Article
Geosciences, Multidisciplinary
Lorenz Roth
Summary: Previous studies have shown the presence of molecular oxygen in Europa's atmosphere, with a new analysis revealing a stable water vapor atmosphere in addition to oxygen, predominantly in the trailing hemisphere. These findings were based on observations from the Hubble Space Telescope taken in various years, indicating a consistent pattern of emissions and abundance ratios over time.
GEOPHYSICAL RESEARCH LETTERS
(2021)
Review
Environmental Sciences
Imke de Pater, Edward M. Molter, Chris M. Moeckel
Summary: Radio observations of the giant planets in the solar system have been crucial in understanding their atmospheres, dynamics, and planet formation theories. Recent studies have revealed global circulation patterns, composition data supporting different planet formation scenarios, and constraints on models of outer proto-planetary disk and ice giant accretion. The importance of radio observations for planetary research will continue in the coming decades, particularly with the advancements in proposed and under-construction radio telescopes.
Article
Astronomy & Astrophysics
Sagnick Mukherjee, Natasha E. Batalha, Mark S. Marley
Summary: Future space-based direct imaging missions will perform low-resolution optical spectroscopy of cool giants, providing rich information about the scattering and absorbing properties of planet atmospheres. The retrieval of atmospheric and scattering properties heavily depends on the choice of cloud parameterizations.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Munazza K. Alam, Mercedes Lopez-Morales, Ryan J. MacDonald, Nikolay Nikolov, James Kirk, Jayesh M. Goyal, David K. Sing, Hannah R. Wakeford, Alexander D. Rathcke, Drake L. Deming, Jorge Sanz-Forcada, Nikole K. Lewis, Joanna K. Barstow, Thomas Mikal-Evans, Lars A. Buchhave
Summary: Exoplanets with cloud-free, haze-free atmospheres are important for detailed atmospheric characterization and precise chemical abundance constraints. The study presents the first transmission spectrum of WASP-62b, showing Na i and SiH spectral features. Using simulated observations, it is demonstrated that the James Webb Space Telescope can conclusively detect various molecules in the atmosphere of WASP-62b, making it a benchmark giant exoplanet for atmospheric characterization.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Geosciences, Multidisciplinary
Ilai Guendelman, Yohai Kaspi
Summary: This study examines the factors influencing the seasonal cycle of a planet by using a general circulation model and an energy balance model, finding that in addition to obliquity and orbital period, the rotation rate also plays a nontrivial role in determining seasonality.
Article
Geochemistry & Geophysics
P. Scarica, D. Grassi, A. Mura, A. Adriani, A. Ingersoll, C. Li, G. Piccioni, G. Sindoni, M. L. Moriconi, C. Plainaki, F. Altieri, A. Cicchetti, B. M. Dinelli, G. Filacchione, A. Migliorini, R. Noschese, R. Sordini, S. Stefani, F. Tosi, D. Turrini
Summary: The Jovian InfraRed Auroral Mapper (JIRAM) onboard the NASA Juno mission has monitored the evolution of Jupiter's polar cyclones since February 2017. The data acquired by JIRAM reveal complex and stable geometrical patterns of cloudy cyclones at both poles. This study presents vorticity maps deduced from wind fields for the region poleward of approximately -80 degrees, and confirms the general stability of both the cyclones and the whole system, while also noting variations in vortex shape and local structures.
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
(2022)
Article
Astronomy & Astrophysics
Michael T. Roman, Eliza M. -R. Kempton, Emily Rauscher, Caleb K. Harada, Jacob L. Bean, Kevin B. Stevenson
Summary: By using a general circulation model, trends in simulated hot Jupiter atmospheres were investigated for different irradiation temperatures, surface gravities, and cloud conditions. The study found that clouds significantly modify the radiative transport and affect the observable properties of planets. Clouds lead to larger phase-curve amplitudes and smaller phase-curve offsets at IR wavelengths compared to cloud-free models.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Shuang Wang, Jun Yang
Summary: Recent studies have shown that atmospheric superrotation can alter the phase of planetary waves, with a nonlinear relationship between the strength of the mean flow and phase shift. Resonance mechanisms are found to be similar to those observed on Earth and hot Jupiters, providing insights into wave-mean-flow interactions on tidally locked planets.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Kevin Heng, Liming Li
Summary: This study fits model atmospheres of Jupiter within a Bayesian framework, finding that using the double Henyey-Greenstein reflection law provides better fits to the data. The aerosols in the Jovian atmosphere are inferred to be large, irregular, polydisperse particles with strong forward scattering and a narrow backscattering lobe. The near-unity values of single-scattering albedos suggest multiple scattering of radiation is an important effect.
