ファイル:Pillars of Creation (NIRCam and MIRI Composite Image) (pillarsofcreation composite).jpeg
ページのコンテンツが他言語でサポートされていません。
表示
このプレビューのサイズ: 640 × 599 ピクセル。 その他の解像度: 256 × 240 ピクセル | 820 × 768 ピクセル | 1,094 × 1,024 ピクセル | 2,188 × 2,048 ピクセル | 7,130 × 6,675 ピクセル。
元のファイル (7,130 × 6,675 ピクセル、ファイルサイズ: 9.77メガバイト、MIME タイプ: image/jpeg)
ウィキメディア・コモンズのファイルページにある説明を、以下に表示します。
|
概要
解説Pillars of Creation (NIRCam and MIRI Composite Image) (pillarsofcreation composite).jpeg |
English: By combining images of the iconic Pillars of Creation from two cameras aboard the NASA/ESA/CSA James Webb Space Telescope, the Universe has been framed in its infrared glory. Webb’s near-infrared image was fused with its mid-infrared image, setting this star-forming region ablaze with new details.Myriad stars are spread throughout the scene. The stars primarily show up in near-infrared light, marking a contribution of Webb’s Near-Infrared Camera (NIRCam). Near-infrared light also reveals thousands of newly formed stars – look for bright orange spheres that lie just outside the dusty pillars.In mid-infrared light, the dust is on full display. The contributions from Webb’s Mid-Infrared Instrument (MIRI) are most apparent in the layers of diffuse, orange dust that drape the top of the image, relaxing into a V. The densest regions of dust are cast in deep indigo hues, obscuring our view of the activities inside the dense pillars.Dust also makes up the spire-like pillars that extend from the bottom left to the top right. This is one of the reasons why the region is overflowing with stars – dust is a major ingredient of star formation. When knots of gas and dust with sufficient mass form in the pillars, they begin to collapse under their own gravitational attraction, slowly heat up, and eventually form new stars. Newly formed stars are especially apparent at the edges of the top two pillars – they are practically bursting onto the scene.At the top edge of the second pillar, undulating detail in red hints at even more embedded stars. These are even younger, and are quite active as they form. The lava-like regions capture their periodic ejections. As stars form, they periodically send out supersonic jets that can interact within clouds of material, like these thick pillars of gas and dust. These young stars are estimated to be only a few hundred thousand years old, and will continue to form for millions of years.Almost everything you see in this scene is local. The distant universe is largely blocked from our view both by the interstellar medium, which is made up of sparse gas and dust located between the stars, and a thick dust lane in our Milky Way galaxy. As a result, the stars take center stage in Webb’s view of the Pillars of Creation.The Pillars of Creation is a small region within the vast Eagle Nebula, which lies 6,500 light-years away.Revisit Webb’s near-infrared image and its its mid-infrared image. The Pillars of Creation was made famous by the NASA/ESA Hubble Space Telescope in 1995, and again in 2014.MIRI was contributed by ESA and NASA, with the instrument designed and built by a consortium of nationally funded European Institutes (The MIRI European Consortium) in partnership with JPL and the University of Arizona.Webb’s NIRCam was built by a team at the University of Arizona and Lockheed Martin’s Advanced Technology Center.[Image Description: Semi-opaque layers of blue, purple, and grey gas and dust start at the bottom left and rise toward the top right. There are three prominent pillars. The left pillar is the largest and widest. The background is orange near the top and dark blue and purple near the bottom. Some blue and white stars dot the overall scene.] |
日付 | 2022年11月30日, 18:25 (アップロード日) |
原典 | Pillars of Creation (NIRCam and MIRI Composite Image) |
作者 | NASA, ESA, CSA, STScI, J. DePasquale (STScI), A. Pagan (STScI), A. M. Koekemoer (STScI) |
その他のバージョン |
|
ライセンス
ESA/Webb images, videos and web texts are released by the ESA under the Creative Commons Attribution 4.0 International license and may on a non-exclusive basis be reproduced without fee provided they are clearly and visibly credited. Detailed conditions are below; see the ESA copyright statement for full information. For images created by NASA or on the webbtelescope.org website, use the {{PD-Webb}} tag.
