Tonight's Sky
Sun
Sun
Moon
Moon
Mercury
Mercury
Venus
Venus
Mars
Mars
Jupiter
Jupiter
Saturn
Saturn

Tonight's Sky — Change location

OR

Searching...

Tonight's Sky — Select location

Tonight's Sky — Enter coordinates

° '
° '

The universe's first light?

Scientists may have detected the faint glow of the first stars.
Spitzer CIB
After scientists subtracted the infrared light of stars, galaxies, and other artifacts from this 10-hour Spitzer exposure, the diffuse background was revealed. In this image, the gray splotches are where objects have been subtracted out, white shows the strongest infrared signal, and black the weakest.
NASA/JPL-Caltech/A. Kashlinsky (GSFC)
November 3, 2005
The earliest stars in the universe were massive — at least 100 times our Sun's mass — and burned their fuel quickly. They ended their lives just a few million years after their births, in huge explosions that left no direct way to detect them. However, ultraviolet light from these stars shifted to near-infrared in the universe's expansion and contributes to a large portion of the cosmic infrared background (CIB) radiation.

NASA's cosmic background explorer (COBE) detected a possible CIB signal in 1992. Scientists used NASA's Spitzer Space Telescope to analyze ripples in the infrared sky, in much the same way the Wilkinson Microwave Anisotropy Probe (WMAP) measured the ripples in the microwave sky. The Spitzer group then subtracted out all known infrared sources — stars, galaxies, and dust — and was left with a background of infrared fluctuations.

The infrared signal Spitzer detected is statistically similar in each of four wavelengths — 3.6, 4.5, 5.8, and 8 micrometers — so this cannot be noise in one particular channel. In addition, the signal did not change between two observations taken 6 months apart, therefore, this signal is independent of the solar system's zodiacal light (sunlight scattering off interplanetary dust in the elliptical plane, which changes direction depending on where Earth is during its path around the Sun).

Stars that lived roughly 100 million years after the Big Bang — when WMAP and computer simulations predict the first stars existed — would have had their light shifted to the wavelengths Spitzer imaged. "We think we are seeing the collective light from millions of the first objects to form in the universe," says Alexander Kashlinsky, lead author of the November 3 Nature letter.

The scientists did not see point sources of light, but the diffuse signal is likely the combined light emitted by the first stars. NASA's James Webb Space Telescope, expected to launch in 2013, will further analyze the CIB, dissecting it into individual objects.
0

JOIN THE DISCUSSION

Read and share your comments on this article
Comment on this article
Want to leave a comment?
Only registered members of Astronomy.com are allowed to comment on this article. Registration is FREE and only takes a couple minutes.

Login or Register now.
0 comments
ADVERTISEMENT

FREE EMAIL NEWSLETTER

Receive news, sky-event information, observing tips, and more from Astronomy's weekly email newsletter.

ADVERTISEMENT
ADVERTISEMENT
BoxProductcovernov

Click here to receive a FREE e-Guide exclusively from Astronomy magazine.

Find us on Facebook

Loading...