ASTROPHYSICAL JOURNAL LETTERS
(2021)
Article
Multidisciplinary Sciences
Maggie A. Thompson, Joshua Krissansen-Totton, Nicholas Wogan, Myriam Telus, Jonathan J. Fortney
Summary: Methane has been proposed as a potential biosignature for exoplanets, but it is important to consider the specific planetary conditions. Methane has a short lifetime in terrestrial planet atmospheres and requires large replenishment fluxes. While methane can be produced abiotically, known abiotic processes cannot easily generate atmospheres rich in methane and carbon dioxide with limited carbon monoxide. Therefore, planets with certain conditions are more likely to have biogenic methane.
PROCEEDINGS OF THE NATIONAL ACADEMY OF SCIENCES OF THE UNITED STATES OF AMERICA
(2022)
Article
Meteorology & Atmospheric Sciences
Baosheng Li, Lei Zhou, Tao Lian, Ting Liu, Jianhuang Qin, Yan Du, Dake Chen
Summary: The role of the intraseasonal sea surface temperature (SST) gradient in the northward-propagating monsoon intraseasonal oscillation (MISO) is examined. It is found that the positive meridional SST gradient induces positive wind convergence and leads to convection. This study highlights the importance of the SST meridional gradient in the feedback to MISO.
JOURNAL OF CLIMATE
(2023)
Article
Meteorology & Atmospheric Sciences
Timothy W. Cronin, Ishir Dutta
Summary: Understanding the radiative response to warming is crucial for predicting global warming. The difference between the radiative response estimated by climate models and the theoretical estimate is mainly due to the lack of stratospheric warming in the models. Neglecting this warming can lead to an overly optimistic analysis of climate change feedbacks.
JOURNAL OF ADVANCES IN MODELING EARTH SYSTEMS
(2023)
Review
Environmental Sciences
Csaba Palotai, Shawn Brueshaber, Ramanakumar Sankar, Kunio Sayanagi
Summary: The atmospheres of the outer planets in our Solar System exhibit a wide array of intriguing cloud features, varying in color and size. The distinct differences in cloud types observed suggest a complex interplay between the dynamics and chemistry at play in these atmospheres. The contrasting banded structures of Jupiter and Saturn compared to the sporadic clouds on the ice giants highlight the diverse dynamic, chemical, and thermal processes shaping these atmospheres. This review presents evidence of moist convective activity in the gas giant atmospheres of our Solar System through remote sensing data from both ground- and space-based observations. The processes driving moist convective activity, including dynamics and microphysics shaping the resulting clouds, are discussed, as well as the effects of moist convection on large-scale dynamics such as jet structures on these planets.
Article
Geochemistry & Geophysics
Thaddeus D. Komacek, Wanying Kang, Jacob Lustig-Yaeger, Stephanie L. Olson
Summary: Numerical climate models originally developed for Earth have been used to study exoplanetary climates, allowing investigation into the range of factors that may affect an exoplanet's climate. The recent discovery of rocky exoplanets close to Earth and upcoming characterization provide insight into the processes shaping planetary climates and Earth's own habitability. Recent advances in understanding the climate of rocky exoplanets and upcoming astronomical observations will help constrain and interpret future climate studies.
Article
Astronomy & Astrophysics
D. Lemasquerier, B. Favier, M. Le Bars
Summary: This study presents experimental results from a laboratory analog of zonal jets in deep gas giants. The researchers found that turbulent zonal jets can spontaneously emerge and reach equilibrium in the experiments, with up to 70% of the total kinetic energy of the flow. They also validated the zonostrophic theory in a fully three-dimensional framework. Additionally, they quantified the mixing of potential vorticity in the flow and showed that it can be estimated using the Thorpe scale.
