Article
Astronomy & Astrophysics
P. Rannou, M. Coutelier, E. Riviere, S. Lebonnois, M. Rey, L. Maltagliati
Summary: Methane plays crucial roles in the complex prebiotic chemistry, global haze, cloud formation, and rainfall on Titan. Through solar occultation studies, researchers have found methane intrusion into the stratosphere and its impact on the long-term evolution of Titan's atmosphere and climate. Further studies using global climate models are necessary to fully understand the methane cycle and its implications under changing conditions.
ASTROPHYSICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
Erich Karkoschka
Summary: An analysis of three new image cubes of Titan by the Space Telescope Imaging Spectrograph reveals that Titan's seasonal variation is close to harmonic and not influenced by variations due to Saturn's orbital eccentricity. The reversal consists of two components, with small temporary deviations observed. These new observations provide an improved seasonal model that will help in future global circulation models of Titan.
Article
Astronomy & Astrophysics
Darci Snowden, Alexandre Higgins
Summary: The study shows that Titan's induced magnetosphere is effective in shielding the atmosphere from thermal proton precipitation but only partially shields it from thermal oxygen precipitation. The energy deposited by thermal magnetospheric oxygen is lower than solar EUV input but similar to energy deposited by high energy neutral atoms and magnetospheric electrons.
Article
Geosciences, Multidisciplinary
F. Comola, J. F. Kok, J. M. Lora, K. Cohanim, X. Yu, C. He, P. McGuiggan, S. M. Horst, F. Turney
Summary: Titan, Saturn's largest moon, has huge linear dunes and an active dust cycle. Similar to Earth, these aeolian processes are caused by wind moving surface grains. However, it is still unclear how saltation can occur on Titan with its weak winds and potentially cohesive grains. This study suggests that saltation may occur on Titan through granular splash instead of aerodynamic lifting, and the prevailing circulation on Titan can generate significant yet intermittent saltation.
GEOPHYSICAL RESEARCH LETTERS
(2022)
Article
Astronomy & Astrophysics
Juan M. Lora, J. Michael Battalio, Mary Yap, Colin Baciocco
Summary: The cause of the hemispheric asymmetry of Titan's methane lakes and seas is still under debate, with seasonal insolation asymmetries and topographic variations both proposed as contributing factors. However, simulations suggest that topography has a minor effect on the global distribution of methane liquid, while orbital forcing and surface hydrology are more likely to dictate the distribution.
Article
Astronomy & Astrophysics
A. Sanchez-Lopez, M. Lopez-Puertas, M. Garcia-Comas, B. Funke, T. Fouchet, I. A. G. Snellen
Summary: This study investigates the methane concentration in the upper atmosphere of Jupiter and accurately models the methane radiance measured by ISO/SWS. The results indicate that a high concentration of methane is required to explain the data, and the observations support the lower limit of methane collisional relaxation rates.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
Motoki Sumi, Shin-ichi Takehiro, Wataru Ohfuchi, Hideko Nomura, Yuka Fujii
Summary: In this paper, the effects of the haze layer on the stratospheric superrotation in Titan's atmosphere were explored using numerical experiments. It was found that the intensity and location of the maximum zonal wind velocity are highly dependent on the optical thickness and altitude of the haze layer. The analysis suggests that the quasi-stationary stratospheric superrotation is maintained by the balance between the meridional circulation decoupled from the surface and the eddies that transport angular momentum equatorward. This structure may explain the no-wind region at about 80 km in altitude.
ASTROPHYSICAL JOURNAL
(2022)
Article
Astronomy & Astrophysics
J. Michael Battalio, Juan M. Lora, Scot Rafkin, Alejandro Soto
Summary: The influence of methane on the circulation of Titan is investigated using a simplified moist convection parameterization scheme. The results show that the reference relative humidity has a significant impact on convective instability and precipitation, while the relaxation timescale of convection has minor effects. The behavior of convection varies with the relative humidity, with infrequent and intense events at low relative humidity and near-continuous precipitation at high relative humidity during summer. Intermediate relative humidity values result in frequent events of moderate intensity.
