AAO image reference AAT 82. « Previous || Next »
Top left is NE. Image width is about 11 arc min
Image and text © 1993-2002, Anglo-Australian Observatory, photograph by David Malin.
Other planetary nebulae in this series of photographs show they can take a wide variety of shapes. Most show a distinctive and well marked symmetry, which can vary from more or less spherical, to doughnut-like annuli or to bi-polar, butterfly-like objects. Planetary nebulae also usually have well-defined boundaries, sometimes even a shell-like structure. For reasons that are not understood, NGC 1360 defies all these conventions, yet its colour still clearly identifies it as a planetary nebula. The green hue is oxygen, excited by the hot central star, and to the north-east of the nebula is a faint red smudge, probably traces of material ejected before the star became a true planetary nebula.
Entry from NGC 2000.0 (R.W. Sinnott, Ed.) © Sky Publishing Corporation, 1988:
NGC 1360 Pl 03 33.3 -25 51 s For6.5 *8 in B, L neb, E nsFor details of photographic exposure, search technical table by AAT reference number.