Article
Astronomy & Astrophysics
Julianne Moses, Zarah L. Brown, Tommi T. Koskinen, Leigh N. Fletcher, Joseph Serigano, Sandrine Guerlet, Luke Moore, J. Hunter Waite, Lotfi Ben-Jaffel, Marina Galand, Joshua M. Chadney, Sarah M. Horst, James A. Sinclair, Veronique Vuitton, Ingo Muller-Wodarg
Summary: During the Grand Finale stage of the Cassini mission, researchers discovered the flow of organic-rich ring material into Saturn's equatorial upper atmosphere. Through photochemical models, they studied the impact of this material on the composition of Saturn's atmosphere. However, observations did not confirm the predicted chemical consequences, leading to the conclusion that the ring influx may have been a transient event triggered by a recent dynamical event or that the material entered the atmosphere in the form of small dust particles.
Article
Astronomy & Astrophysics
Francesca E. DeMeo, Michael Marsset, David Polishook, Brian J. Burt, Richard P. Binzel, Sunao Hasegawa, Mikael Granvik, Nicholas A. Moskovitz, Alissa Earle, Schelte J. Bus, Cristina A. Thomas, Andrew S. Rivkin, Stephen M. Slivan
Summary: Evidence shows that there are young, fresh surfaces among Near-Earth and Main-Belt asteroids, even though space weathering timescales are shorter than the age of the surfaces. Multiple mechanisms including planetary encounters, YORP spinup, thermal degradation, and collisions may play a role in refreshing asteroid surfaces on short timescales. Grain size effects have also been proposed to explain the existence of fresh-looking spectra. The Q/S ratio, which represents the fresh or weathered state, shows several trends including size dependence, dependence on perihelion distance, a sharp peak near 5 degrees orbital inclination, and a higher ratio for objects that have the possibility of encounter with Earth and Venus.
Article
Astronomy & Astrophysics
James S. D. Blake, L. N. Fletcher, G. S. Orton, A. Antunano, M. T. Roman, Y. Kasaba, T. Fujiyoshi, H. Melin, D. Bardet, J. A. Sinclair, M. Es-Sayeh
Summary: Ground-based mid-infrared images of Saturn over a multi-decade period reveal seasonal and non-seasonal variability in thermal emission. 8-m class observatories can resolve thermal contrasts on various scales and confirm the consistency of Saturn's thermal structure from year to year. However, inter-annual variations are observed in the equatorial banding, suggesting the influence of tropospheric meteorology.
Article
Multidisciplinary Sciences
Cristina A. Thomas, Shantanu P. Naidu, Peter Scheirich, Nicholas A. Moskovitz, Petr Pravec, Steven R. Chesley, Andrew S. Rivkin, David J. Osip, Tim A. Lister, Lance A. M. Benner, Marina Brozovic, Carlos Contreras, Nidia Morrell, Agata Rozek, Peter Kusnirak, Kamil Hornoch, Declan Mages, Patrick A. Taylor, Andrew D. Seymour, Colin Snodgrass, Uffe G. Jorgensen, Martin Dominik, Brian Skiff, Tom Polakis, Matthew M. Knight, Tony L. Farnham, Jon D. Giorgini, Brian Rush, Julie Bellerose, Pedro Salas, William P. Armentrout, Galen Watts, Michael W. Busch, Joseph Chatelain, Edward Gomez, Sarah Greenstreet, Liz Phillips, Mariangela Bonavita, Martin J. Burgdorf, Elahe Khalouei, Penelope Longa-Pena, Markus Rabus, Sedighe Sajadian, Nancy L. Chabot, Andrew F. Cheng, William H. Ryan, Eileen V. Ryan, Carrie E. Holt, Harrison F. Agrusa
Summary: The DART spacecraft successfully tested a kinetic impactor by colliding with the asteroid Dimorphos and changing its orbital period. The change in orbit suggests that ejecta contributed momentum to the asteroid beyond what the spacecraft carried.
