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by Tinetti, Giovanna and Drossart, Pierre and Eccleston, Paul and Hartogh, Paul and Heske, Astrid and Leconte, Jérémy and Micela, Giusi and Ollivier, Marc and Pilbratt, Göran and Puig, Ludovic and Turrini, Diego and Vandenbussche, Bart and Wolkenberg, Paulina and Beaulieu, Jean-Philippe and Buchave, Lars A and Ferus, Martin and Griffin, Matt and Guedel, Manuel and Justtanont, Kay and Lagage, Pierre-Olivier and Machado, Pedro and Malaguti, Giuseppe and Min, Michiel and Nørgaard-Nielsen, Hans Ulrik and Rataj, Mirek and Ray, Tom and Ribas, Ignasi and Swain, Mark and Szabo, Robert and Werner, Stephanie and Barstow, Joanna and Burleigh, Matt and Cho, James and du Foresto, Vincent Coudé and Coustenis, Athena and Decin, Leen and Encrenaz, Therese and Galand, Marina and Gillon, Michael and Helled, Ravit and Morales, Juan Carlos and Muñoz, Antonio García and Moneti, Andrea and Pagano, Isabella and Pascale, Enzo and Piccioni, Giuseppe and Pinfield, David and Sarkar, Subhajit and Selsis, Franck and Tennyson, Jonathan and Triaud, Amaury and Venot, Olivia and Waldmann, Ingo and Waltham, David and Wright, Gillian and Amiaux, Jerome and Auguères, Jean-Louis and Berthé, Michel and Bezawada, Naidu and Bishop, Georgia and Bowles, Neil and Coffey, Deirdre and Colomé, Josep and Crook, Martin and Crouzet, Pierre-Elie and Da Peppo, Vania and Sanz, Isabel Escudero and Focardi, Mauro and Frericks, Martin and Hunt, Tom and Kohley, Ralf and Middleton, Kevin and Morgante, Gianluca and Ottensamer, Roland and Pace, Emanuele and Pearson, Chris and Stamper, Richard and Symonds, Kate and Rengel, Miriam and Renotte, Etienne and Ade, Peter and Affer, Laura and Alard, Christophe and Allard, Nicole and Altieri, Francesca and André, Yves and Arena, Claudio and Argyriou, Ioannis and Aylward, Alan and Baccani, Cristian and Bakos, Gaspar and Banaszkiewicz, Marek and Barlow, Mike and Batista, Virginie and Bellucci, Giancarlo and Benatti, Serena and Bernardi, Pernelle and Bézard, Bruno and Blecka, Maria and Bolmont, Emeline and ...
Experimental Astronomy, ISSN 0922-6435, 11/2018, Volume 46, Issue 1, pp. 135 - 209
Thousands of exoplanets have now been discovered with a huge range of masses, sizes and orbits: from rocky Earth-like planets to large gas giants grazing the... 
Statistics for Engineering, Physics, Computer Science, Chemistry and Earth Sciences | Space missions | Molecular signatures | IR spectroscopy | Physics | Exoplanets | Astronomy, Observations and Techniques | VALIDATED PLANETS | EXTRASOLAR GIANT PLANETS | TRANSITING EXOPLANETS | INFRARED-EMISSION-SPECTRUM | SUPER-EARTH | BROWN DWARF | STELLAR ACTIVITY | JUPITER EXOPLANETS | TRANSMISSION SPECTRUM | ASTRONOMY & ASTROPHYSICS | SPACE-BASED PHOTOMETRY | Extrasolar planets | Analysis | Natural history | Terrestrial planets | Clouds | Molecular structure | Metal compounds | Carbon dioxide | Mapping | Planetary composition | Hydrogen sulfide | Star formation | Planet detection | Planet formation | Chemical composition | Ephemerides | Solar system | Atmospheric gases | Photometry | Stellar systems | Spectroscopy | Computer simulation | Feasibility studies | Noise measurement | Transit | Surveys | Gases | Organic chemistry | Ammonia | Satellites | Atmosphere | Planetary evolution | Gas giant planets | Astrochemistry | Stellar activity | Nebulae | Earth and Planetary Astrophysics | Sciences of the Universe | Astrophysics | Astronomi, astrofysik och kosmologi | Meteorologi och atmosfärforskning | Atom- och molekylfysik och optik | Atom and Molecular Physics and Optics | Meteorology and Atmospheric Sciences | Astronomy, Astrophysics and Cosmology
Journal Article
Philosophical Transactions of the Royal Society A: Mathematical, Physical and Engineering Sciences, ISSN 1364-503X, 2019, Volume 377, Issue 2154
Thirty years of observations of H 3 + on Jupiter have addressed many complex questions about the physics of the ionospheres of the giant planets. Spectroscopy,... 
