets due to the advent of JWST. These astronomical observations motivate us to understand exoplanetary atmospheres to constrain habitability. We study the influence greenhouse gas supplement has on the atmosphere of TRAPPIST-1e, an Earth-like exoplanet, and Earth itself by analyzing ExoCAM and CMIP6 model simulations. We find an analogous relationship between CO2 supplement and amplified warming at non-irradiated regions (night side and polar)-such spatial heterogeneity results in significant global circulation changes. A dynamical systems framework provides additional insight into the vertical dynamics of the atmospheres. Indeed, we demonstrate that adding CO2 increases temporal stability near the surface and decreases stability at low pressures. Although Earth and TRAPPIST-1e take entirely different climate states, they share the relative response between climate dynamics and greenhouse gas supplements.
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Affiliation(s)
- Assaf Hochman
- Fredy and Nadine Hermann Institute of Earth Sciences, The Hebrew University of Jerusalem, Jerusalem, Israel.
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10
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Zhang X. JWST's eyes on an alien world. Innovation (N Y) 2023; 4:100428. [PMID: 37206619 PMCID: PMC10189546 DOI: 10.1016/j.xinn.2023.100428] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/09/2023] [Accepted: 04/18/2023] [Indexed: 05/21/2023] Open
Affiliation(s)
- Xi Zhang
- Department of Earth and Planetary Sciences, University of California Santa Cruz, Santa Cruz, CA 95064, USA
- Corresponding author
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11
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Seidel JV, Nielsen LD, Sarkar S. JWST opens a window on exoplanet skies. Nature 2023; 614:632-633. [PMID: 36792896 DOI: 10.1038/d41586-023-00394-6] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Key Words] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 02/17/2023]
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12
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Feinstein AD, Radica M, Welbanks L, Murray CA, Ohno K, Coulombe LP, Espinoza N, Bean JL, Teske JK, Benneke B, Line MR, Rustamkulov Z, Saba A, Tsiaras A, Barstow JK, Fortney JJ, Gao P, Knutson HA, MacDonald RJ, Mikal-Evans T, Rackham BV, Taylor J, Parmentier V, Batalha NM, Berta-Thompson ZK, Carter AL, Changeat Q, Dos Santos LA, Gibson NP, Goyal JM, Kreidberg L, López-Morales M, Lothringer JD, Miguel Y, Molaverdikhani K, Moran SE, Morello G, Mukherjee S, Sing DK, Stevenson KB, Wakeford HR, Ahrer EM, Alam MK, Alderson L, Allen NH, Batalha NE, Bell TJ, Blecic J, Brande J, Caceres C, Casewell SL, Chubb KL, Crossfield IJM, Crouzet N, Cubillos PE, Decin L, Désert JM, Harrington J, Heng K, Henning T, Iro N, Kempton EMR, Kendrew S, Kirk J, Krick J, Lagage PO, Lendl M, Mancini L, Mansfield M, May EM, Mayne NJ, Nikolov NK, Palle E, Petit Dit de la Roche DJM, Piaulet C, Powell D, Redfield S, Rogers LK, Roman MT, Roy PA, Nixon MC, Schlawin E, Tan X, Tremblin P, Turner JD, Venot O, Waalkes WC, Wheatley PJ, Zhang X. Early Release Science of the exoplanet WASP-39b with JWST NIRISS. Nature 2023; 614:670-675. [PMID: 36623550 PMCID: PMC9946829 DOI: 10.1038/s41586-022-05674-1] [Citation(s) in RCA: 7] [Impact Index Per Article: 7.0] [Reference Citation Analysis] [Abstract] [Grants] [Track Full Text] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 11/02/2022] [Accepted: 12/20/2022] [Indexed: 01/11/2023]
Abstract
The Saturn-mass exoplanet WASP-39b has been the subject of extensive efforts to determine its atmospheric properties using transmission spectroscopy1-4. However, these efforts have been hampered by modelling degeneracies between composition and cloud properties that are caused by limited data quality5-9. Here we present the transmission spectrum of WASP-39b obtained using the Single-Object Slitless Spectroscopy (SOSS) mode of the Near Infrared Imager and Slitless Spectrograph (NIRISS) instrument on the JWST. This spectrum spans 0.6-2.8 μm in wavelength and shows several water-absorption bands, the potassium resonance doublet and signatures of clouds. The precision and broad wavelength coverage of NIRISS/SOSS allows us to break model degeneracies between cloud properties and the atmospheric composition of WASP-39b, favouring a heavy-element enhancement ('metallicity') of about 10-30 times the solar value, a sub-solar carbon-to-oxygen (C/O) ratio and a solar-to-super-solar potassium-to-oxygen (K/O) ratio. The observations are also best explained by wavelength-dependent, non-grey clouds with inhomogeneous coverageof the planet's terminator.
