This infrared light picture of the Small Magellanic Cloud galaxy was assembled using data from the Herschel Space Observatory, a European Space Agency-led mission, and NASA’s Spitzer Space Telescope. The Large and Small Magellanic Clouds are the two biggest satellite galaxies of our home galaxy. They are considered dwarf galaxies compared to the big spiral of the Milky Way.
By combining data from Herschel and Spitzer, the irregular distribution of dust in the Small Magellanic Cloud becomes clear. A stream of dust called the galaxy’s “wing” extends to the left in the picture, and a vertical line of star formation is on the right.
The colors in this image indicate temperatures in the dust in the Cloud. Regions where star formation is at its earliest stages or is shut off are cooler. Warm spot occur around new stars heating surrounding dust. The coldest areas and objects are red, corresponding to infrared light taken up by Herschel’s at 250 microns (A micron is 0.000001 m). Herschel 100 and 160 micron data shown in green indicates warmer areas.1 The warmest spots appear in blue and are derived from 24 and 70 micron data from Spitzer.
Image Credit: ESA/NASA/JPL