Article
Multidisciplinary Sciences
R. Terik Daly, Carolyn M. Ernst, Olivier S. Barnouin, Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Elena Y. Adams, Harrison F. Agrusa, Elisabeth D. Abel, Amy L. Alford, Erik I. Asphaug, Justin A. Atchison, Andrew R. Badger, Paul Baki, Ronald-L. Ballouz, Dmitriy L. Bekker, Julie Bellerose, Shyam Bhaskaran, Bonnie J. Buratti, Saverio Cambioni, Michelle H. Chen, Steven R. Chesley, George Chiu, Gareth S. Collins, Matthew W. Cox, Mallory E. DeCoster, Peter S. Ericksen, Raymond C. Espiritu, Alan S. Faber, Tony L. Farnham, Fabio Ferrari, Zachary J. Fletcher, Robert W. Gaskell, Dawn M. Graninger, Musad A. Haque, Patricia A. Harrington-Duff, Sarah Hefter, Isabel Herreros, Masatoshi Hirabayashi, Philip M. Huang, Syau-Yun W. Hsieh, Seth A. Jacobson, Stephen N. Jenkins, Mark A. Jensenius, Jeremy W. John, Martin Jutzi, Tomas Kohout, Timothy O. Krueger, Frank E. Laipert, Norberto R. Lopez, Robert Luther, Alice Lucchetti, Declan M. Mages, Simone Marchi, Anna C. Martin, Maria E. McQuaide, Patrick Michel, Nicholas A. Moskovitz, Ian W. Murphy, Naomi Murdoch, Shantanu P. Naidu, Hari Nair, Michael C. Nolan, Jens Ormoe, Maurizio Pajola, Eric E. Palmer, James M. Peachey, Petr Pravec, Sabina D. Raducan, K. T. Ramesh, Joshua R. Ramirez, Edward L. Reynolds, Joshua E. Richman, Colas Q. Robin, Luis M. Rodriguez, Lew M. Roufberg, Brian P. Rush, Carolyn A. Sawyer, Daniel J. Scheeres, Petr Scheirich, Stephen R. Schwartz, Matthew P. Shannon, Brett N. Shapiro, Caitlin E. Shearer, Evan J. Smith, R. Joshua Steele, Jordan K. Steckloff, Angela M. Stickle, Jessica M. Sunshine, Emil A. Superfin, Zahi B. Tarzi, Cristina A. Thomas, Justin R. Thomas, Josep M. Trigo-Rodriguez, B. Teresa Tropf, Andrew T. Vaughan, Dianna Velez, C. Dany Waller, Daniel S. Wilson, Kristin A. Wortman, Yun Zhang
Summary: Although no known asteroid poses a threat to Earth for at least the next century, the current catalogue of near-Earth asteroids is not comprehensive enough to include those that could cause regional devastation. Various methods, such as kinetic impact, have been proposed to prevent asteroid impacts on Earth. NASA's DART mission successfully demonstrated the viability of kinetic impactor technology through its autonomous collision with the asteroid Dimorphos.
Review
Astronomy & Astrophysics
Leigh N. Fletcher, Thibault Cavalie, Davide Grassi, Ricardo Hueso, Luisa M. Lara, Yohai Kaspi, Eli Galanti, Thomas K. Greathouse, Philippa M. Molyneux, Marina Galand, Claire Vallat, Olivier Witasse, Rosario Lorente, Paul Hartogh, Francois Poulet, Yves Langevin, Pasquale Palumbo, G. Randall Gladstone, Kurt D. Retherford, Michele K. Dougherty, Jan-Erik Wahlund, Stas Barabash, Luciano Iess, Lorenzo Bruzzone, Hauke Hussmann, Leonid I. Gurvits, Ondrej Santolik, Ivana Kolmasova, Georg Fischer, Ingo Mueller-Wodarg, Giuseppe Piccioni, Thierry Fouchet, Jean-Claude Gerard, Agustin Sanchez-Lavega, Patrick G. J. Irwin, Denis Grodent, Francesca Altieri, Alessandro Mura, Pierre Drossart, Josh Kammer, Rohini Giles, Stephanie Cazaux, Geraint Jones, Maria Smirnova, Emmanuel Lellouch, Alexander S. Medvedev, Raphael Moreno, Ladislav Rezac, Athena Coustenis, Marc Costa
Summary: ESA's Jupiter Icy Moons Explorer (JUICE) will conduct a detailed investigation of the Jovian system in the 2030s, utilizing state-of-the-art instruments and a tailored orbital tour. The mission aims to gather information on the climate, meteorology, and chemistry of Jupiter's atmosphere and auroras, as well as studying phenomena on various timescales. The remote sensing payload includes spectroscopy, imaging, and sounding techniques, allowing for a comprehensive characterization of the planet's atmosphere and auroras.
