My two-year-old loves radio telescopes. My friends are convinced that I trained my son Günther to point to and…
Dr. Kristina Nyland was a postdoctoral research associate at the National Radio Astronomy Observatory from 2015 to 2018. She has…
The NRAO-led National and International Non-Traditional Exchange (NINE) Program, part of the NRAO Office of Diversity and Inclusion, trains…
Astronomy has shown us striking images of galaxies, star clusters, and vast glowing nebula. But for many scientists, that…
Last June 2018, a group of astronomy educators, under the auspices of the National Science Foundation’s Astronomy in Chile…
Radio astronomy and amateur radio have a close historical connection, and one theme of the hamfest VLA tour is…
How do we know what’s going on in protoplanetary disks? Visible light telescopes don’t reveal much, because the thick…
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Aerial Shot of the Long Wavelength Array
Looking down on the 256 white, tent-shaped antennas of the Long Wavelength Array (LWA). Like the Very Large Array, the LWA combines the views of its individual antennas into impressive radio images of the sky. Unlike the VLA, however, the LWA antennas cannot dip or turn. To image different parts of the sky, the antennas rely on sophisticated electronics, software, and their four-sided faces. The LWA is tuned to natural radio waves that are below the range of manmade FM radio broadcast channels to observe pulsars, the Sun and its effects on the planets, and the most distant stars and galaxies in the Universe. In addition, the LWA also studies the radio-bouncing layer of our atmosphere, called the ionosphere.
Dark Energy has become the largest factor in the equations that may govern the Universe.
