Rengel, M.; Moreno, R.; Courtin, R.; Lellouch, E.; Sagawa, H.; Hartogh, P.; Swinyard, B.; Lara, L.; Feuchtgruber, H.; Jarchow, C.et al.; Fulton, T.; Cernicharo, J.; Bockelée-Morvan, D.; Biver, N.; Banaszkiewicz, M.; González, A.: Tracing the Oxygen-related Gas Composition of Titan's Atmosphere with Herschel. Water in the Universe: from Clouds to Oceans, Noordwijk, Netherlands (2016)
Rengel, M.; Reach, W.; Hartogh, P.; Sagawa, H.: Tracing the Composition of Hydrogen Cyanide in the Stratosphere of Titan from Space, Airbone and Ground-Based Observations. Asia Oceania Geosciences Society (AOGS) 13th Annual Meeting, Beijing, China (2016)
de Val-Borro, M.; Bockelée-Morvan, D.; Jehin, E.; Hartogh, P.; Opitom, C.; Szutowicz, S.; Biver, N.; Crovisier, J.; Lis, D. C.; Rezac, L.et al.; de Graauw, T.; Hutsemékers, D.; Jarchow, C.; Kidger, M. R.; Küppers, M.; Lara, L. M.; Manfroid, J.; Rengel, M.; Swinyard, B. M.; Teyssier, D.; Vandenbussche, B.; Waelkens, C.: Distant activity of comet C/2006 W3 (Christensen) as observed with Herschel. Ground and space observatories: a joint venture to planetary science, Santiago, Chile (2015)
Rengel, M.: Trans-Neptunian Objects: recent Advances, Synergy from ground and space-based observations, and Perspectives. Ground and space observatories: a joint venture to planetary science, Santiago, Chile (2015)
Rengel, M.: La extraña química de la atmósfera de Titán vista con el Observatorio Espacial Herschel. Seminar at the Center of Physics, Caracas, Venezuela (2015)
Rengel, M.; Sagawa, H.; Hartogh, P.: Hydrogen Cyanide in the Stratosphere of Titan. 12th Annual Meeting Asia Oceania Geosciences Society, Singapore (2015)
Rengel, M.; Sagawa, H.; Hartogh, P.: Hydrogen Cyanide in the Stratosphere of Titan. 12th Annual Meeting Asia Oceania Geosciences Society, Singapore (2015)
de Val-Borro, M.; Bockelée-Morvan, D.; Jehin, E.; Hartogh, P.; Opitom, C.; Szutowicz, S.; Biver, N.; Crovisier, J.; Lis, D.; Rezac, L.et al.; de Graauw, T.; Hutsemékers, D.; Jarchow, C.; Kidger, M. R.; Küppers, M.; Lara, L. M.; Manfroid, J.; Rengel, M.; Swinyard, B. M.; Teyssier, D.; Vandenbussche, B.; Waelkens, C.: Distant activity of comet C/2006 W3 (Christensen) as observed with Herschel. Asteroids, Comets, Meteors, Helsinki, Finland (2014)
Hartogh, P.; Rezac, L.; Moreno, R.; Lellouch, E.; Rengel, M.; Jarchow, C.; de Val-Borro, M.; Crovisier, J.; Biver, N.; Bockeleé-Morvan: Detection and characterization of Ganymede's and Callisto's water atmospheres. 11th Annual Meeting, Asia Oceania Geosciences Society, Sapporo, Japan (2014)
Hartogh, P.; Sagawa, H.; Rengel, M.: APEX submillimetre observations of HCl and HDO in the mesosphere of Venus. 40th COSPAR Scientific Assembly, Moscow, Russia (2014)
Lara, L.-M.; Lellouch, E.; González, M.; Moreno, R.; Rengel, M.: Exploring external time-dependent sources of H2O into Titan's atmosphere. European Geosciences Union General Assembly 2014, Vienna, Austria (2014)
Lellouch, E.; Hartogh, P.; Moreno, R.; Billebaud, F.; Bockelée-Morvan, D.; Biver, N.; Cassidy, T.; Courtin, R.; Crovisier, J.; Dobrijevic, M.et al.; Feuchtgruber, H.; González, A.; Greathouse, T.; Jarchow, C.; Kidger, M.; Lara, L. M.; Rengel, M.; Orton, G.; Sagawa, H.; de Val-Borro, M.; Cavalié, T.: The origin of external oxygen in Jupiter and Saturn's environments. Semaine de l'Astrophysique Francaise, Paris, France (2014)
Rengel, M.; Moreno, R.; Courtin, R.; Lellouch, E.; Sagawa, H.; Hartogh, P.; Swinyard, B.; Lara, L.; Feuchtgruber, H.; Jarchow, C.et al.; Fulton, T.; Cernicharo, J.; Bockelée-Morvan, D.; Biver, N.; Banaszkiewicz, M.; González, A.: Tracing the gas composition of Titan's atmosphere with Herschel: Advances and Discoveries. 46th Annual Meeting of the Division for Planetary Sciences, Tucson, AZ, USA (2014)
Rengel, M.; Sagawa, H.; Hartogh, P.: The HCN distribution in the stratosphere of Titan: an intercomparison between the HCN distributions obtained with Herschel/PACS and APEX-2. Asia Oceania Geosciences Society (AOGS) 11th Annual Meeting, Sapporo, Japan (2014)
The dwarf planet is a bizarre, cryovolcanic world. However, the organic deposits discovered on its surface so far are unlikely to originate from its interior.
The Uranian magnetic field is more expansive than previously thought, according to newly analyzed data from Voyager 2, making it easier to search for moons with oceans.