NGC 891 is an edge-on spiral galaxy located some 10 million light years away in the direction of the constellation of Andromeda. NGC 891 has a large dust lane that is typical of spiral galaxies. It is often studied as a model of the Milky Way, as it is thought to be quite similar to our home galaxy.

This composite image was obtained using the 200-inch Hale Telescope's Wide-field Infrared Camera at Palomar Observatory and the 10-meter W.M. Keck Observatory's Low Resolution Imaging Spectrograph. Yellow colors in this composite correspond to the near-infrared image which was obtained at Palomar. The blue colors correspond to the visible light image which was obtained at Keck.

This kind of representation is useful because it demonstrates the utility of observing at many wavelengths. Because the central bulge of NGC 891 appears yellow in the composite, it is clear that the infrared does a better job penetrating the dust lane of this galaxy, which almost completely obscures the bulge in the optical image.

Previous                     Next