File:Soap Bubble Nebula - Noao0904a.jpg

預覽大小：428 × 599 像素。其他解析度：171 × 240 像素 | 343 × 480 像素 | 548 × 768 像素 | 731 × 1,024 像素 | 2,500 × 3,500 像素。

原始檔案（2,500 × 3,500 像素，檔案大小：5.96 MB，MIME 類型：image/jpeg）

本檔案並非來自中文維基百科，而是來自維基共享資源。請參閱維基共享資源上的詳細描述、討論頁、頁面歷史、日誌。

維基共享資源是一個儲存自由版權作品的項目。您可以向此項目作出貢獻。

摘要

描述

English: Soap Bubble Nebula, PN G075.5+01.7

Informally known as the "Soap Bubble Nebula", this planetary nebula (officially known as PN G075.5+01.7) was discovered by amateur astronomer Dave Jurasevich on July 6th, 2008. It was noted and reported by Keith Quattrocchi and Mel Helm on July 17th, 2008. This image was obtained with the Kitt Peak Mayall 4-meter telescope on June 19th, 2009 in the H-alpha (orange) and [OIII] (blue) narrowband filters. In this image, north is to the left and east is down. PN PN G075.5+01.7 is located in the constellation of Cygnus, not far from the Crescent Nebula (NGC 6888). It is embedded in a diffuse nebula which, in conjunction with its faintness, is the reason it was not discovered until recently. The spherical symmetry of the shell is remarkable, making it very similar to Abell 39.

Credit:

T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOIRLab/NSF/AURA

日期

2013年2月12日

來源

https://noirlab.edu/public/images/noao0904a/

作者

Credit:

T.A. Rector (University of Alaska Anchorage) and H. Schweiker (WIYN and NOIRLab/NSF/AURA)

授權許可
(重用此檔案)

This media was created by the National Optical-Infrared Astronomy Research Laboratory (NOIRLab).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public NOIRLab website, along with the texts of press releases, announcements, images of the week and captions; are licensed under a Creative Commons Attribution 4.0 International License, and may on a non-exclusive basis be reproduced without fee provided the credit is clear and visible."
To the uploader: You must provide a link (URL) to the original file and the authorship information if available.

此檔案採用創用CC 姓名標示 4.0 國際授權條款。

您可以自由：

分享 – 複製、發佈和傳播本作品
重新修改 – 創作演繹作品

惟需遵照下列條件：

姓名標示 – 您必須指名出正確的製作者，和提供授權條款的連結，以及表示是否有對內容上做出變更。您可以用任何合理的方式來行動，但不得以任何方式表明授權條款是對您許可或是由您所使用。

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	用戶	備⁠註
目前	2021年11月22日 (一) 22:15		2,500 × 3,500（5.96 MB）	Fabian RRRR	== {{int:filedesc}} == {{Information \|description={{en\|1='''Soap Bubble Nebula, PN G75.5+1.7 Informally known as the "Soap Bubble Nebula", this planetary nebula (officially known as PN G75.5+1.7) was discovered by amateur astronomer Dave Jurasevich on July 6th, 2008. It was noted and reported by Keith Quattrocchi and Mel Helm on July 17th, 2008. This image was obtained with the Kitt Peak Mayall 4-meter telescope on June 19th, 2009 in the H-alpha (orange) and [OIII] (blue) narrowband filters....

檔案用途

下列頁面有用到此檔案：

泡泡星雲

全域檔案使用狀況

以下其他 wiki 使用了這個檔案：

af.wikipedia.org 的使用狀況
- Lys van planetêre newels
- Seepborrelnewel
de.wikipedia.org 的使用狀況
- Seifenblasen-Nebel
en.wikipedia.org 的使用狀況
- Soap Bubble Nebula
fr.wikipedia.org 的使用狀況
- Nébuleuse de la Bulle de savon
- Discussion:Listes de nébuleuses planétaires
ja.wikipedia.org 的使用狀況
- はくちょう座
pt.wikipedia.org 的使用狀況
- PN G75.5+1.7
ru.wikipedia.org 的使用狀況
- Мыльный Пузырь (туманность)
www.wikidata.org 的使用狀況
- Q1568725

