Saiz pralihat ini: 800 × 565 piksel. Leraian-leraian lain: 320 × 226 piksel | 640 × 452 piksel | 1,024 × 723 piksel | 1,280 × 904 piksel | 2,560 × 1,809 piksel | 6,500 × 4,592 piksel.
Fail asli (6,500 × 4,592 piksel, saiz fail: 13.38 MB, jenis MIME: image/jpeg)
Ringkasan
| Keterangan |
English: Born from clouds of gas and dust, stars like our Sun spend most of their lifetime slowly burning their primary nuclear fuel, hydrogen, into the heavier element helium. After leading this bright and shiny life for several billion years, their fuel is almost exhausted and they start swelling, pushing the outer layers away from what has turned into a small and very hot core. These “middle-aged” stars become enormous, hence cool and red — red giants. All red giants exhibit a slow oscillation in brightness due their rhythmic “breathing” in and out, and one third of them are also affected by additional, slower and mysterious changes in their luminosity. After this rapid and tumultuous phase of their later life, these stars do not end in dramatic explosions, but die peacefully as planetary nebulae, blowing out everything but a tiny remnant, known as white dwarf. |
| Tarikh | |
| Sumber | http://www.eso.org/public/images/eso0948a/ |
| Pengarang | ESO/S. Steinhöfel |
Perlesenan
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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.
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Sejarah fail
Klik pada tarikh/waktu untuk melihat rupa fail tersebut pada waktu itu.
| Tarikh/Waktu | Gambar kenit | Ukuran | Pengguna | Komen | |
|---|---|---|---|---|---|
| semasa | 11:33, 1 Jun 2013 | | 6,500 × 4,592 (13.38 MB) | Stas1995 | {{Information |Description ={{en|1=Born from clouds of gas and dust, stars like our Sun spend most of their lifetime slowly burning their primary nuclear fuel, hydrogen, into the heavier element helium. After leading this bright and shiny life for s... |
Penggunaan fail
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Penggunaan fail sejagat
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- Penggunaan di af.wikipedia.org
- Penggunaan di ar.teknopedia.teknokrat.ac.id
- Penggunaan di ast.wikipedia.org
- Penggunaan di bn.wikipedia.org
- Penggunaan di cs.wikipedia.org
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- Penggunaan di fa.teknopedia.teknokrat.ac.id
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- Penggunaan di it.teknopedia.teknokrat.ac.id
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- Penggunaan di no.wikipedia.org
- Penggunaan di pl.teknopedia.teknokrat.ac.id
- Penggunaan di si.wikipedia.org
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- Penggunaan di uk.wikipedia.org
- Penggunaan di war.teknopedia.teknokrat.ac.id
- Penggunaan di zh-yue.wikipedia.org
- Penggunaan di zh.teknopedia.teknokrat.ac.id
