We have launched the new Spitzer website! Send feedback to outreach@ipac.caltech.edu. Find the old website at http://legacy.spitzer.caltech.edu.
Hubble View of Galaxy Merger II Zw 096
Sig10 023b

Credit: NASA/JPL-Caltech/STScI/H. Inami (SSC/Caltech)

Observation • November 18th, 2010 • sig10-023b

sig10-023b

The merging galaxies known collectively as II Zw 096 are shown in this image from NASA's Hubble Space Telescope. This rendering combines light spanning the far-ultraviolet into the near-infrared.

This galaxy merger is the site of a spectacular burst of star formation that is hinted at in the red speckles near the middle of the image. This dust-shrouded area conceals a brilliant burst of star formation that becomes more apparent at longer wavelengths of infrared light.

Researchers using infrared data from NASA's Spitzer Space Telescope estimate the starburst is cranking out stars at the breakneck pace of around 100 solar masses, or masses of our Sun, per year. They were surprised to see such a brilliant infrared glow in an area so far offset from the center of the spiral galaxy. Starbursts are often found crammed into the very centers of merging galaxies, but this is the brightest starburst ever seen outside a galaxy's nucleus.

This Hubble image represents far-ultraviolet light at a wavelength of 0.15 microns as blue, visible light at 0.44 microns as cyan, and near infrared light at 0.9 microns as red.

About the Object

Name
II Zw 096
Type
Galaxy > Type > Interacting
Galaxy > Type > Spiral
Galaxy > Activity > Starburst
Galaxy > Grouping > Pair
Distance
525,000,000 Light Years
Redshift
0.036

Color Mapping

Band Wavelength Telescope
UV 140 nm Hubble SBC
Optical 440 nm Hubble ACS
Infrared 900 nm Hubble ACS

Astrometrics

Position (J2000)
RA =20h 57m 24.3s
Dec = 17° 7' 40.3"
Field of View
1.5 x 1.5 arcminutes
Orientation
North is up