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Chandra X-ray Image of
NGC 5315
(Credit: NASA/CXC/RIT/J. Kastner et al. )



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NGC 5315:
When Serendipity Becomes Science



Credit: NASA/CXC/RIT/J. Kastner et al.

NGC 5315 is a planetary nebula about 7,000 light years from Earth in the constellation of Circinus. Planetary nebulas are gaseous clouds that are created in the last stages of the lifetime of a star like the Sun. The name of "planetary nebula" is a misnomer, since these objects have nothing to do with planets. But the term was born because these objects look like planets when viewed through small optical telescopes. Chandra does not always see planetary nebulas in X-ray light. Rather, they may only become X-ray sources, like NGC 5315, when powerful winds from a particularly young star at the center collide with the ejected material.

This image of NGC 5315 shows the box-shaped outlines for two of the detectors on Chandra, plus the so-called aimpoint of the telescope, where the Chandra images are the sharpest (the spatial resolution of Chandra images, like those for other X-ray telescopes, descreases with distance from the aimpoint). For optimal imaging of Hen 2-99, Chandra was pointed so that this planetary nebula would fall near the aimpoint. Although Hen 2-99 was too faint to be detected, the planetary nebula NGC 5315 was serendipitously detected a large distance away from the aimpoint, where the image is not as sharp.

Fast Facts for NGC 5315:
Credit  NASA/CXC/RIT/J. Kastner et al.
Scale  Inset is approx. 5 arcmin across
Category  White Dwarfs & Planetary Nebulas
Coordinates (J2000)  RA 13 h 26m 08s | Dec -29d 52m 24s
Constellation  Circinus
Observation Date  November 12, 2003
Observation Time  8 hours
Obs. ID  4480
Color Code  Intensity
Instrument  ACIS
References Kastner, J.H. et al, 2007, ApJ, Accepted
Distance Estimate  About 7,000 light years
Release Date  September 27, 2007