Conditions:
Notes:
|
このファイルはクリエイティブ・コモンズ 表示 4.0 国際ライセンスのもとに利用を許諾されています。
帰属: NASA, ESA, CSA, STScI, J. DePasquale (STScI), A. Pagan (STScI), A. M. Koekemoer (STScI)
- あなたは以下の条件に従う場合に限り、自由に
- 共有 – 本作品を複製、頒布、展示、実演できます。
- 再構成 – 二次的著作物を作成できます。
- あなたの従うべき条件は以下の通りです。
- 表示 – あなたは適切なクレジットを表示し、ライセンスへのリンクを提供し、変更があったらその旨を示さなければなりません。これらは合理的であればどのような方法で行っても構いませんが、許諾者があなたやあなたの利用行為を支持していると示唆するような方法は除きます。
image/jpeg
ファイルの履歴
過去の版のファイルを表示するには、その版の日時をクリックしてください。
日付と時刻 | サムネイル | 寸法 | 利用者 | コメント | |
---|---|---|---|---|---|
現在の版 | 2022年12月11日 (日) 21:46 | 7,130 × 6,675 (9.77メガバイト) | OptimusPrimeBot | #Spacemedia - Upload of https://cdn.esawebb.org/archives/images/large/pillarsofcreation_composite.jpg via Commons:Spacemedia |
ファイルの使用状況
以下のページがこのファイルを使用しています:
グローバルなファイル使用状況
以下に挙げる他のウィキがこの画像を使っています:
- en-two.iwiki.icu での使用状況
メタデータ
このファイルには、追加情報があります (おそらく、作成やデジタル化する際に使用したデジタルカメラやスキャナーが追加したものです)。
このファイルが元の状態から変更されている場合、修正されたファイルを完全に反映していない項目がある場合があります。
作者 | Space Telescope Science Institute Office of Public Outreach |
---|---|
撮影著作権者/編集著作権者 |
|
帰属/提供者 | NASA, ESA, CSA, STScI, J. DePasquale (STScI), A. Pagan (STScI), A. M. Koekemoer (STScI) |
ソース | ESA/Webb |
短いタイトル |
|
画像の説明 |
|
使用条件 |
|
原画像データの生成日時 | 2022年11月30日 (水) 18:25 |
JPEGファイルのコメント | By combining images of the iconic Pillars of Creation from two cameras aboard the NASA/ESA/CSA James Webb Space Telescope, the Universe has been framed in its infrared glory. Webb’s near-infrared image was fused with its mid-infrared image, setting this star-forming region ablaze with new details. Myriad stars are spread throughout the scene. The stars primarily show up in near-infrared light, marking a contribution of Webb’s Near-Infrared Camera (NIRCam). Near-infrared light also reveals thousands of newly formed stars – look for bright orange spheres that lie just outside the dusty pillars. In mid-infrared light, the dust is on full display. The contributions from Webb’s Mid-Infrared Instrument (MIRI) are most apparent in the layers of diffuse, orange dust that drape the top of the image, relaxing into a V. The densest regions of dust are cast in deep indigo hues, obscuring our view of the activities inside the dense pillars. Dust also makes up the spire-like pillars that extend from the bottom left to the top right. This is one of the reasons why the region is overflowing with stars – dust is a major ingredient of star formation. When knots of gas and dust with sufficient mass form in the pillars, they begin to collapse under their own gravitational attraction, slowly heat up, and eventually form new stars. Newly formed stars are especially apparent at the edges of the top two pillars – they are practically bursting onto the scene. At the top edge of the second pillar, undulating detail in red hints at even more embedded stars. These are even younger, and are quite active as they form. The lava-like regions capture their periodic ejections. As stars form, they periodically send out supersonic jets that can interact within clouds of material, like these thick pillars of gas and dust. These young stars are estimated to be only a few hundred thousand years old, and will continue to form for millions of years. Almost everything you see in this scene is local. The distant universe is largely blocked from our view both by the interstellar medium, which is made up of sparse gas and dust located between the stars, and a thick dust lane in our Milky Way galaxy. As a result, the stars take center stage in Webb’s view of the Pillars of Creation. The Pillars of Creation is a small region within the vast Eagle Nebula, which lies 6,500 light-years away. Revisit Webb’s near-infrared image and its its mid-infrared image. The Pillars of Creation was made famous by the NASA/ESA Hubble Space Telescope in 1995, and again in 2014. |
使用ソフトウェア名 | Adobe Photoshop 24.0 (Macintosh) |
ファイル変更日時 | 2022年11月29日 (火) 15:48 |
デジタルデータの作成日時 | 2022年8月30日 (火) 10:10 |
メタデータの最終更新日 | 2022年11月29日 (火) 11:04 |
元文書の一意なID | xmp.did:279f8cb9-587e-484b-a2d1-36c6e80921d2 |
著作権情報 | 著作権情報未設定 |
キーワード |
|
連絡先情報 | outreach@stsci.edu
ESA Office, Space Telescope Science Institute, 3700 San Martin Dr Baltimore, MD, 21218 United States |
IIMバージョン | 4 |