South polar features on Venus similar to those near the north pole

Autor: Piccioni, G, Drossart, P., Sanchez Lavega, A., Hueso, R., Taylor, F. W., Wilson, C. F., Grassi, D., Zasova, L., Moriconi, M., Adriani, A., Lebonnois, S., Coradini, A., Bézard, B., Angrilli, Francesco, Arnold, G., Baines, K. H., Bellucci, G., Benkhoff, J., Bibring, J. P., Blanco, A., Blecka, M. I., Carlson, R. W., Di Lellis, A., Encrenaz, T., Erard, S., Fonti, S., Formisano, V., Fouchet, T., Garcia, R., Haus, R., Helbert, J., Ignatiev, N. I., Irwin, P. G. J., Langevin, Y., Lopez Valverde, M. A., Luz, D., Marinangeli, L., Orofino, V., Rodin, A. V., Roos Serote, M. C., Saggin, Bortolino, Stam, D. M., Titov, D., Visconti, G., Zambelli, M., Ammannito, Eleonora, Barbis, Alessandra, Berlin, Rainer, BETTANINI FECIA DI COSSATO, Carlo, Boccaccini, Angelo, Bonnello, Guillaume, Bouye, Marc, Capaccioni, Fabrizio, Cardesin Moinelo, Alejandro, Carraro, Francesco, Cherubini, Giovanni, Cosi, Massimo, Dami, Michele, De Nino, Maurizio, Del Vento, Davide, Di Giampietro, Marco, Donati, Alessandro, Dupuis, Olivier, Espinasse, Sylvie, Fabbri, Anna, Fave, Agnes, Veltroni, Iacopo Ficai, Filacchione, Gianrico, Garceran, Katia, Ghomchi, Yamina, Giustini, Maurizio, Gondet, Brigitte, Hello, Yann, Henry, Florence, Hofer, Stefan, Huntzinger, Gerard, Kachlicki, Juergen, Knoll, René, Driss, Kouach, Mazzoni, Alessandro, Melchiorri, Riccardo, Mondello, Giuseppe, Monti, Francesco, Neumann, Christian, Nuccilli, Fabrizio, Parisot, Jerome, Pasqui, Claudio, Perferi, Stefano, Peter, Gisbert, Piacentino, Alain, Pompei, Carlo, Reess, Jean Michel, Rivet, Jean Pierre, Romano, Antonio, Russ, Natalie, Santoni, Massimo, Scarpelli, Adelmo, Semery, Alain, Soufflot, Alain, Stefanovitch, Douchane, Suetta, Enrico, Tarchi, Fabio, Tonetti, Nazzareno, Tosi, Federico, Ulmer, Bernd

Publikováno v: Nature
Nature, Nature Publishing Group, 2007, 450, pp.637-640. ⟨10.1038/nature06209⟩
Nature, 2007, 450, pp.637-640. ⟨10.1038/nature06209⟩
Nature (Lond.) 450 (2007): 637–640. doi:10.1038/nature06209
info:cnr-pdr/source/autori:Piccioni G.,1; P. Drossart,4; A. Sanchez-Lavega,5; R. Hueso,5; F. W. Taylor,6; C. F. Wilson,6; D. Grassi,4; L. Zasova,7;,M. Moriconi,2; A. Adriani,3; S. Lebonnois,8; A. Coradini,3; B. Bezard,4; F. Angrilli,9; G. Arnold,10; K. H. Baines,11; G. Bellucci,3;J. Benkhoff,10; J. P. Bibring,12; A. Blanco,13;M.I.Blecka,14;R. W. Carlson,11; A. Di Lellis,15; T. Encrenaz,4;S. Erard,4;S. Fonti,13; V. Formisano,3; T. Fouchet,4; R. Garcia,16; R. Haus,10; J. Helbert,10; N. I. Ignatiev,7; P. G. J. Irwin,6; Y. Langevin,12;M. A. Lopez-Valverde,17; D. Luz,4,19; L. Marinangeli,18; V. Orofino,13; A. V. Rodin,7; M. C. Roos-Serote,19; B. Saggin,20;D. M. Stam,21; D. Titov,22; G. Visconti,23; M. Zambelli,1/titolo:South-polar features on Venus similar to those near the North Pole/doi:10.1038%2Fnature06209/rivista:Nature (Lond.)/anno:2007/pagina_da:637/pagina_a:640/intervallo_pagine:637–640/volume:450

Venus has no seasons, slow rotation and a very massive atmosphere, which is mainly carbon dioxide with clouds primarily of sulphuric acid droplets. Infrared observations by previous missions to Venus revealed a bright 'dipole' feature surrounded by a

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