Sciences of the Universe | Astrophysics | exoplanets | planetary atmospheres | 169 | Solar System | 1002 | 1000 | 196 | infrared spectroscopy
Journal Article
PHILOSOPHICAL TRANSACTIONS OF THE ROYAL SOCIETY A-MATHEMATICAL PHYSICAL AND ENGINEERING SCIENCES, ISSN 1364-503X, 09/2019, Volume 377, Issue 2154, p. 20180404
Thirty years of observations of H-3(+) on Jupiter have addressed many complex questions about the physics of the ionospheres of the giant planets.... 
exoplanets | planetary atmospheres | GRAVITY-WAVES | MULTIDISCIPLINARY SCIENCES | UPPER-ATMOSPHERE | MODEL | H-3 | Solar System | FUNDAMENTAL-BAND | THERMOSPHERE | SPECTRO-IMAGING OBSERVATIONS | AURORAL EMISSION | LOW-LATITUDE | IO FLUX TUBE | infrared spectroscopy
Journal Article
Science, ISSN 0036-8075, 4/2006, Volume 312, Issue 5772, pp. 400 - 404
Global mineralogical mapping of Mars by the Observatoire pour la Mineralogie, l'Eau, les Glaces et l'Activité (OMEGA) instrument on the European Space Agency's... 
Mars | Liquids | Pyroxenes | Clay minerals | Oxides | Weathering processes | Planetary science | Orbits | Research Articles | Minerals | Sulfates | GUSEV CRATER | CRUST | DUST | EVOLUTION | SPIRIT ROVER | MULTIDISCIPLINARY SCIENCES | SURFACE | DIVERSITY | IDENTIFICATION | MERIDIANI | CLIMATE | Water | Ferric Compounds | Atmosphere | Aluminum Silicates | Time | Extraterrestrial Environment | Silicates | Carbon Dioxide | Analysis | Mars (Planet) | Research
Journal Article
Nature, ISSN 0028-0836, 04/2004, Volume 428, Issue 6983, pp. 627 - 630
The inventory of water and carbon dioxide reservoirs on Mars are important clues for understanding the geological, climatic and potentially exobiological... 
SURFACE | TOPOGRAPHY | MULTIDISCIPLINARY SCIENCES | RESIDUAL CO2 FROST | Geography | Exobiology | Mars | Carbon Dioxide - chemistry | Water - analysis | Water - chemistry | Ice - analysis | Carbon Dioxide - analysis | Extraterrestrial Environment - chemistry | Water | Ice | Carbon dioxide
Journal Article
Journal of Geophysical Research - Planets, ISSN 0148-0227, 08/2007, Volume 112, Issue E8, pp. E08S15 - n/a
Journal Article
Science, ISSN 0036-8075, 4/2010, Volume 328, Issue 5978, pp. 605 - 608
Journal Article
Journal Article
by Piccioni, G and Drossart, P and Sanchez-Lavega, A and Hueso, R and Taylor, F.W and Wilson, C.F and Grassi, D and Zasova, L and Moriconi, M and Adriani, A and Lebonnois, S and Coradini, A and Bézard, B and Angrilli, F and Arnold, G and Baines, K.H and Bellucci, G and Benkhoff, J and Bibring, J.P and Blanco, A and Blecka, M.I and Carlson, R.W and Di Lellis, A and Encrenaz, T and Erard, S and Fonti, S and Formisano, V and Fouchet, T and Garcia, R and Haus, R and Helbert, J and Ignatiev, N.I and Irwin, P.G.J and Langevin, Y and Lopez-Valverde, M.A and Luz, D and Marinangeli, L and Orofino, V and Rodin, A.V and Roos-Serote, M.C and Saggin, B and Stam, D.M and Titov, D and Visconti, G and Zambelli, M and Ammannito, Eleonora and Barbis, Alessandra and Berlin, Rainer and Bettanini, Carlo and Boccaccini, Angelo and Bonnello, Guillaume and Bouye, Marc and Capaccioni, Fabrizio and Cardesin Moinelo, Alejandro and Carraro, Francesco and Cherubini, Giovanni and Cosi, Massimo and Dami, Michele and De Nino, Maurizio and Del Vento, Davide and Di Giampietro, Marco and Donati, Alessandro and Dupuis, Olivier and Espinasse, Sylvie and Fabbri, Anna and Fave, Agnes and Veltroni, Iacopo Ficai and Filacchione, Gianrico and Garceran, Katia and Ghomchi, Yamina and Giustini, Maurizio and Gondet, Brigitte and Hello, Yann and Henry, Florence and Hofer, Stefan and Huntzinger, Gerard and Kachlicki, Juergen and Knoll, René and Driss, Kouach and Mazzoni, Alessandro and Melchiorri, Riccardo and Mondello, Giuseppe and Monti, Francesco and Neumann, Christian and Nuccilli, Fabrizio and Parisot, Jerome and Pasqui, Claudio and Perferi, Stefano and Peter, Gisbert and Piacentino, Alain and Pompei, Carlo and Reess, Jean-Michel and Rivet, Jean-Pierre and Romano, Antonio and Russ, Natalie and Santoni, Massimo and Scarpelli, Adelmo and Semery, Alain and Soufflot, Alain and Stefanovitch, Douchane and ... and VIRTIS-Venis Express Tech Te and VIRTIS-Venus Express Technical Team and the VIRTIS-Venus Express Technical Team
Nature, ISSN 0028-0836, 11/2007, Volume 450, Issue 7170, pp. 637 - 640
Venus has no seasons, slow rotation and a very massive atmosphere, which is mainly carbon dioxide with clouds primarily of sulphuric acid droplets. Infrared... 
CLOUD STRUCTURE | NIGHT-SIDE | SPECTRA | MULTIDISCIPLINARY SCIENCES | ATMOSPHERE | PIONEER ORBITER | Gases | Astrophysics | Astronomical research | Venus | Atmosphere | Planetology | Earth Sciences | Sciences of the Universe
Journal Article