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Keyword: MyCn18
![MyCn18: планетарная туманность в форме песочных часов](https://images.astronet.ru/pubd/2015/05/10/0001336879/mycn18_hst_960.preview.jpg)
10.05.2015
The sands of time are running out for the central star of this hourglass-shaped planetary nebula. With its nuclear fuel exhausted, this brief, spectacular, closing phase of a Sun-like star's life occurs as its outer layers are ejected - its core becoming a cooling, fading white dwarf.
![MyCn18: туманность Песочные часы](https://images.astronet.ru/pubd/2011/08/07/0001253184/mycn18_hst_900.preview.jpg)
7.08.2011
The sands of time are running out for the central star of this hourglass-shaped planetary nebula. With its nuclear fuel exhausted, this brief, spectacular, closing phase of a Sun-like star's life occurs as its outer layers are ejected - its core becoming a cooling, fading white dwarf.
![Туманность "Песочные часы" MyCn18](https://images.astronet.ru/pubd/2002/08/24/0001179188/hst_hourglass_big.preview.gif)
18.01.1996
The sands of time are running out for the central star of this hourglass-shaped planetary nebula. With its nuclear fuel exhausted, this brief, spectacular, closing phase of a Sun-like star's life occurs as its outer layers are ejected - its core becoming a cooling, fading White Dwarf.
![MyCn18: туманность Песочные часы](https://images.astronet.ru/pubd/2003/08/15/0001192346/mycn18_hst_big.preview.gif)
14.09.1997
The sands of time are running out for the central star of this hourglass-shaped planetary nebula. With its nuclear fuel exhausted, this brief, spectacular, closing phase of a Sun-like star's life occurs as its outer layers are ejected - its core becoming a cooling, fading white dwarf.
![М15: плотное шаровое звездное скопление](https://images.astronet.ru/pubd/2001/03/15/0001166722/m15_hstheritage_big1.preview.jpg)
4.08.2000
Life might get dull at the core of M15 but the sky would always be bright with stars! In fact, only 40,000 light-years away in the constellation Pegasus, M15 is one of the most densely packed globular star clusters in our Milky Way Galaxy.
![MyCn18: Туманность Песочные Часы](https://images.astronet.ru/pubd/2001/03/15/0001166625/mycn18_hst_big.preview.jpg)
4.06.2000
The sands of time are running out for the central star of this hourglass-shaped planetary nebula. With its nuclear fuel exhausted, this brief, spectacular, closing phase of a Sun-like star's life occurs as its outer layers are ejected - its core becoming a cooling, fading White Dwarf.
![MyCn18: туманность в форме песочных часов](https://images.astronet.ru/pubd/2002/06/15/0001177356/MyCn18_hst.preview.jpg)
15.06.2002
The sands of time are running out for the central star of this hourglass-shaped planetary nebula. With its nuclear fuel exhausted, this brief, spectacular, closing phase of a Sun-like star's life occurs as its outer layers are ejected - its core becoming a cooling, fading white dwarf.
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