A mosaic of images from WISE in the constellation of Cassiopeia. This region contains a large star-forming nebula within the Milky Way Galaxy, called IC 1805 (sometimes called the Heart Nebula), a portion of which is seen at the right of the image. Also visible in this image are two nearby galaxies, Maffei 1 and Maffei 2. In visible light, these galaxies are hidden by dust from IC 1805; they were unknown until 1968, when Paolo Maffei found them using infrared observations. Both galaxies contain billions of stars and are located some 10 million light-years away (well outside our own Milky Way Galaxy). Maffei 1 is the bluish elliptical object in the center of the image. It is a Lenticular-type galaxy, which has a disk-like structure and a central bulge but no spiral structure or appreciable dust content. Maffei 2 (to the upper left of Maffei 1) is a Spiral type galaxy that also has a disk shape, but with a bar-like central bulge and two prominent dusty spiral arms.
The image size is about 1.6 by 4.5 degrees (by comparison, the full Moon is about 0.5 degrees across). Blue light represents 3.4 & 4.6 micron channels, dominated by starlight; green is 12 microns; and red is the 22 micron channel, which is dominated by infrared emission from warm interstellar dust.