The (Almost) Invisible Aftermath of a Massive Star's Death
Sig06 012c

Credit: NASA/JPL-Caltech/P. Morris (NHSC)

Observation • May 10th, 2006 • sig06-012c

sig06-012c

For the universe's biggest stars, even death is a show. Massive stars typically end their lives in explosive cataclysms, or supernovae, flinging abundant amounts of hot gas and radiation into outer space. Remnants of these dramatic deaths can linger for thousands of years and be easily detected by professional astronomers.

However, not all stars like attention. Thirty thousand light-years away in the Cepheus constellation, astronomers think they've found a massive star whose death barely made a peep. Remnants of this shy star's supernova would have gone completely unnoticed if the super-sensitive eyes of NASA's Spitzer Space Telescope hadn't accidentally stumbled upon it.

Unlike most supernova remnants, which are detectable at a variety of wavelengths ranging from radio to X-rays, this source only shows up in mid-infrared images taken by Spitzer's Multiband Imaging Photometer (MIPS). The remnant can be seen as a red-orange blob at the center of the picture. Although companion visible-light and near-infrared images capture the exact same region of space, the source is completely invisible in both pictures.

Astronomers suspect that the remnant's elusiveness is due to its location away from our Milky Way galaxy's dusty main disk, which contains most of the galaxy's stars. A supernova is most noticeable when the material expelled during the star's furious death throes violently collides with surrounding dust. Since the shy star sits away from the galaxy's dusty and crowded disk, the hot gas and radiation it flung into space had little surrounding material to crash into. Thus, it is largely invisible at most wavelengths. MIPS did not need dust to see the remnant. The mid-infrared instrument was able to directly detect the oxygen-rich gas from the supernova's explosive death throes.

In this image, starlight captured at 4.5 microns is represented in blue, 8-micron light from dust is green and light from 24 microns in red. The image combines the Spitzer infrared array camera data with the multiband imaging photometer data.

About the Object

Name
SSTGFLS J222557+601148
Type
Nebula > Type > Supernova Remnant
Distance
30,000 Light Years

Color Mapping

Band Wavelength Telescope
Infrared 4.5 µm Spitzer IRAC
Infrared 8.0 µm Spitzer IRAC
Infrared 24.0 µm Spitzer MIPS

Astrometrics

Position (J2000)
RA =22h 25m 36.2s
Dec = 60° 11' 49.9"
Field of View
6.6 x 6.3 arcminutes
Orientation
North is 75.9° right of vertical