The energy is visible in microwave wavelengths, which means it can't be seen unless you're above the atmosphere somewhere. But observations taken for spacecraft caught something extraordinary: a remarkably uniform background about 2.275 degrees Celsius (36 degrees Fahrenheit) above absolute zero, or the coldest possible temperature allowed by physics. Mapping and understanding the tiny variations of temperature at the part per million level that require ongoing observations and modeling.
Scientists have observed the CMB before with spacecraft, and even a specially adapted 747 called SOFIA (Stratospheric Observatory for Infrared Astronomy). A proposal published in the Monthly Notices of the Royal Astronomical Society suggests using an airship called Airlander 10, which is cheaper than a spacecraft, but allows for lengthy observations of up to weeks at a time.
"The main advantage is flight duration," Stephen Feeney, lead author and a postdoctoral researcher at the Flatiron Institute's Center for Computational Astrophysics in New York City, told Seeker in an email.
"Using remote piloting, Airlander 10 should fly for up to three weeks at a time,” he said. “We could therefore observe the sky roughly 20 times longer on an Airlander 10 flight than using, for example, a 747 like SOFIA. Airlander 10 is also able to operate without an airport, and should have a significantly smaller environmental impact, as it generates 60 percent of its lift through buoyancy."
"We are currently working with Hybrid Air Vehicles, Airlander 10's designers, to ascertain whether the vibrations from Airlander 10's engines are low enough to allow a CMB telescope to gather useful data,” Feeney said. “If this critical criterion is satisfied, we will look to develop the concept further.”
Feeney's research, in part, concerns how to operate CMB detectors at higher altitudes, which requires knowledge of how they perform at sea level, then extrapolating their performance at higher and higher altitudes. The research also seeks to ways to avoid confusing radiation from galaxies, which are closer to us than the CMB. Both galaxies and CMB can emit radiation at the same wavelengths.
"These foregrounds can be cleaned from the CMB by observing the sky at many different wavelengths, as the amplitudes of the foregrounds and CMB change differently with wavelength," Feeney said.
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