The Surface Age of Titan

نویسندگان

  • Ralf Jaumann
  • Gerhard Neukum
چکیده

Introduction: Since its arrival at the Saturnian system, the Cassini spacecraft has made about 100 Titan flybys. The surface of Titan has been revealed almost globally by the Cassini observations in the infrared and regionally to about 25% in radar wavelengths [1,2,3] as well as locally by the Huygens optical instruments [4]. Extended dune fields, lakes, distinct landscapes of volcanic and tectonic origin, dendritic erosion patterns and deposited erosional remnants exhibit a geologically active surface indicating significant endogenic and exogenic processes leading to dynamic surface alteration. Consequently, impact craters are rare on Titan [5,6,7,8].

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

منابع مشابه

Infestations of Piagetiella titan (Menoponidae: Mallophaga) on juvenile white pelicans (Pelecanus nocrotalus, L.) in Urmia Lake National Park, northwest Iran.

Pelecaniformes are large water birds feeding by hunting fish and living usually in the sea and in fresh water. Ectoparasitic lice of the genus Piagetiella are interesting from an ecological standpoint as they are found in the pouches of pelicans. Unlike chewing lice, which live on the body surface of the host, P. titan lives in the oral cavity of white pelicans (Pelecanus nocrotalus, L.). This ...

متن کامل

Assessing Cryovolcanic Resurfacing of Titan

Introduction: A quantitative assessment is made of " cryovolcanism " as a resurfacing process on the saturnian moon Titan. The geologically young surface of Titan indicates that much resurfacing has taken place. However, to date, there has been no unambigu-ous detection of active " cryovolcanism " , such as the emplacement of a " cryolava " flow. The dense Titan atmosphere makes this kind of ob...

متن کامل

Titan as a Laboratory for Linear Dune Formation

Introduction: Synthetic Aperture Radar images of Titan collected by the Cassini spacecraft show that dunes are abundant on Titan's surface, covering almost 20% of Titan's surface [1,2]. Nearly all of the dunes found on Titan are linear in form, are found near the equator (±30and have a west-east orientation. Since there is likely active linear dune formation presently on Titan [3], we can use T...

متن کامل

Relative rates of fluvial bedrock incision on Titan and Earth

[1] Observations of likely fluvial channels on the surface of Titan, along with Titan’s geologically youthful surface, motivate this study of comparative fluvial erosion rates on Titan and the Earth. The roles of bedload abrasion, suspended load abrasion, plucking, and cavitation are considered. Despite orders of magnitude differences in some of the physical parameters that control fluvial inci...

متن کامل

Discovery of Fog at the South Pole of Titan

While Saturn’s moon Titan appears to support an active methane hydrological cycle, no direct evidence for surface-atmosphere exchange has yet appeared. It is possible that the identified lake-features could be filled with ethane, an involatile long term residue of atmospheric photolysis; the apparent stream and channel features could be ancient from a previous climate; and the tropospheric meth...

متن کامل

ذخیره در منابع من


  با ذخیره ی این منبع در منابع من، دسترسی به آن را برای استفاده های بعدی آسان تر کنید

برای دانلود متن کامل این مقاله و بیش از 32 میلیون مقاله دیگر ابتدا ثبت نام کنید

ثبت نام

اگر عضو سایت هستید لطفا وارد حساب کاربری خود شوید

عنوان ژورنال:

دوره   شماره 

صفحات  -

تاریخ انتشار 2009