Article
Astronomy & Astrophysics
Benoit Seignovert, Pascal Rannou, Robert A. West, Sandrine Vinatier
Summary: This study presents a 13-year survey of haze UV extinction profiles in Titan's upper atmosphere, observing the evolution of the detached haze layer (DHL) at different latitudes. The DHL globally sunk and disappeared in 2012, re-emerging from the Northern hemisphere in late 2015. Variability of the DHL was observed in 2005, with slightly higher extinction on the dawn side and some local inhomogeneities during a 2009 polar flyby.
ASTROPHYSICAL JOURNAL
(2021)
Article
Engineering, Aerospace
Teyen Widdicombe, R. A. Borrelli
Summary: A pressure vessel was used to simulate the atmosphere of Titan and measure neutron attenuation. The results showed that the atmosphere and surface material have minimal impact on neutron measurements. This study confirms the accuracy of neutron modeling and concludes that neutrons from MMRTG are unlikely to affect Dragonfly's measurements on Titan's surface.
Article
Environmental Sciences
J. Sanchez-Rodriguez, A. Sierra, D. Jimenez-Lopez, T. Ortega, A. Gomez-Parra, J. Forja
Summary: The study investigated the concentration of dissolved CH4 and N2O, as well as the partial pressure of CO2 in the Guadalquivir estuary. Factors such as temperature, salinity, exchange with the atmosphere, biochemical processes, and river inputs were found to influence the distribution of gases. The estuary acts as a source of these gases to the atmosphere, with positive water-atmosphere fluxes throughout the study.
SCIENCE OF THE TOTAL ENVIRONMENT
(2022)
Article
Astronomy & Astrophysics
Nicholas A. Lombardo, Juan M. Lora
Summary: Titan's atmosphere shows variations in composition as it goes through different seasons. Winter stratosphere above 100 km has been found to have higher amounts of short-lived molecules. Seasonal changes in stratospheric dynamics on Titan also lead to a transient detached haze layer above 400 km. These seasonal variations affect the radiative heating rates in both shortwave and longwave regions. Based on simulations using the Titan Atmospheric Model (TAM), this study examines the impact of a new dataset derived from Cassini observations on aerosol opacity and trace gas abundance. The results show that including seasonally varying radiative species (SVRS) decreases the temperature of polar stratopause in autumn and winter by up to 10 K, and increases the seasonality in zonal winds.
Article
Geochemistry & Geophysics
J. Mouzay, I. Couturier-Tamburelli, N. Pietri, T. Chiavassa
Summary: Laboratory experiments were conducted to study the photochemical evolution induced by long-UV irradiation of benzene ices in Titan's atmosphere. The formation of volatile photo-products and residue dominated by nu CH IR features from UV photolysis of benzene ices were observed, providing insights into the composition of Titan's stratospheric haze layer. Additionally, the characterization of benzene-containing aerosol analogs induced by long-UV will contribute to Titan's surface organics layer and future Dragonfly space mission.
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
(2021)
Article
Geochemistry & Geophysics
Jianping Huang, Zhaopeng Wu, Jun Cui, Xin Wan, Jiahao Zhong, Yongqiang Hao
Summary: This study used a full-wave model to simulate the observed gravity wave structure on Titan and found that gravity waves could significantly modify the temperature structure of the upper atmosphere. The thermal effect of gravity waves is sensitive to eddy viscosity.
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
(2022)
Article
Astronomy & Astrophysics
Scot C. R. Rafkin, Juan M. Lora, Alejandro Soto, J. Michael Battalio
Summary: The deep convective cloud-environment feedback loop is crucial for understanding Titan's global methane, energy, and momentum cycles. This study uses cloud resolving modeling to quantify the effects of deep convective methane storms on their environment and improve parameterizations in global models.
Article
Astronomy & Astrophysics
Adam D. Jacobs, Michael E. Summers, Andrew F. Cheng, G. Randall Gladstone, Carey M. Lisse, W. Dean Pesnell, Tanguy Bertrand, Darrell F. Strobel, Leslie A. Young, Harold A. Weaver, Joshua Kammer, Peter Gao
Summary: Analysis of images captured by New Horizons spacecraft during its flyby of Pluto revealed the existence of wave structures in Pluto's atmosphere, suggesting possible wave types and characteristics. These findings provide valuable insights into the dynamics of Pluto's atmosphere and motivate further research.
