File:NH-Pluto-Atmosphere-ArtistConcept-20140911.jpg
原始檔案 (1,041 × 650 像素,檔案大小:288 KB,MIME 類型: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 | |
來源 | http://www.nasa.gov/sites/default/files/thumbnails/image/nh-atmosphere.jpg |
作者 | NASA |
授權條款
Public domainPublic domainfalsefalse |
本作品由NASA創作,屬於公有領域。根據NASA的版權政策:“NASA的創作除非另有聲明否則不受版權保護。”(參見:Template:PD-USGov/zh,NASA版權政策或JPL圖像使用政策) | ||
警告:
|
在此檔案描寫的項目
描繪內容
19 3 2015
檔案歷史
點選日期/時間以檢視該時間的檔案版本。
日期/時間 | 縮圖 | 尺寸 | 使用者 | 備註 | |
---|---|---|---|---|---|
目前 | 2015年7月11日 (六) 17:35 | 1,041 × 650(288 KB) | Drbogdan | User created page with UploadWizard |
檔案用途
下列2個頁面有用到此檔案:
全域檔案使用狀況
以下其他 wiki 使用了這個檔案:
- sr.wikipedia.org 的使用狀況
詮釋資料
此檔案中包含其他資訊,這些資訊可能是由數位相機或掃描器在建立或數位化過程中所新增的。若檔案自原始狀態已被修改,一些詳細資料可能無法完整反映出已修改的檔案。
寬度 | 919 px |
---|---|
高度 | 574 px |
每像素位元 |
|
像素合成 | RGB |
方位 | 標準 |
像素數量 | 3 |
水平解析度 | 220 dpi |
垂直解析度 | 220 dpi |
使用軟體 | Adobe Photoshop CS6 (Macintosh) |
檔案修改日期時間 | 2015年3月19日 (四) 13:21 |
Exif 版本 | 2.21 |
色彩空間 | 顏色未校準 |
原始文件唯一識別碼 | 5048ED14AA54950A67275C214E51C571 |
數位化的日期時間 | 2015年3月19日 (四) 09:18 |
詮釋資料最後修改日期 | 2015年3月19日 (四) 09:21 |