File:NGC 6886.jpg
Original file (672 × 672 pixels, file size: 253 KB, MIME type: image/jpeg)
Captions
Summary
editDescriptionNGC 6886.jpg |
English: Astronomers have used the NASA/ESA Hubble Space Telescope to image the tiny planetary nebula NGC 6886. These celestial objects signal the final death throes of mid-sized stars (up to about eight times the mass of the Sun); when such a star exhausts its supply of hydrogen fuel, the outer layers begin to expand and cool, which creates an envelope of gas and dust that shrouds the dying star. However, the star doesn't go down without a fight, finding alternative ways to prevent it from collapsing under its own gravity and emerging as a white dwarf. In the process, the star's surface temperature increases and it is eventually hot enough to emit strong ultraviolet radiation and make the cocoon of gas glow as a stunning planetary nebula.
Stellar death isn't quick and painless: the planetary nebula stage typically lasts several tens of thousands of years. By studying the elements that are present in the nebula today, astronomers can determine the original chemical make-up of the star. Studies suggest that the star belonging to NGC 6886 may have originally been similar to the Sun, containing similar quantities of carbon, nitrogen and neon, although heavier elements, such as sulphur, were less plentiful. Keen amateur astronomers with mid-level telescopes will find it a rewarding challenge to track down NGC 6886 in the small constellation of Sagitta. It is tiny, but not particularly faint: high magnification, a good chart, a dark site and averted vision are needed to spot this elusive celestial jewel. This picture was created by combining images taken using the Wide Field Planetary Camera 2 on Hubble. Filters that let through emission from ionised nitrogen gas (F658N, coloured red), ionised oxygen (F502N, coloured blue) and a broadband yellow filter (F555W, coloured green, and also contributing to the blue) were used. The exposure times were 700 s, 600 s and 320 s respectively. The field of view is merely 30 arcseconds across. |
|||
Date | ||||
Source | http://www.spacetelescope.org/images/potw1102a/ | |||
Author | ESA/Hubble & NASA | |||
Permission (Reusing this file) |
This file is licensed under the Creative Commons Attribution 4.0 International license. Attribution: ESA/Hubble
|
File history
Click on a date/time to view the file as it appeared at that time.
Date/Time | Thumbnail | Dimensions | User | Comment | |
---|---|---|---|---|---|
current | 13:13, 20 April 2019 | 672 × 672 (253 KB) | Kesäperuna (talk | contribs) | 100% Quality JPEG from Tiff source. | |
16:56, 21 January 2011 | 672 × 672 (33 KB) | Jmencisom (talk | contribs) | {{Information |Description={{en|1=Astronomers have used the NASA/ESA Hubble Space Telescope to image the tiny planetary nebula NGC 6886. These celestial objects signal the final death throes of mid-sized stars (up to about eight times the mass of the Sun) |
You cannot overwrite this file.
File usage on Commons
The following 2 pages use this file:
File usage on other wikis
The following other wikis use this file:
- Usage on ar.wikipedia.org
- Usage on az.wikipedia.org
- Usage on be.wikipedia.org
- Usage on bs.wikipedia.org
- Usage on ce.wikipedia.org
- Usage on de.wikipedia.org
- Usage on diq.wikipedia.org
- Usage on en.wikipedia.org
- Usage on eo.wikipedia.org
- Usage on eu.wikipedia.org
- Usage on fa.wikipedia.org
- Usage on fr.wikipedia.org
- Usage on hr.wikipedia.org
- Usage on it.wikipedia.org
- Usage on kk.wikipedia.org
- Usage on ko.wikipedia.org
- Usage on kw.wikipedia.org
- Usage on lb.wikipedia.org
- Usage on mk.wikipedia.org
- Usage on nl.wikipedia.org
- Usage on pl.wikipedia.org
- Usage on pt.wikipedia.org
- Usage on ru.wikipedia.org
- Usage on si.wikipedia.org
- Usage on sk.wikipedia.org
- Usage on sl.wikipedia.org
- Usage on sr.wikipedia.org
- Usage on tr.wikipedia.org
- Usage on tt.wikipedia.org
- Usage on uk.wikipedia.org
- Usage on uz.wikipedia.org
- Usage on www.wikidata.org
- Usage on zh.wikipedia.org