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<p>of its mass was ejected in the event which created the planetary nebula. The luminosity and temperature of the star indicate it has ceased nuclear burning and is on its way to becoming a <a href="page.php?w=white_dwarf">white dwarf</a>, fading at a predicted rate of 1% per year.</p>

<p><big>Dust chemistry</big></p>
<p>The prominent dark lane that runs through the centre of the nebula has been shown to have an unusual composition, showing evidence for multiple crystalline silicates, crystalline water ice and <a href="page.php?w=quartz">quartz</a>, with</p><p>
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