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Affiliation(s)
- Adina D Feinstein
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA.
| | - Michael Radica
- Department of Physics, Université de Montréal, Montreal, Quebec, Canada
- Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Luis Welbanks
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Catriona Anne Murray
- Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Boulder, CO, USA
| | - Kazumasa Ohno
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Louis-Philippe Coulombe
- Department of Physics, Université de Montréal, Montreal, Quebec, Canada
- Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Néstor Espinoza
- Space Telescope Science Institute, Baltimore, MD, USA
- Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA
| | - Jacob L Bean
- Department of Astronomy and Astrophysics, University of Chicago, Chicago, IL, USA
| | - Johanna K Teske
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Björn Benneke
- Department of Physics, Université de Montréal, Montreal, Quebec, Canada
- Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Michael R Line
- School of Earth and Space Exploration, Arizona State University, Tempe, AZ, USA
| | - Zafar Rustamkulov
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
| | - Arianna Saba
- Department of Physics and Astronomy, University College London, London, UK
| | - Angelos Tsiaras
- Department of Physics and Astronomy, University College London, London, UK
- INAF - Osservatorio Astrofisico di Arcetri, Florence, Italy
| | - Joanna K Barstow
- School of Physical Sciences, The Open University, Milton Keynes, UK
| | - Jonathan J Fortney
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Peter Gao
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Heather A Knutson
- Division of Geological and Planetary Sciences, California Institute of Technology, Pasadena, CA, USA
| | - Ryan J MacDonald
- Department of Astronomy, University of Michigan, Ann Arbor, MI, USA
- Department of Astronomy, Cornell University, Ithaca, NY, USA
- Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | | | - Benjamin V Rackham
- Department of Earth, Atmospheric and Planetary Sciences, Massachusetts Institute of Technology, Cambridge, MA, USA
- Kavli Institute for Astrophysics and Space Research, Massachusetts Institute of Technology, Cambridge, MA, USA
| | - Jake Taylor
- Department of Physics, Université de Montréal, Montreal, Quebec, Canada
- Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
| | - Vivien Parmentier
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
- Observatoire de la Côte d'Azur, CNRS, Laboratoire Lagrange, Université Côte d'Azur, Nice, France
| | - Natalie M Batalha
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
- Astrobiology Program, UC Santa Cruz, Santa Cruz, CA, USA
| | - Zachory K Berta-Thompson
- Department of Astrophysical and Planetary Sciences, University of Colorado Boulder, Boulder, CO, USA
| | - Aarynn L Carter
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - Quentin Changeat
- Space Telescope Science Institute, Baltimore, MD, USA
- Department of Physics and Astronomy, University College London, London, UK
- European Space Agency, Space Telescope Science Institute, Baltimore, MD, USA
| | | | - Neale P Gibson
- School of Physics, Trinity College Dublin, Dublin, Ireland
| | - Jayesh M Goyal
- School of Earth and Planetary Sciences (SEPS), National Institute of Science Education and Research (NISER), Homi Bhabha National Institute (HBNI), Jatani, India
| | | | | | | | - Yamila Miguel
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
- SRON Netherlands Institute for Space Research, Leiden, The Netherlands
| | - Karan Molaverdikhani
- Max Planck Institute for Astronomy, Heidelberg, Germany
- Universitäts-Sternwarte, Ludwig-Maximilians-Universität München, Munich, Germany
- Exzellenzcluster Origins, Garching, Germany
| | - Sarah E Moran
- Lunar and Planetary Laboratory, University of Arizona, Tucson, AZ, USA
| | - Giuseppe Morello
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
- Departamento de Astrofísica, Universidad de La Laguna (ULL), Tenerife, Spain
- INAF - Palermo Astronomical Observatory, Palermo, Italy
| | - Sagnick Mukherjee
- Department of Astronomy and Astrophysics, University of California, Santa Cruz, Santa Cruz, CA, USA
| | - David K Sing
- Department of Physics & Astronomy, Johns Hopkins University, Baltimore, MD, USA
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
| | - Kevin B Stevenson
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA
| | | | - Eva-Maria Ahrer
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Munazza K Alam
- Earth and Planets Laboratory, Carnegie Institution for Science, Washington, DC, USA
| | - Lili Alderson
- School of Physics, University of Bristol, Bristol, UK
| | - Natalie H Allen
- Department of Earth and Planetary Sciences, Johns Hopkins University, Baltimore, MD, USA
| | | | - Taylor J Bell
