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National Aeronautics and Space Administration

Goddard Space Flight Center

Astrophysics Science Division | Sciences and Exploration

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ARCADE Instrument

Imagine standing outside on a cold winter night and trying to warm your hands by holding them out to the stars. Not a very warming prospect, is it? Now imagine that the stars are moved away from us, far from our Milky Way galaxy, and are instead located at the other end of space and time. That's the problem that the ARCADE team must address -- detecting the heating of the universe by the very first stars.

ARCADE must measure temperature differences as small as 1/1000 of a degree in a background only 3 degrees above absolute zero. The problem is not sensitivity, but confusion: everything else in the universe, including the Earth and the balloon payload, is hotter than the microwave background. Room temperature objects, for instance, are 100 times hotter than the microwaves ARCADE must observe, and 100,000 times hotter than the signal from the first stars. If ARCADE is to reliably measure the microwave background with accuracy of 0.001 K, the total contribution from the rest of the world must be made smaller than this limit.
Instrument schematic
ARCADE is designed to reduce or eliminate these unwanted "systematic errors" from the rest of the world:

  • The entire instrument is cooled with liquid helium to 2.7 degrees above absolute zero. If the instrument is the same temperature as the microwave background, it can not contaminate the signal.

  • The instrument has an unobstructed view to deep space, with nothing warm allowed between the antennas and the sky. If there are no warm objects in the beam, there will be no signal contamination.

  • The instrument uses multiple levels of comparison to eliminate any residual contamination. Each radiometer continuously compares the signal coming in through the antenna to a stable internal reference load. Each antenna alternately views the sky or a precision blackbody calibration target. All of the different frequency channels view the same target. Since the target is known to be a precise blackbody, by comparing the output when the antennas view the target to the output when the antennas view the sky, we can immediately tell whether or not the sky is also a blackbody.

    Additional Instrument Information


    Radiometers

    Radiometers

    Calibration Target

    Calibration Target

    Stupid Dewar Tricks

    Stupid Dewar Tricks