We have launched the new Spitzer website! Send feedback to outreach@ipac.caltech.edu. Find the old website at http://legacy.spitzer.caltech.edu.
Distant Galaxies and Origins of the Universe
Default banner 2
Distant Galaxies and Origins of the  Universe

Spitzer sees a galaxy sitting more than 13 billion light-years away as a red smudge above a bright nearby galaxy.

The Universe is expanding. This means that from Earth, astronomers see that the most distant galaxies seem to be moving away much faster than those that are close by. As a distant galaxy travels away from us, the wavelength of light that it emits stretches and is "redshifted" toward the infrared part of the electromagnetic spectrum. This means that a very distant galaxy emitting primarily visible or ultraviolet light will appear in infrared light by the time its light reaches Earth.

Our Universe is about 14 billion years old, and Spitzer spotted galaxies sitting more than 13 billion light-years away. This means that the light from these distant galaxies started traveling toward us when the Universe was still very young, only a few hundred million years old. Because the speed of light is finite, these distant objects are observed as they appeared when the Universe was much younger. By capturing this light, Spitzer provided valuable information about how and when the first objects in the Universe formed, ultimately giving us snapshots of the way things were.

Spitzer's supersensitive infrared eyes could also probe the cumulative infrared glow of countless unseen galaxies that are too faint to be detected individually. This allowed astronomers to interpret the history of star and galaxy formation, as well as the presence of dust in the earliest baby galaxies. Scientists refer to this glow as the cosmic infrared background.

Like sitting in a noisy room and not being able to make out a single conversation, the cosmic infrared background can be likened to the combination of all the room's sounds. Like a cosmic eavesdropper, Spitzer not only detected the Universe's infrared background "noise," it could also characterize some of the sources contributing to the noise, similar to making out and understanding a single conversation in the noisy room. This "talent" helped scientists understand how our modern Universe came to be.