SPACE SCIENCE REVIEWS
(2023)
Article
Multidisciplinary Sciences
Samantha K. K. Trumbo, Michael E. E. Brown, Dominique Bockelee-Morvan, Imke de Pater, Thierry Fouchet, Michael H. H. Wong, Stephanie Cazaux, Leigh N. Fletcher, Katherine de Kleer, Emmanuel Lellouch, Alessandro Mura, Olivier Poch, Eric Quirico, Pablo Rodriguez-Ovalle, Mark R. R. Showalter, Matthew S. S. Tiscareno, Federico Tosi
Summary: Ganymede, the only satellite with an intrinsic magnetic field, experiences interactions with the Jovian magnetosphere, resulting in the accumulation of charged particles in its polar regions. Observations with JWST have revealed the presence of hydrogen peroxide, a product of radiolysis, at high latitudes, indicating the modification of polar caps by precipitation of Jovian charged particles along partially open field lines within Ganymede's magnetosphere. This discovery, along with the contrasting distribution of hydrogen peroxide on Europa, has important implications for understanding water-ice radiolysis in the solar system.
Article
Astronomy & Astrophysics
Brandon Park Coy, Conor A. Nixon, Naomi Rowe-Gurney, Richard Achterberg, Nicholas A. Lombardo, Leigh N. Fletcher, Patrick Irwin
Summary: This work presents the first infrared spectra of Titan obtained from the Spitzer Space Telescope. The data includes emissions of various molecules such as CH4, C2H2, C2H4, C2H6, C3H4, C3H6, C3H8, C4H2, HCN, HC3N, and CO2. Comparisons with the Cassini Composite Infrared Spectrometer (CIRS) reveal discrepancies in the observations, suggesting the need for further analysis.
PLANETARY SCIENCE JOURNAL
(2023)
Article
Astronomy & Astrophysics
Andrew S. Rivkin, Cristina A. Thomas, Ian Wong, Benjamin Rozitis, Julia de Leon, Bryan Holler, Stefanie N. Milam, Ellen S. Howell, Heidi B. Hammel, Anicia Arredondo, John R. Brucato, Elena M. Epifani, Simone Ieva, Fiorangela La Forgia, Michael P. Lucas, Alice Lucchetti, Maurizio Pajola, Giovanni Poggiali, Jessica N. Sunshine, Josep M. Trigo-Rodriguez
Summary: The Didymos binary asteroid, studied through the DART mission, is classified as an S-type asteroid with LL chondrite composition. Its thermal properties and emission spectrum are consistent with those of S-complex asteroids, making it a good proxy for ordinary chondrite asteroids and potential future impactors.
PLANETARY SCIENCE JOURNAL
(2023)
Article
Geochemistry & Geophysics
P. G. J. Irwin, J. Dobinson, A. James, M. H. Wong, L. N. Fletcher, M. T. Roman, N. A. Teanby, D. Toledo, G. S. Orton, S. Perez-Hoyos, A. Sanchez-Lavega, A. Simon, R. Morales-Juberias, I. de Pater
Summary: Spectral observations of Neptune in 2019 reveal spatial variations in aerosol scattering properties and methane abundance in the planet's atmosphere. The darkening of certain features in the atmosphere is due to spectrally dependent darkening of particles in a deep aerosol layer, while bright zones at longer wavelengths are attributed to brightening of particles in the same aerosol layer. The properties of an upper methane/haze aerosol layer remain constant with latitude, and variations in an upper tropospheric haze layer account for changes in reflectivity at methane-absorbing wavelengths.
