Saiz pralihat ini: 600 × 600 piksel. Leraian-leraian lain: 240 × 240 piksel | 480 × 480 piksel | 768 × 768 piksel | 1,024 × 1,024 piksel | 1,807 × 1,807 piksel.
Fail asli (1,807 × 1,807 piksel, saiz fail: 1.36 MB, jenis MIME: image/jpeg)
Ringkasan
| Keterangan |
English: This image, captured by ESO’s Very Large Telescope (VLT) at Paranal, shows a small part of the well-known emission nebula, NGC 6357, located some 8000 light-years away, in the tail of the southern constellation of Scorpius (The Scorpion). The image glows with the characteristic red of an H II region, and contains a large amount of ionised and excited hydrogen gas.
The cloud is bathed in intense ultraviolet radiation — mainly from the open star cluster Pismis 24, home to some massive, young, blue stars — which it re-emits as visible light, in this distinctive red hue. The cluster itself is out of the field of view of this picture, its diffuse light seen illuminating the cloud on the centre-right of the image. We are looking at a close-up of the surrounding nebula, showing a mesh of gas, dark dust, and newly born and still forming stars. |
| Tarikh | |
| Sumber | http://www.eso.org/public/images/potw1334a/ |
| Pengarang | ESO |
Perlesenan
_logo.svg){kind=logo} |
This media was created by the European Southern Observatory (ESO).
Their website states: "Unless specifically noted, the images, videos, and music distributed on the public ESO website, along with the texts of press releases, announcements, pictures of the week, blog posts 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. |
  Fail ini dilesenkan di bawah lesen Pengiktirafan 4.0 Antarabangsa Creative Commons.
| |
Sejarah fail
Klik pada tarikh/waktu untuk melihat rupa fail tersebut pada waktu itu.
| Tarikh/Waktu | Gambar kenit | Ukuran | Pengguna | Komen | |
|---|---|---|---|---|---|
| semasa | 13:15, 26 Ogos 2013 | | 1,807 × 1,807 (1.36 MB) | Stas1995 | User created page with UploadWizard |
Penggunaan fail
Laman berikut menggunakan fail ini:
Penggunaan fail sejagat
Fail ini digunakan oleh wiki-wiki lain yang berikut:
- Penggunaan di ar.teknopedia.teknokrat.ac.id
- Penggunaan di bg.wikipedia.org
- Penggunaan di bn.wikipedia.org
- Penggunaan di bs.wikipedia.org
- Penggunaan di cv.wikipedia.org
- Penggunaan di da.wikipedia.org
- Penggunaan di de.teknopedia.teknokrat.ac.id
- Penggunaan di en.wikipedia.org
- Penggunaan di es.teknopedia.teknokrat.ac.id
- Penggunaan di et.wikipedia.org
- Penggunaan di eu.wikipedia.org
- Penggunaan di fa.teknopedia.teknokrat.ac.id
- Penggunaan di fr.teknopedia.teknokrat.ac.id
- Penggunaan di he.wikipedia.org
- Penggunaan di hr.wikipedia.org
- Penggunaan di hy.wikipedia.org
- Penggunaan di teknopedia.teknokrat.ac.id
- Penggunaan di kn.wikipedia.org
- Penggunaan di mk.wikipedia.org
- Penggunaan di ro.wikipedia.org
- Penggunaan di simple.wikipedia.org
- Penggunaan di sk.wikipedia.org
- Penggunaan di tr.wikipedia.org
- Penggunaan di uk.wikipedia.org
- Penggunaan di zh-min-nan.wikipedia.org
- Penggunaan di zh.teknopedia.teknokrat.ac.id