Article
Astronomy & Astrophysics
G. Randall Gladstone, Joshua A. Kammer, Danica J. Adams, Yuk L. Yung, Wayne R. Pryor, Darrell F. Strobel, Leslie A. Young, Joel W. M. Parker, S. Alan Stern
Summary: The Alice spectrograph on New Horizons observed far-ultraviolet airglow emissions on Pluto during a flyby in July 2015. One particular observation, PColor2, provided insight into the emission lines of atomic hydrogen and the abundance profiles of H atoms and CH4 molecules in Pluto's atmosphere, which can be used to monitor seasonal climate variations remotely. The brightness of Lyman alpha emissions and the near-surface mixing ratio of CH4 on Pluto were highlighted in the study.
Article
Astronomy & Astrophysics
Jane S. Greaves, Anita M. S. Richards, William Bains, Paul B. Rimmer, Hideo Sagawa, David L. Clements, Sara Seager, Janusz J. Petkowski, Clara Sousa-Silva, Sukrit Ranjan, Emily Drabek-Maunder, Helen J. Fraser, Annabel Cartwright, Ingo Mueller-Wodarg, Zhuchang Zhan, Per Friberg, Iain Coulson, E'lisa Lee, Jim Hoge
Summary: Measurements of phosphine gas in Venus's atmosphere have been reported, with the presence of the gas currently unexplained. Possible origins include unknown photochemical or geochemical processes, or even the presence of life, resembling the biological production of phosphine on Earth. Further research is needed to investigate the sources and nature of this gas on Venus.
Correction
Astronomy & Astrophysics
M. Galand, P. D. Feldman, D. Bockelee-Morvan, N. Biver, Y. -C. Cheng, G. Rinaldi, M. Rubin, K. Altwegg, J. Deca, A. Beth, P. Stephenson, K. L. Heritier, P. Henri, J. Wm. Parker, C. Carr, A. I. Eriksson, J. Burch
Summary: The paper has been corrected and the updated version can be found at https://doi.org/10.1038/s41550-021-01373-5.
Article
Astronomy & Astrophysics
G. Randall Gladstone, Wayne R. Pryor, Doyle T. Hall, Joshua A. Kammer, Darrell F. Strobel, Harold A. Weaver, John R. Spencer, Kurt D. Retherford, Maarten H. Versteeg, Michael W. Davis, Leslie A. Young, Andrew J. Steffl, Joel Wm Parker, Carey M. Lisse, Kelsi N. Singer, S. Alan Stern
Summary: Observations using the Alice spectrograph on the New Horizons spacecraft have revealed a distant and constant Lyman-alpha background in the interplanetary medium, representing the local Galactic Lyman-alpha background. The brightness of the background is not strongly correlated with the cloud structure of the local interplanetary medium, and the absorption coefficient of interstellar dust at Lyman-alpha wavelength has been constrained to be approximately 0.2 kpc(-1).
ASTRONOMICAL JOURNAL
(2021)
Article
Astronomy & Astrophysics
J. Marques Oliveira, B. Sicardy, A. R. Gomes-Junior, J. L. Ortiz, D. F. Strobel, T. Bertrand, F. Forget, E. Lellouch, J. Desmars, D. Berard, A. Doressoundiram, J. Lecacheux, R. Leiva, E. Meza, F. Roques, D. Souami, T. Widemann, P. Santos-Sanz, N. Morales, R. Duffard, E. Fernandez-Valenzuela, A. J. Castro-Tirado, F. Braga-Ribas, B. E. Morgado, M. Assafin, J. I. B. Camargo, R. Vieira-Martins, G. Benedetti-Rossi, S. Santos-Filho, M. Banda-Huarca, F. Quispe-Huaynasi, C. L. Pereira, F. L. Rommel, G. Margoti, A. Dias-Oliveira, F. Colas, J. Berthier, S. Renner, R. Hueso, S. Perez-Hoyos, A. Sanchez-Lavega, J. F. Rojas, W. Beisker, M. Kretlow, D. Herald, D. Gault, K-L Bath, H-J