Detection of hydrogen sulfide above the clouds in Uranus’s atmosphere

Nature Astronomy Nature Publishing Group 2:2018 (2018) 420-427

Authors:

Patrick Irwin, Daniel Toledo Carrasco, Ryan Garland, N Teanby, L Fletcher, GS Orton, B Bezard

Abstract:

Visible-to-near-infrared observations indicate that the cloud top of the main cloud deck on Uranus lies at a pressure level of between 1.2 bar and 3 bar. However, its composition has never been unambiguously identified, although it is widely assumed to be composed primarily of either ammonia or hydrogen sulfide (H2S) ice. Here, we present evidence of a clear detection of gaseous H2S above this cloud deck in the wavelength region 1.57–1.59 μm with a mole fraction of 0.4–0.8 ppm at the cloud top. Its detection constrains the deep bulk sulfur/nitrogen abundance to exceed unity (>4.4–5.0 times the solar value) in Uranus’s bulk atmosphere, and places a lower limit on the mole fraction of H2S below the observed cloud of (1.0−2.5)×10−5. The detection of gaseous H2S at these pressure levels adds to the weight of evidence that the principal constituent of 1.2–3-bar cloud is likely to be H2S ice.

The Transiting Exoplanet Community Early Release Science Program for JWST

(2018)

Authors:

Jacob L Bean, Kevin B Stevenson, Natalie M Batalha, Zachory Berta-Thompson, Laura Kreidberg, Nicolas Crouzet, Björn Benneke, Michael R Line, David K Sing, Hannah R Wakeford, Heather A Knutson, Eliza M-R Kempton, Jean-Michel Désert, Ian Crossfield, Natasha E Batalha, Julien de Wit, Vivien Parmentier, Joseph Harrington, Julianne I Moses, Mercedes Lopez-Morales, Munazza K Alam, Jasmina Blecic, Giovanni Bruno, Aarynn L Carter, John W Chapman, Leen Decin, Diana Dragomir, Thomas M Evans, Jonathan J Fortney, Jonathan D Fraine, Peter Gao, Antonio García Muñoz, Neale P Gibson, Jayesh M Goyal, Kevin Heng, Renyu Hu, Sarah Kendrew, Brian M Kilpatrick, Jessica Krick, Pierre-Olivier Lagage, Monika Lendl, Tom Louden, Nikku Madhusudhan, Avi M Mandell, Megan Mansfield, Erin M May, Giuseppe Morello, Caroline V Morley, Nikolay Nikolov, Seth Redfield, Jessica E Roberts, Everett Schlawin, Jessica J Spake, Kamen O Todorov, Angelos Tsiaras, Olivia Venot, William C Waalkes, Peter J Wheatley, Robert T Zellem, Daniel Angerhausen, David Barrado, Ludmila Carone, Sarah L Casewell, Patricio E Cubillos, Mario Damiano, Miguel de Val-Borro, Benjamin Drummond, Billy Edwards, Michael Endl, Nestor Espinoza, Kevin France, John E Gizis, Thomas P Greene, Thomas K Henning, Yucian Hong, James G Ingalls, Nicolas Iro, Patrick GJ Irwin, Tiffany Kataria, Fred Lahuis, Jérémy Leconte, Jorge Lillo-Box, Stefan Lines, Joshua D Lothringer, Luigi Mancini, Franck Marchis, Nathan Mayne, Enric Palle, Emily Rauscher, Gaël Roudier, Evgenya L Shkolnik, John Southworth, Mark R Swain, Jake Taylor, Johanna Teske, Giovanna Tinetti, Pascal Tremblin, Gregory S Tucker, Roy van Boekel, Ingo P Waldmann, Ian C Weaver, Tiziano Zingales

The proposed Caroline ESA M3 mission to a Main Belt Comet

Advances in Space Research Elsevier 62:8 (2018) 1921-1946

Authors:

GH Jones, J Agarwal, Neil Bowles, M Burchell, AJ Coates, A Fitzsimmons, A Graps, HH Hsieh, CM Lisse, SC Lowry, A Masters, C Snodgrass, C Tubiana

Abstract:

We describe Caroline, a mission proposal submitted to the European Space Agency in 2010 in response to the Cosmic Visions M3 call for medium-sized missions. Caroline would have travelled to a Main Belt Comet (MBC), characterizing the object during a flyby, and capturing dust from its tenuous coma for return to Earth. MBCs are suspected to be transition objects straddling the traditional boundary between volatile–poor rocky asteroids and volatile–rich comets. The weak cometary activity exhibited by these objects indicates the presence of water ice, and may represent the primary type of object that delivered water to the early Earth. The Caroline mission would have employed aerogel as a medium for the capture of dust grains, as successfully used by the NASA Stardust mission to Comet 81P/Wild 2. We describe the proposed mission design, primary elements of the spacecraft, and provide an overview of the science instruments and their measurement goals. Caroline was ultimately not selected by the European Space Agency during the M3 call; we briefly reflect on the pros and cons of the mission as proposed, and how current and future mission MBC mission proposals such as Castalia could best be approached.

Investigations of the Mars Upper Atmosphere with ExoMars Trace Gas Orbiter

SPACE SCIENCE REVIEWS 214:1 (2018) UNSP 29

Authors:

MA Lopez-Valverde, J-C Gerard, F Gonzalez-Galindo, A-C Vandaele, I Thomas, O Korablev, N Ignatiev, A Fedorova, F Montmessin, A Maattanen, S Guilbon, F Lefevre, MR Patel, S Jimenez-Monferrer, M Garcia-Comas, A Cardesin, CF Wilson, RT Clancy, A Kleinboehl, DJ McCleese, DM Kass, NM Schneider, MS Chaffin, JJ Lopez-Moreno, J Rodriguez

LRG-BEASTS III: ground-based transmission spectrum of the gas giant orbiting the cool dwarf WASP-80

MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY 474:1 (2018) 876-885

Authors:

J Kirk, PJ Wheatley, T Louden, I Skillen, GW King, J McCormac, PGJ Irwin