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Keywords: planetary nebula, NGC 7293
![M2 9: крылья туманности Бабочка](https://images.astronet.ru/pubd/2004/02/01/0001196423/m2-9_hst.preview.jpg)
31.01.2004
Are stars better appreciated for their art after they die? Actually, stars usually create their most artistic displays as they die. In the case of low-mass stars like our Sun and M2-9 pictured above, the stars transform themselves from normal stars to white dwarfs by casting off their outer gaseous envelopes.
![Гало вокруг туманности Гантель](https://images.astronet.ru/pubd/2003/07/25/0001191751/m27ha_gendler_c1.preview.jpg)
25.07.2003
In 1764, French astronomer Charles Messier sighted this gorgeous cosmic cloud which he described as an oval nebula without stars. Cataloged as M27, it is now popularly known as the Dumbbell Nebula...
![M27: это не комета](https://images.astronet.ru/pubd/2004/04/24/0001197795/m27_vlt_f1_sm.preview.jpg)
24.04.2004
While searching the skies above 18th century France for comets, astronomer Charles Messier diligently recorded this object as number 27 on his list of things which are definitely not comets. So what is it?
![Наблюдения туманности Улитка на телескопах Бланко и Хаббл](https://images.astronet.ru/pubd/2004/12/30/0001201626/helix_hst.preview.jpg)
28.12.2004
How did a star create the Helix nebula? The shapes of planetary nebula like the Helix are important because they likely hold clues to how stars like the Sun end their lives. Recent observations...
![Планетарная туманность Красный Паук](https://images.astronet.ru/pubd/2002/08/25/0001179300/ngc6537_hst.preview.jpg)
24.07.2001
Oh what a tangled web a planetary nebula can weave. The Red Spider Planetary Nebula shows the complex structure that can result when a normal star ejects its outer gases and becomes a white dwarf star.
![NGC 2346: планетарная туманность в форме бабочки](https://images.astronet.ru/pubd/2001/11/02/0001172424/ngc2346_heritage.preview.jpg)
28.10.2001
It may look like a butterfly, but it's bigger than our Solar System. NGC 2346 is a planetary nebula made of gas and dust that has evolved into a familiar shape. At the heart of the bipolar planetary nebula is a pair of close stars orbiting each other once every sixteen days.
![Планетарная туманность Mz3: туманность Муравей](https://images.astronet.ru/pubd/2005/05/03/0001205445/mz3_hst.preview.jpg)
1.05.2005
Why isn't this ant a big sphere? Planetary nebula Mz3 is being cast off by a star similar to our Sun that is, surely, round. Why then would the gas that is streaming away create an ant-shaped nebula that is distinctly not round?
![NGC 6826: Мигающий Глаз](https://images.astronet.ru/pubd/2001/05/26/0001168383/ngc6826_hst.preview.jpg)
26.05.2001
The colorful planetary nebula phase of a sun-like star's life is brief. Almost in the "blink of an eye" - cosmically speaking - the star's outer layers are cast off, forming an expanding emission nebula. This nebula lasts perhaps 10 thousand years compared to a 10 billion year stellar life span.
![IC 418: Туманность Спирографа](https://images.astronet.ru/pubd/2000/12/19/0001162437/spirograph_heritage_big.preview.jpg)
7.09.2000
What is creating the strange texture of IC 418? Dubbed the Spirograph Nebula for its resemblance to drawings from a cyclical drawing tool, planetary nebula IC 418 shows patterns that are not well understood. Perhaps they are related to chaotic winds from the variable central star, which changes brightness unpredictably in just a few hours.
![IC 418: Туманность Спирограф](https://images.astronet.ru/pubd/2002/12/14/0001181294/spirograph_heritage.preview.jpg)
13.12.2002
What is creating the strange texture of IC 418? Dubbed the Spirograph Nebula for its resemblance to drawings from a cyclical drawing tool, planetary nebula IC 418 shows patterns that are not well understood. Perhaps they are related to chaotic winds from the variable central star, which changes brightness unpredictably in just a few hours.
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