Academic Journal

The lakes of Titan

التفاصيل البيبلوغرافية
العنوان: The lakes of Titan
المؤلفون: E. R. Stofan, C. Elachi, J. I. Lunine, R. D. Lorenz, B. Stiles, K. L. Mitchell, S. Ostro, L. Soderblom, C. Wood, H. Zebker, S. Wall, M. Janssen, R. Kirk, R. Lopes, F. Paganelli, J. Radebaugh, L. Wye, Y. Anderson, M. Allison, R. Boehmer, P. Callahan, P. Encrenaz, E. Flamini, G. Francescetti, Y. Gim, G. Hamilton, S. Hensley, W. T. K. Johnson, K. Kelleher, D. Muhleman, P. Paillou, F. Posa, L. Roth, S. Shaffer, S. Vetrella, R. West, PICARDI, Giovanni, SEU, Roberto
المساهمون: E. R., Stofan, C., Elachi, J. I., Lunine, R. D., Lorenz, B., Stile, K. L., Mitchell, S., Ostro, L., Soderblom, C., Wood, H., Zebker, S., Wall, M., Janssen, R., Kirk, R., Lope, F., Paganelli, J., Radebaugh, L., Wye, Y., Anderson, M., Allison, R., Boehmer, P., Callahan, P., Encrenaz, E., Flamini, G., Francescetti, Y., Gim, G., Hamilton, S., Hensley, W. T. K., Johnson, K., Kelleher, D., Muhleman, P., Paillou, Picardi, Giovanni, F., Posa, L., Roth, Seu, Roberto, S., Shaffer, S., Vetrella, R., West
بيانات النشر: NATURE PUBLISHING GROUP
سنة النشر: 2007
المجموعة: Sapienza Università di Roma: CINECA IRIS
الوصف: The surface of Saturn's haze-shrouded moon Titan has long been proposed to have oceans or lakes, on the basis of the stability of liquid methane at the surface(1,2). Initial visible(3) and radar(4,5) imaging failed to find any evidence of an ocean, although abundant evidence was found that flowing liquids have existed on the surface(5,6). Here we provide definitive evidence for the presence of lakes on the surface of Titan, obtained during the Cassini Radar flyby of Titan on 22 July 2006 (T(16)). The radar imaging polewards of 70 degrees north shows more than 75 circular to irregular radar-dark patches, in a region where liquid methane and ethane are expected to be abundant and stable on the surface(2,7). The radar-dark patches are interpreted as lakes on the basis of their very low radar reflectivity and morphological similarities to lakes, including associated channels and location in topographic depressions. Some of the lakes do not completely fill the depressions in which they lie, and apparently dry depressions are present. We interpret this to indicate that lakes are present in a number of states, including partly dry and liquid-filled. These northern-hemisphere lakes constitute the strongest evidence yet that a condensable-liquid hydrological cycle is active in Titan's surface and atmosphere, in which the lakes are filled through rainfall and/or intersection with the subsurface 'liquid methane' table.
نوع الوثيقة: article in journal/newspaper
وصف الملف: ELETTRONICO
اللغة: English
Relation: info:eu-repo/semantics/altIdentifier/pmid/17203056; info:eu-repo/semantics/altIdentifier/wos/WOS:000243225100035; volume:445; issue:7123; firstpage:61; lastpage:64; numberofpages:4; journal:NATURE; http://hdl.handle.net/11573/69686; info:eu-repo/semantics/altIdentifier/scopus/2-s2.0-33846072871; http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000243225100035&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a; http://www.scopus.com/inward/record.url?eid=2-s2.0-33846072871&partnerID=65&md5=655f669be17b503f2c43135bebba395b
DOI: 10.1038/nature05438
الاتاحة: http://hdl.handle.net/11573/69686
https://doi.org/10.1038/nature05438
http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000243225100035&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a
http://www.scopus.com/inward/record.url?eid=2-s2.0-33846072871&partnerID=65&md5=655f669be17b503f2c43135bebba395b
رقم الانضمام: edsbas.6DD533F5
قاعدة البيانات: BASE