These images show four fine examples of "planetary nebulae" - glowing gas
that surrounds a very hot compact stars that represents the distant
future of our Sun.
Once stars like our Sun have exhausted all of their available fuel, they
expand to huge diameters (as big as the orbit of the Earth). Then, their
outer layers are gently ejected into space. The remnant hot core energizes
the surrounding gas, producing the planetary nebula. This is a very brief
phase - lasting just 100,000 years, after which the nebula disperses and the
core cools. In these images, the greenish tinge is given by the light of
glowing oxygen gas, while red signifies the light from hydrogen.
These four examples show the variety of shapes and sizes that planetary
nebulae can display. The reason why they are so asymmetrical remains a
mystery... the solution to which will give us details on the circumstances
surrounding their central stars' demise.