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Кольцевая Планетарная Туманность Shapley 1 Shapley 1: An Annular Planetary Nebula
25.06.2000

What happens when a star runs out of nuclear fuel? The center condenses into a white dwarf while the outer atmospheric layers are expelled into space and appear as a planetary nebula. This particular planetary nebula, designated Shapley 1 after the famous astronomer Harlow Shapley, has a very apparent annular ring like structure.



Шепли-1: кольцеобразная планетарная туманность Shapley 1: An Annular Planetary Nebula
14.02.1997

What happens when a star runs out of nuclear fuel? The center condenses into a white dwarf while the outer atmospheric layers are expelled into space and appear as a planetary nebula. This particular planetary nebula, designated Shapley 1 after the famous astronomer Harlow Shapley, has a very apparent annular ring like structure.



NGC 4361: планетарная туманность в форме галактики NGC 4361: Galaxy Shaped Planetary Nebula
28.12.1995

Glowing in the red light emitted by hydrogen atoms, the planetary nebula NGC 4361 is pictured above. The nebula itself is formed by the outer layers of gas shrugged off by the central star visible in the image.



Кольцеобразная планетарная туманность Шепли-1 Shapley 1: An Annular Planetary Nebula
9.08.1998

What happens when a star runs out of nuclear fuel? The center condenses into a white dwarf while the outer atmospheric layers are expelled into space and appear as a planetary nebula. This particular planetary nebula, designated Shapley 1 after the famous astronomer Harlow Shapley, has a very apparent annular ring like structure.



Шепли 1: кольцевая планетарная туманность Shapley 1: An Annular Planetary Nebula
16.08.2011

What happens when a star runs out of nuclear fuel? For stars about the mass of our Sun, the center condenses into a white dwarf while the outer atmospheric layers are expelled into space and appear as a planetary nebula.



Чудная планетарная туманность NGC 5189 NGC 5189: A Strange Planetary Nebula
10.12.1995

After a Sun-like star can no longer support fusion in its core, the center condenses into a white dwarf while the outer atmospheric layers are expelled into space and appear as a planetary nebula. This particular planetary nebula has a quite strange and chaotic structure.



Кольцеобразная туманность Шепли-1 Shapley 1: An Annular Planetary Nebula
11.12.1995

This strange structure is what can result when a normal star runs out of nuclear fuel in its core. At that time, the center condenses into a white dwarf while the outer atmospheric layers are expelled into space and appear as a planetary nebula.



Планетарная туманность Бабочка The Butterfly Planetary Nebula
21.10.1997

As stars age, they throw off their outer layers. Sometimes a highly symmetric gaseous planetary nebula is created, as is the case in M2-9, also called the Butterfly. Most planetary nebulae show this bipolar appearance, although some appear nearly spherical.



Планетарная туманность NGC 7027 в инфракрасном свете Planetary Nebula NGC 7027 in Infrared
24.03.1998

NGC 7027 is one of the smallest known planetary nebulae. Even so, NGC 7027 is 14,000 times larger than the Earth-Sun distance. Planetary nebula are so named because the first few discovered appeared similar to planets. Planetary nebula are actually dying stars, though, that have recently run out of nuclear fuel.



Планетарная туманность Хаббл-5 The Hubble 5 Planetary Nebula
18.01.1998

The Hubble Double Bubble Planetary Nebula is bubbling over with excitement. More mundanely known as Hubble 5, this bipolar planetary nebula is being created by a hot wind of particles streaming away from the central star system.




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