Discovery of temperate latitude clouds on Titan

被引:62
作者
Roe, HG
Bouchez, AH
Trujillo, CA
Schaller, EL
Brown, ME
机构
[1] CALTECH, Div Geol & Planetary Sci, Pasadena, CA 91125 USA
[2] WM Keck Observ, Kamuela, HI 96743 USA
[3] Gemini Observ, Hilo, HI 96720 USA
基金
美国国家科学基金会; 澳大利亚研究理事会;
关键词
infrared : solar system; planets and satellites : individual (Titan);
D O I
10.1086/427499
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
Until now, all the clouds imaged in Titan's troposphere have been found at far southern latitudes (60degrees-90degrees south). The occurrence and location of these clouds is thought to be the result of convection driven by the maximum annual solar heating of Titan's surface, which occurs at summer solstice (2002 October) in this south polar region. We report the first observations of a new recurring type of tropospheric cloud feature, confined narrowly to similar to40degrees south latitude, which cannot be explained by this simple insolation hypothesis. We propose two classes of formation scenario, one linked to surface geography and the other to seasonally evolving circulation, which will be easily distinguished with continued observations over the next few years.
引用
收藏
页码:L49 / L52
页数:4
相关论文
共 12 条
[1]   Statistics of Titan's south polar tropospheric clouds [J].
Bouchez, AH ;
Brown, ME .
ASTROPHYSICAL JOURNAL, 2005, 618 (01) :L53-L56
[2]  
BOUCHEZ AH, 2003, THESIS CALTECH
[3]   Direct detection of variable tropospheric clouds near Titan's south pole [J].
Brown, ME ;
Bouchez, AH ;
Griffith, CA .
NATURE, 2002, 420 (6917) :795-797
[4]   Detection of daily clouds on Titan [J].
Griffith, CA ;
Hall, JL ;
Geballe, TR .
SCIENCE, 2000, 290 (5491) :509-513
[5]   Transient clouds in Titan's lower atmosphere [J].
Griffith, CA ;
Owen, T ;
Miller, GA ;
Geballe, T .
NATURE, 1998, 395 (6702) :575-578
[6]   Progress on Altair:: The Gemini North Adaptive Optics System [J].
Herriot, G ;
Morris, S ;
Anthony, A ;
Derdall, D ;
Duncan, D ;
Dunn, J ;
Ebbers, A ;
Fletcher, JM ;
Hardy, T ;
Leckie, B ;
Mirza, A ;
Morbey, C ;
Pfleger, M ;
Roberts, S ;
Shott, P ;
Smith, M ;
Saddlemyer, L ;
Sebesta, J ;
Szeto, K ;
Wooff, B ;
Windels, W ;
Véran, JP .
ADAPTIVE OPTICAL SYSTEMS TECHNOLOGY, PTS 1 AND 2, 2000, 4007 :115-125
[7]   The Gemini Near-Infrared Imager (NIRI) [J].
Hodapp, KW ;
Jensen, JB ;
Irwin, EM ;
Yamada, H ;
Chung, R ;
Fletcher, K ;
Robertson, L ;
Hora, JL ;
Simons, DA ;
Mays, W ;
Nolan, R ;
Bec, M ;
Merrill, M ;
Fowler, AM .
PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF THE PACIFIC, 2003, 115 (814) :1388-1406
[8]   Pillow lava on Titan: Expectations and constraints on cryovolcanic processes [J].
Lorenz, RD .
PLANETARY AND SPACE SCIENCE, 1996, 44 (09) :1021-1028
[9]   Thermodynamics of geysers: Application to Titan [J].
Lorenz, RD .
ICARUS, 2002, 156 (01) :176-183
[10]   Titan's clouds from Gemini and Keck adaptive optics imaging [J].
Roe, HG ;
de Pater, I ;
Macintosh, BA ;
McKay, CP .
ASTROPHYSICAL JOURNAL, 2002, 581 (02) :1399-1406