The Space Roar is an anomalous radio signal first discovered by
NASA's Goddard Space Flight Center via the balloon-borne ARCADE
(Absolute Radiometer for Cosmology, Astrophysics, and Diffuse
Emission) instrument on July 22nd, 2006, and formally announced on January 7th,
2009 at the American Astronomical Society in Long Beach,
California. The unexplained signal was found to be six times louder
than the combined emissions of all known radio sources in the
universe—sources which further analysis has likewise eliminated as
potential origins for the signal.
ARCADE was initially designed
for the purpose of observing heat signs from the earliest generation of
primordial stars. The first instrument of its kind capable of detecting
such a signal, ARCADE's precision and sensitivity is produced, in part,
through the use of over 500 gallons of superfluid liquid helium; at
2.7° K, the instrument's temperature matches that of the
cosmic microwave background, eliminating its potential to contaminate
data received by ARCADE’s seven radiometers. Ironically, it was that
accuracy which allowed ARCADE to perceive the Space Roar signal, the
intensity of the noise effectively obscuring anything else it may have
found.
Sources
- "NASA Balloon Mission Tunes in to a Cosmic Radio Mystery" by Francis Reddy, NASA (January 7th, 2009)
- "Mystery Roar from Faraway Space Detected" by Andrea Thompson, SPACE (January 7th, 2009)
- "Absolute Radiometer for Cosmology, Astrophysics, and Diffuse Emission" NASA