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
(2023)
Article
Astronomy & Astrophysics
Michael T. Roman, Leigh N. Fletcher, Glenn S. Orton, Thomas K. Greathouse, Julianne I. Moses, Naomi Rowe-Gurney, Patrick G. J. Irwin, Arrate Antunano, James Sinclair, Yasumasa Kasaba, Takuya Fujiyoshi, Imke de Pater, Heidi B. Hammel
Summary: This study analyzes all currently available ground-based imaging data of Neptune in the mid-infrared and reveals significant subseasonal variation in the stratosphere. The observations show changes in stratospheric temperature and provide strong evidence for subseasonal processes on both global and regional scales in Neptune's atmosphere.
PLANETARY SCIENCE JOURNAL
(2022)
Article
Astronomy & Astrophysics
Simone Ieva, E. Mazzotta Epifani, D. Perna, M. Dall'Ora, V Petropoulou, J. D. P. Deshapriya, P. H. Hasselmann, A. Rossi, G. Poggiali, J. R. Brucato, M. Pajola, A. Lucchetti, S. L. Ivanovski, P. Palumbo, V Della Corte, A. Zinzi, A. S. Rivkin, C. A. Thomas, J. de Leon, E. Dotto, M. Amoroso, I Bertini, A. Capannolo, B. Cotugno, G. Cremonese, V Di Tana, I Gai, G. Impresario, M. Lavagna, A. Meneghin, F. Miglioretti, D. Modenini, S. Pirrotta, E. Simioni, S. Simonetti, P. Tortora, M. Zannoni, G. Zanotti
Summary: This study presents the spectral characterization of the smallest member of the Didymos binary near-Earth object system (Dimorphos). It confirms the presence of subtle and persistent spectral variability, suggesting different compositions may play a role. Future observations in synergy with data from LUKE on board LICIACube will further investigate this conundrum.
PLANETARY SCIENCE JOURNAL
(2022)
Article
Astronomy & Astrophysics
Shantanu P. Naidu, Steven R. Chesley, Davide Farnocchia, Nick Moskovitz, Petr Pravec, Petr Scheirich, Cristina Thomas, Andrew S. Rivkin
Summary: By analyzing the occultations and eclipses in the light curves of the 65803 Didymos binary system, we estimated the orbital parameters of Dimorphos relative to Didymos. Our results show that the period of Dimorphos' mutual orbit is approximately 11.921 487 hours, and the mean motion of the orbit is changing at a rate of (5.0 +/- 1.0) x 10(-18) rad s(-2). These findings are of significance for studying the orbital phase during the Double Asteroid Redirection Test (DART) mission.
PLANETARY SCIENCE JOURNAL
(2022)
Article
Astronomy & Astrophysics
Andrew S. Rivkin, Joshua P. Emery, Ellen S. Howell, Theodore Kareta, John W. Noonan, Matthew Richardson, Benjamin N. L. Sharkey, Amanda A. Sickafoose, Laura M. Woodney, Richard J. Cartwright, Sean Lindsay, Lucas T. Mcclure
Summary: This study presents evidence of a divide in the 3 μm spectral properties of low-albedo asteroids. The spectra can be divided into two groups: sharp types (STs) with spectral shape consistent with carbonaceous chondrite meteorites, and not sharp types (NSTs) that are not represented in meteorite literature. Statistical tests reveal significant differences in average band depth, semimajor axis, and perihelion between the STs and NSTs.
PLANETARY SCIENCE JOURNAL
(2022)
Meeting Abstract
Geochemistry & Geophysics
Nancy L. Chabot, Andrew S. Rivkin, Andrew F. Cheng, Elena Y. Adams, Edward L. Reynolds
METEORITICS & PLANETARY SCIENCE
(2022)