- Bay Area Environmental Research Institute, NASA Ames Research Center, Moffett Field, CA, USA
| | - Jasmina Blecic
- Department of Physics, New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
- Center for Astro, Particle, and Planetary Physics (CAP3), New York University Abu Dhabi, Abu Dhabi, United Arab Emirates
| | - Jonathan Brande
- Department of Physics & Astronomy, University of Kansas, Lawrence, KS, USA
| | - Claudio Caceres
- Instituto de Astrofísica, Universidad Andrés Bello, Santiago, Chile
- Núcleo Milenio de Formación Planetaria (NPF), Valparaíso, Chile
- Centro de Astrofísica y Tecnologías Afines (CATA), Santiago, Chile
| | - S L Casewell
- School of Physics and Astronomy, University of Leicester, Leicester, UK
| | - Katy L Chubb
- Centre for Exoplanet Science, University of St Andrews, St Andrews, UK
| | - Ian J M Crossfield
- Department of Physics & Astronomy, University of Kansas, Lawrence, KS, USA
| | - Nicolas Crouzet
- Leiden Observatory, University of Leiden, Leiden, The Netherlands
| | - Patricio E Cubillos
- INAF - Osservatorio Astrofisico di Torino, Pino Torinese, Italy
- Space Research Institute, Austrian Academy of Sciences, Graz, Austria
| | - Leen Decin
- Institute of Astronomy, Department of Physics and Astronomy, KU Leuven, Leuven, Belgium
| | - Jean-Michel Désert
- Anton Pannekoek Institute for Astronomy, University of Amsterdam, Amsterdam, The Netherlands
| | - Joseph Harrington
- Planetary Sciences Group, Department of Physics, University of Central Florida, Orlando, FL, USA
- Florida Space Institute, University of Central Florida, Orlando, FL, USA
| | - Kevin Heng
- Universitäts-Sternwarte, Ludwig-Maximilians-Universität München, Munich, Germany
- Department of Physics, University of Warwick, Coventry, UK
- ARTORG Center for Biomedical Engineering Research, University of Bern, Bern, Switzerland
| | | | - Nicolas Iro
- Institute for Astrophysics, University of Vienna, Vienna, Austria
| | - Eliza M-R Kempton
- Department of Astronomy, University of Maryland, College Park, MD, USA
| | - Sarah Kendrew
- European Space Agency, Space Telescope Science Institute, Baltimore, MD, USA
| | - James Kirk
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
- Department of Physics, Imperial College London, London, UK
| | - Jessica Krick
- Infrared Processing and Analysis Center (IPAC), California Institute of Technology, Pasadena, CA, USA
| | - Pierre-Olivier Lagage
- Université Paris-Saclay, Université Paris Cité, CEA, CNRS, AIM, Gif-sur-Yvette, France
| | - Monika Lendl
- Département d'Astronomie, Université de Genève Sauverny, Versoix, Switzerland
| | - Luigi Mancini
- Max Planck Institute for Astronomy, Heidelberg, Germany
- Department of Physics, University of Rome "Tor Vergata", Rome, Italy
- INAF - Turin Astrophysical Observatory, Pino Torinese, Italy
| | | | - E M May
- Johns Hopkins University Applied Physics Laboratory, Laurel, MD, USA
| | - N J Mayne
- Department of Physics and Astronomy, Faculty of Environment, Science and Economy, University of Exeter, Exeter, UK
| | | | - Enric Palle
- Instituto de Astrofísica de Canarias (IAC), Tenerife, Spain
| | | | - Caroline Piaulet
- Department of Physics, Université de Montréal, Montreal, Quebec, Canada
- Institute for Research on Exoplanets, Université de Montréal, Montreal, Quebec, Canada
| | - Diana Powell
- Center for Astrophysics | Harvard & Smithsonian, Cambridge, MA, USA
| | - Seth Redfield
- Astronomy Department, Wesleyan University, Middletown, CT, USA
- Van Vleck Observatory, Wesleyan University, Middletown, CT, USA
| | - Laura K Rogers
- Institute of Astronomy, University of Cambridge, Cambridge, UK
| | - Michael T Roman
- School of Physics and Astronomy, University of Leicester, Leicester, UK
- Universidad Adolfo Ibáñez, Campus Peñalolén, Santiago, Chile
| | - Pierre-Alexis Roy
- Department of Physics, Université de Montréal, Montreal, Quebec, Canada
| | - Matthew C Nixon
- Department of Astronomy, University of Maryland, College Park, MD, USA
- Institute of Astronomy, University of Cambridge, Cambridge, UK
| | | | - Xianyu Tan
- Atmospheric, Oceanic and Planetary Physics, Department of Physics, University of Oxford, Oxford, UK
| | - P Tremblin
- Maison de la Simulation, CEA, CNRS, Université Paris-Sud, Université Versailles St Quentin, Université Paris-Saclay, Gif-sur-Yvette, France
| | - Jake D Turner
- Department of Astronomy, Cornell University, Ithaca, NY, USA
- Carl Sagan Institute, Cornell University, Ithaca, NY, USA
| | - Olivia Venot
- Université de Paris Cité and Université Paris-Est Creteil, CNRS, LISA, Paris, France
| | - William C Waalkes
- Astrophysics & Planetary Sciences, University of Colorado Boulder, Boulder, CO, USA
| | - Peter J Wheatley
- Centre for Exoplanets and Habitability, University of Warwick, Coventry, UK
- Department of Physics, University of Warwick, Coventry, UK
| | - Xi Zhang
- Department of Earth and Planetary Sciences, University of California, Santa Cruz, Santa Cruz, CA, USA
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