GSTDTAP  > 气候变化
DOI10.1029/2018GL078161
Limits on Dione's Activity Using Cassini/CIRS Data
Howett, Carly J. A.1; Spencer, John R.1; Hurford, Terry2; Verbiscer, Anne3; Segura, Marcia2
2018-06-28
发表期刊GEOPHYSICAL RESEARCH LETTERS
ISSN0094-8276
EISSN1944-8007
出版年2018
卷号45期号:12页码:5876-5898
文章类型Article
语种英语
国家USA
英文摘要

We use nighttime Cassini Composite Infrared Spectrometer (CIRS) data to look for discrete regions of elevated nighttime temperatures indicative of endogenic activity on Dione's surface. This is achieved by producing low latitude and midlatitude (less than 60 degrees) maps of Dione's nighttime surface temperature, derived from 10 to 1,100-cm(-1) CIRS data. The surface temperatures observed do not show evidence of any small discrete regions of elevated nighttime temperatures and are comparable to temperatures predicted by a passive thermophysical model of Dione's surface. Thus, we conclude that no evidence for activity exists on Dione at midlatitude to low latitude. Using the derived surface temperature maps, we set upper limits for the temperature at which a 50-, 100-, or 200-km(2) hot spot would remain undetected by this study. We find the mean temperature of such a hot spot would be 117.147.2K (-249F), 104.827.7K (-272F), and 95.419.5K (-288F) for a 50-, 100-, and 200-km(2) hot spot, respectively, corresponding to endogenic emission of 1.07, 0.68, and 0.47GW.


Plain Language Summary We use data from National Aeronautics and Space Administration's Cassini spacecraft to map the nighttime surface temperature of one of its large icy moons Dione. These maps show no evidence of small very hot regions, which (if present) would provide evidence of activity on Dione. Instead, the surface temperatures we do see are comparable with those we would expect to see on Dione if it were inactive. So we find no evidence for activity on Dione in this study. However, it is possible that very small regions of high surface temperatures would not be detected in this work. We use the observed surface temperatures to define how hot a small region (50, 100, or 200km(2)) could be and remain undetected. The results show such a region would have a mean temperature of 117.147.2K (-249F), 104.8 +/- 27.7K (-272F), and 95.4 +/- 19.5K (-288F) for a 50-, 100-, and 200-km(2) hot spot, respectively, corresponding to endogenic emission of 1.07, 0.68, and 0.47GW.


英文关键词Dione activity CIRS
领域气候变化
收录类别SCI-E
WOS记录号WOS:000438499100009
WOS关键词SATURN SYSTEM ; ICY SATELLITES ; SOUTH-POLE ; ENCELADUS ; VIMS ; RHEA ; IDENTIFICATION ; SPECTROMETER ; TEMPERATURE ; ATMOSPHERE
WOS类目Geosciences, Multidisciplinary
WOS研究方向Geology
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/26648
专题气候变化
作者单位1.Southwest Res Inst, Boulder, CO 80302 USA;
2.Godard Space Flight Ctr, Greenbelt, MD USA;
3.Univ Virginia, Dept Astron, Charlottesville, VA 22903 USA
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Howett, Carly J. A.,Spencer, John R.,Hurford, Terry,et al. Limits on Dione's Activity Using Cassini/CIRS Data[J]. GEOPHYSICAL RESEARCH LETTERS,2018,45(12):5876-5898.
APA Howett, Carly J. A.,Spencer, John R.,Hurford, Terry,Verbiscer, Anne,&Segura, Marcia.(2018).Limits on Dione's Activity Using Cassini/CIRS Data.GEOPHYSICAL RESEARCH LETTERS,45(12),5876-5898.
MLA Howett, Carly J. A.,et al."Limits on Dione's Activity Using Cassini/CIRS Data".GEOPHYSICAL RESEARCH LETTERS 45.12(2018):5876-5898.
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