File:NH-Pluto-Atmosphere-ArtistConcept-20140911.jpg
原始文件 (1,041 × 650像素,文件大小:288 KB,MIME类型:image/jpeg)
摘要
描述NH-Pluto-Atmosphere-ArtistConcept-20140911.jpg |
English: Sep. 11, 2014 - Atmosphere of Pluto (artist concept)
Artist’s impression of Pluto, with its wispy atmosphere. Artist’s impression of Pluto, with its wispy atmosphere. Data from New Horizons’ Alice ultraviolet spectrograph will answer a full range of questions about the composition and structure of that atmosphere. Randy Gladstone New Horizons Co-Investigator
What is Pluto’s atmosphere like? It seems like I’ve been wondering about that for decades! We’ve known so little for so long about Pluto’s atmosphere – other than it’s low-pressure, made mostly of molecular nitrogen (with a little methane and carbon monoxide mixed in) and may be quite extended – it’s nice to realize that we’ll know a whole lot more after New Horizons visits in summer 2015. My professional interests on New Horizons lie with Pluto’s upper atmosphere – what it’s made of, how it interacts with space, and how it is processed by sunlight into different gases and aerosols. A problem in planning atmospheric observations for New Horizons during the flyby is that we really don’t know what to expect. Only a few models have been made that try to predict the composition of Pluto’s atmosphere, and they don’t agree very much with each other because of the many present uncertainties. So our plans generally include a lot of survey-type observations, where we try not to assume too much about what we will detect, but are ready for anything. The best example of this is the Pluto solar occultation observation. The Alice ultraviolet spectrograph will watch the Sun set (and then rise again) as New Horizons flies through Pluto’s shadow, about an hour after closest approach. Watching how the different colors of sunlight fade (and then return) as New Horizons enters (and leaves) the shadow will tell us nearly all we could ask for about composition (all gases have unique absorption signatures at the ultraviolet wavelengths covered by Alice) and structure (how the absorption features vary with altitude will tell us about temperatures, escape rates and possibly about dynamics and clouds). When the New Horizons data start coming down, these are the data I’ll be waiting for the most!
|
日期 | |
来源 | http://www.nasa.gov/sites/default/files/thumbnails/image/nh-atmosphere.jpg |
作者 | NASA |
许可协议
Public domainPublic domainfalsefalse |
本文件完全由NASA创作,在美国属于公有领域。根据NASA的版权方针,NASA的材料除非另有声明否则不受版权保护。(参见Template:PD-USGov/zh、NASA版权方针页面或JPL图片使用方针。) | ||
警告:
|
此文件中描述的项目
描繪內容
19 3 2015
文件历史
点击某个日期/时间查看对应时刻的文件。
日期/时间 | 缩略图 | 大小 | 用户 | 备注 | |
---|---|---|---|---|---|
当前 | 2015年7月11日 (六) 17:35 | 1,041 × 650(288 KB) | Drbogdan | User created page with UploadWizard |
文件用途
以下2个页面使用本文件:
全域文件用途
以下其他wiki使用此文件:
- sr.wikipedia.org上的用途
元数据
此文件中包含有扩展的信息。这些信息可能是由数码相机或扫描仪在创建或数字化过程中所添加。
如果此文件的源文件已经被修改,一些信息在修改后的文件中将不能完全反映出来。
宽度 | 919 px |
---|---|
高度 | 574 px |
每色彩组分位数 |
|
像素构成 | RGB |
方向 | 正常 |
色彩组分数 | 3 |
水平分辨率 | 220 dpi |
垂直分辨率 | 220 dpi |
使用软件 | Adobe Photoshop CS6 (Macintosh) |
文件修改日期时间 | 2015年3月19日 (四) 13:21 |
Exif版本 | 2.21 |
色彩空间 | 未标定 |
原始文件唯一ID | 5048ED14AA54950A67275C214E51C571 |
数字化日期时间 | 2015年3月19日 (四) 09:18 |
元数据最后修改日期 | 2015年3月19日 (四) 09:21 |