詮釋資料

此檔案中包含擴展的資訊。這些資訊可能是由數位相機或掃描器在建立時或數位化過程中所加入。

如果此檔案的來源檔案已被修改，一些資訊在修改後的檔案中將不能完全反映出來。

影像標題	Informally known as the "Soap Bubble Nebula", this planetary nebula (officially known as PN G75.5+1.7) was discovered by amateur astronomer Dave Jurasevich on July 6th, 2008. It was noted and reported by Keith Quattrocchi and Mel Helm on July 17th, 2008. This image was obtained with the Kitt Peak Mayall 4-meter telescope on June 19th, 2009 in the H-alpha (orange) and [OIII] (blue) narrowband filters. In this image, north is to the left and east is down. PN G75.5+1.7 is located in the constellation of Cygnus, not far from the Crescent Nebula (NGC 6888). It is embedded in a diffuse nebula which, in conjunction with its faintness, is the reason it was not discovered until recently. The spherical symmetry of the shell is remarkable, making it very similar to Abell 39.
製作/提供者	T. A. Rector/University of Alaska Anchorage, H. Schweiker/WIYN and NOIRLab/NSF/AURA
來源	NSF's NOIRLab
簡稱	Soap Bubble Nebula, PN G75.5+1.7
使用條款	Creative Commons Attribution 4.0 International License
資料產生的日期時間	2009年10月15日 (四) 00:00
JPEG 檔案備註	Informally known as the "Soap Bubble Nebula", this planetary nebula (officially known as PN G75.5+1.7) was discovered by amateur astronomer Dave Jurasevich on July 6th, 2008. It was noted and reported by Keith Quattrocchi and Mel Helm on July 17th, 2008. This image was obtained with the Kitt Peak Mayall 4-meter telescope on June 19th, 2009 in the H-alpha (orange) and [OIII] (blue) narrowband filters. In this image, north is to the left and east is down. PN G75.5+1.7 is located in the constellation of Cygnus, not far from the Crescent Nebula (NGC 6888). It is embedded in a diffuse nebula which, in conjunction with its faintness, is the reason it was not discovered until recently. The spherical symmetry of the shell is remarkable, making it very similar to Abell 39.
使用軟體	Adobe Photoshop CS3 Macintosh
檔案修改日期時間	2009年7月21日 (二) 12:32
數位化的日期時間	2009年6月21日 (日) 06:38
詮釋資料最後修改日期	2009年7月21日 (二) 05:32
原始文件唯一識別碼	uuid:4214BC8EE25FDE11B9BBFA5BC186AA94
關鍵字	PN G75.5+1.7 Soap Bubble Nebula
聯絡資訊	https://noirlab.edu 950 North Cherry Ave. Tucson, AZ, 85719 USA
IIM 版本	4

File:Soap Bubble Nebula - Noao0904a.jpg

摘要

說明

在此檔案描寫的項目

描繪內容

著作權狀態 ^{繁體中文 (已轉換拼寫)}

有著作權 ^{繁體中文 (已轉換拼寫)}

特許條款

共享創意署名4.0國際

成立或建立時間

12 2 2013

多媒體型式 ^{繁體中文 (已轉換拼寫)}

image/jpeg

檔案歷史

檔案用途

全域檔案使用狀況

詮釋資料

摘要

說明

在此檔案描寫的項目

描繪內容

著作權狀態 繁體中文 (已轉換拼寫)

有著作權 繁體中文 (已轉換拼寫)

特許條款

共享創意署名4.0國際

成立或建立時間

12 2 2013

多媒體型式 繁體中文 (已轉換拼寫)

image/jpeg

檔案歷史

檔案用途

全域檔案使用狀況

詮釋資料

著作權狀態 ^{繁體中文 (已轉換拼寫)}

有著作權 ^{繁體中文 (已轉換拼寫)}

多媒體型式 ^{繁體中文 (已轉換拼寫)}