astro.wikisort.org - Nebula
The Cotton Candy Nebula is an astronomical object in the constellation of Scorpius. It is considered to fall into an unusual category of nebulae known as protoplanetary nebulae or post-AGB stars.[1] A proto-planetary nebulae is an astronomical object that is in a stellar evolution phase where the star begins to discard its outer layers and is about to proceed to becoming a true planetary nebula, which is another astronomical object made up mostly of gaseous materials that was originally discovered by the IRAS satellite. IRAS was launched in January 1982 and overlooked about 97 percent of the sky.[2] It is also known as IRAS 17150-3224. It is a good example of a DUPLEX-type protoplanetary nebula.[3]
| Reflection nebula | |
|---|---|
| Protoplanetary nebula | |
 The Cotton Candy Nebula as seen by the Hubble Space Telescope | |
| Observation data: epoch | |
| Right ascension | 17h 18m 20s |
| Declination | −32° 27′ 22″ |
| Constellation | Scorpius |
The Cotton Candy Nebula is difficult to spot considering it is only 16′′ long and hardly shines. Michael E. Bakich is an Astronomy senior editor and has studied the Cotton Candy Nebula. He has confirmed that the way to spot the nebula is with the help of a 16'' scope.[1] With the help of the IRAS 17150-3224 and the nebulae being in the perfect position where the starlight is blocked, we were able to examine the ring-like structures that "cocoon" the nebula as astronomer Sun Kwok put it.[2] The spherical ring structures around the nebulae are created throughout the red-giant stage which is the ultimate stage in stellar evolution.[2]
References
- Bakich, Michael (May 2010). "Target 30 obscure celestial gems: this list of faint, fainter, and faintest deep-sky targets will take your observing skills to the next level". Astronomy: 64 – via gale in context biography.
- Kwok, Sun (October 1998). "Stellar metamorphosis" (PDF). Sky & Telescope: 30 – via Gale Biography in Context.
- HST polarimetry of PPN
Constellation of Scorpius | |||||||||||||
|---|---|---|---|---|---|---|---|---|---|---|---|---|---|
| |||||||||||||
| Stars |
| ||||||||||||
| |||||||||||||
| Star clusters |
| ||||||||||||
| Nebulae |
| ||||||||||||
| Galaxies |
| ||||||||||||
 Category | |||||||||||||
 |
Wikimedia Commons has media related to Cotton Candy Nebula. |
 | This nebula-related article is a stub. You can help Wikipedia by expanding it. |
На других языках
[de] IRAS 17150-3224
IRAS 17150-3224 im englischen auch Cotton Candy Nebula ist ein a präplanetarischer Nebel im Sternbild Altar, der mithilfe des IRAS-Satelliten entdeckt wurde.- [en] Cotton Candy Nebula
[ru] Туманность Сахарная Вата
Туманность «Сахарная Вата» — протопланетарная туманность, связанная со звездой, находящейся на стадии после асимптотической ветви гигантов.[3] Протопланетарная туманность представляет собой астрономический объект на такой стадии звёздной эволюции, при которой звезда начинает сбрасывать внешние слои и постепенно переходит к стадии планетарной туманности. Впервые наблюдалась космическим аппаратом IRAS. IRAS был запущен в январе 1982 года и впоследствии наблюдал около 97% неба.[4] Объект также известен как IRAS 17150-3224. Туманность является примером протопланетной туманности типа DUPLEX.[5]Другой контент может иметь иную лицензию. Перед использованием материалов сайта WikiSort.org внимательно изучите правила лицензирования конкретных элементов наполнения сайта.
WikiSort.org - проект по пересортировке и дополнению контента Википедии