Bode, E. Bredner, K. Guhl, T. Haymes, E. Hummel, B. Kattentidt, O. Kloes, A. Pratt, B. Thome, C. Avdellidou, K. Gazeas, E. Karampotsiou, L. Tzouganatos, E. Kardasis, A. A. Christou, E. M. Xilouris, I Alikakos, A. Gourzelas, A. Liakos, V Charmandaris, M. Jelinek, J. Strobl, A. Eberle, K. Rapp, B. Gaehrken, B. Klemt, S. Kowollik, R. Bitzer, M. Miller, G. Herzogenrath, D. Frangenberg, L. Brandis, I Puetz, V Perdelwitz, G. M. Piehler, P. Riepe, K. von Poschinger, P. Baruffetti, D. Cenadelli, J-M Christille, F. Ciabattari, R. Di Luca, D. Alboresi, G. Leto, R. Zanmar Sanchez, P. Bruno, G. Occhipinti, L. Morrone, L. Cupolino, A. Noschese, A. Vecchione, C. Scalia, R. Lo Savio, G. Giardina, S. Kamoun, R. Barbosa, R. Behrend, M. Spano, E. Bouchet, M. Cottier, L. Falco, S. Gallego, L. Tortorelli, S. Sposetti, J. Sussenbach, F. Van den Abbeel, P. Andre, M. Llibre, F. Pailler, J. Ardissone, M. Boutet, J. Sanchez, M. Bretton, A. Cailleau, V Pic, L. Granier, R. Chauvet, M. Conjat, J. L. Dauvergne, O. Dechambre, P. Delay, M. Delcroix, L. Rousselot, J. Ferreira, P. Machado, P. Tanga, J-P Rivet, E. Frappa, M. Irzyk, F. Jabet, M. Kaschinski, A. Klotz, Y. Rieugnie, A. N. Klotz, O. Labrevoir, D. Lavandier, D. Walliang, A. Leroy, S. Bouley, S. Lisciandra, J-F Coliac, F. Metz, D. Erpelding, P. Nougayrede, T. Midavaine, M. Miniou, S. Moindrot, P. Morel, B. Reginato, E. Reginato, J. Rudelle, B. Tregon, R. Tanguy, J. David, W. Thuillot, D. Hestroffer, G. Vaudescal, D. Baba Aissa, Z. Grigahcene, D. Briggs, S. Broadbent, P. Denyer, N. J. Haigh, N. Quinn, G. Thurston, S. J. Fossey, C. Arena, M. Jennings, J. Talbot, S. Alonso, A. Roman Reche, V Casanova, E. Briggs, R. Iglesias-Marzoa, J. Abril Ibanez, M. C. Diaz Martin, H. Gonzalez, J. L. Maestre Garcia, J. Marchant, I Ordonez-Etxeberria, P. Martorell, J. Salamero, F. Organero, L. Ana, F. Fonseca, V Peris, O. Brevia, A. Selva, C. Perello, V Cabedo, R. Goncalves, M. Ferreira, F. Marques Dias, A. Daassou, K. Barkaoui, Z. Benkhaldoun, M. Guennoun, J. Chouqar, E. Jehin, C. Rinner, J. Lloyd, M. El Moutamid, C. Lamarche, J. T. Pollock, D. B. Caton, V Kouprianov, B. W. Timerson, G. Blanchard, B. Payet, A. Peyrot, J-P Teng-Chuen-Yu, J. Francoise, B. Mondon, T. Payet, C. Boissel, M. Castets, W. B. Hubbard, R. Hill, H. J. Reitsema, O. Mousis, L. Ball, G. Neilsen, S. Hutcheon, K. Lay, P. Anderson, M. Moy, M. Jonsen, I Pink, R. Walters, B. Downs
Summary: This study investigated the atmospheric structure and seasonal variations of Triton, Neptune's main satellite, through the observation and analysis of a stellar occultation event. The results suggest that there is a seasonal variation in Triton's atmospheric pressure, and the pressure observed in 2017 is consistent with the extrapolation from 1989 data. However, the reported increase in surface pressure during the 1990s remains controversial.
ASTRONOMY & ASTROPHYSICS
(2022)
Article
Astronomy & Astrophysics
E. Lellouch, B. Butler, R. Moreno, M. Gurwell, P. Lavvas, T. Bertrand, T. Fouchet, D. F. Strobel, A. Moullet
Summary: New observations of Pluto's atmosphere were conducted with ALMA in 2017, revealing the presence of CO and HCN gases, providing vertical resolution of chemical and thermal data. Analysis indicated possible non-uniform temperature fields in the lower atmosphere, with summer pole latitudes being warmer than low latitudes. Detection of HNC was reported for the first time, with a ratio similar to that found in Titan's atmosphere.
