Spitzer and Hubble View of NGC 2207 and IC 2163
Ssc2006 11b1

Credit: NASA, ESA/JPL-Caltech/STScI/D. Elmegreen (Vassar)

Observation • April 26th, 2006 • ssc2006-11b1

ssc2006-11b1

These shape-shifting galaxies have taken on the form of a giant mask. The icy blue eyes are actually the cores of two merging galaxies, called NGC 2207 and IC 2163, and the mask is their spiral arms. The false-colored image consists of infrared data from NASA's Spitzer Space Telescope (red) and visible data from NASA's Hubble Space Telescope (blue/green).

NGC 2207 and IC 2163 met and began a sort of gravitational tango about 40 million years ago. The two galaxies are tugging at each other, stimulating new stars to form. Eventually, this cosmic ball will come to an end, when the galaxies meld into one. The dancing duo is located 140 million light-years away in the Canis Major constellation.

The infrared data from Spitzer highlight the galaxies' dusty regions, while the visible data from Hubble indicates starlight. In the Hubble-only image (not pictured here), the dusty regions appear as dark lanes.

The Hubble data correspond to light with wavelengths of .44 and .55 microns (blue and green, respectively). The Spitzer data represent light of 8 microns.

About the Object

Name
NGC 2207IC2163
Type
Galaxy > Type > Spiral
Galaxy > Type > Interacting
Galaxy > Grouping > Pair
Distance
140,000,000 Light Years
Redshift
0.0091

Color Mapping

Band Wavelength Telescope
Optical 440 nm Hubble ACS
Optical 550 nm Hubble ACS
Infrared 8.0 µm Spitzer IRAC

Astrometrics

Position (J2000)
RA =6h 16m 25.1s
Dec = -21° 22' 35.7"
Field of View
4.8 x 2.5 arcminutes
Orientation
North is 190.7° right of vertical