Article
Astronomy & Astrophysics
J. M. Chadney, T. T. Koskinen, X. Hu, M. Galand, P. Lavvas, Y. C. Unruh, J. Serigano, S. M. Horst, R. Yelle
Summary: Researchers constructed neutral temperature and density profiles of H, H-2, He, and CH4 in Saturn's equatorial region using data from Cassini's instruments. They used an energy deposition model to calculate ion production rate profiles and rates of CH4 photo-dissociation, finding that high-resolution H-2 cross sections produce additional ionization peaks near 800 km altitude.
Article
Astronomy & Astrophysics
Peter Stephenson, M. Galand, J. Deca, P. Henri, G. Carnielli
Summary: The first 3D collisional model of electrons at a comet has been developed in this study. The model provides insights into the behaviors of electrons near the nucleus and their impact on the coma.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2022)
Article
Geosciences, Multidisciplinary
Zarah L. Brown, Alexander S. Medvedev, Ekaterina D. Starichenko, Tommi T. Koskinen, Ingo C. F. Mueller-Wodarg
Summary: This study investigates the gravity wave signatures in the Saturnian thermosphere observed by Cassini/Ultraviolet Imaging Spectrograph during the Grand Finale campaign. It demonstrates the upward propagation, saturation, and breaking of gravity wave packets, as well as the impact of wave drag on atmospheric circulation. The results provide insights into the global impact of gravity waves on Saturn's thermosphere.
GEOPHYSICAL RESEARCH LETTERS
(2022)
Article
Astronomy & Astrophysics
Darrell F. Strobel
Summary: The paper aims to investigate whether the H-2 density measurements reported by Cassini were overestimated by a factor of 2.2, and the potential impact of this overestimation on the atmospheres of Titan and Saturn.
Article
Geochemistry & Geophysics
A. Marzok, S. Schlegel, J. Saur, L. Roth, D. Grodent, D. F. Strobel, K. D. Retherford
Summary: We analyzed Hubble Space Telescope observations of Ganymede and generated a brightness map of its oxygen emission. We found that the brightness of Ganymede's auroral ovals varies significantly with longitude and is asymmetric with respect to the 270 degrees meridian. The southern auroral oval is brighter than the northern oval.
JOURNAL OF GEOPHYSICAL RESEARCH-PLANETS
(2022)
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
Geosciences, Multidisciplinary
Joachim Saur, Stefan Duling, Alexandre Wennmacher, Clarissa Willmes, Lorenz Roth, Darrell F. Strobel, Frederic Allegrini, Fran Bagenal, Scott J. Bolton, Bertrand Bonfond, George Clark, Randy Gladstone, Thomas K. Greathouse, Denis C. Grodent, Candice J. Hansen, William S. Kurth, Glenn S. Orton, Kurt D. Retherford, Abigail M. Rymer, Ali H. Sulaiman
Summary: This study presents the results of Hubble Space Telescope observations taken around the flyby of the Juno spacecraft on 7 June 2021 from Ganymede's orbitally trailing side. It is found that Ganymede's northern and southern auroral ovals alternate in brightness, with the oval facing Jupiter's magnetospheric plasma sheet being brighter. This suggests that the generator powering Ganymede's aurora is the momentum of the Jovian plasma sheet north and south of Ganymede's magnetosphere.
GEOPHYSICAL RESEARCH LETTERS
(2022)
Article
Astronomy & Astrophysics
Z. M. Lewis, A. Beth, K. Altwegg, M. Galand, C. Goetz, K. Heritier, L. O'Rourke, M. Rubin, P. Stephenson
Summary: The European Space Agency/Rosetta mission analyzed the ion composition in the coma of comet 67P/C-G and found high proton affinity species, particularly NH4+, indicating a high level of ion-neutral chemistry. The increased comet outgassing around perihelion led to more detections of NH4+ and other protonated HPA species, suggesting complex ion-neutral chemistry. The low magnetic field strength associated with the diamagnetic cavity was linked to higher NH4+ counts, indicating different transport dynamics inside and outside the diamagnetic cavity.
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
(2023)