The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is supporting Intuitive Machines’ second lunar mission, IM-2, which landed on the surface of the Moon, Thursday, March 6th.
Recent News
Next-Generation Very Large Array Antenna Design to be Used By German Astronomers
The U.S. National Science Foundation National Radio Astronomy Observatory has announced a significant collaboration with the Bavarian State Government to construct a cutting-edge radio telescope atop Germany’s highest mountain. This radio telescope will use the design of the proposed NSF NRAO’s Next Generation Very Large Array (ngVLA).
NSF VLA Contributes Crucial Puzzle Piece to ‘Peculiar’ High Energy Transient
High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.
Listen to the Music of a Dying Star
The ALMA Music Box, currently on display in Japan, now available on iTunes
R Sculptoris, a massive red giant star located roughly 1000 light-years away in the constellation of Sculptor, is in the final stages of its life, and is violently expelling massive amounts of gas into space as it depletes its supply of fuel.
The ALMA Music Box plays musical disks inscribed with information from ALMA’s observations of this dying star, based on images taken at 70 different radio frequencies. The Music Box, a collaboration between the National Astronomical Observatory of Japan, PARTY New York, and Qosmo, plays 70 musical disks, each corresponding to a different radio frequency observation. The disks feature holes corresponding to points of intensity in the emission.
The ALMA Music Box will be on display at the 21st Century Museum of Contemporary Art, Kanazawa, Japan until November 15, 2015. The exhibition also features a miniature model of a Japanese 12-meter ALMA antenna and two receiver cartridges, which are installed into the antennas to receive radio waves.
The exhibition’s success recently prompted the production of the crowd-funded compilation CD “Music for a Dying Star.” This audio set features an assortment of melodies from the box integrated into original tracks from 11 international artists, including Taeji Sawai, Takagi Masakatsu, Throwing a Spoon, and Christian Fennesz.
“Music for a Dying Star” can now be purchased in the iTunes store for $14.88. More information about the ALMA Music Box and the CD is available on the CD’s dedicated website.
More information
ALMA, an international astronomy facility, is a partnership of ESO, the U.S. National Science Foundation (NSF) and the National Institutes of Natural Sciences (NINS) of Japan in cooperation with the Republic of Chile.
Recent News
Space Company Taps Coast-to-Coast Radio Telescopes for Moon Mission
The U.S. National Science Foundation National Radio Astronomy Observatory (NSF NRAO) is supporting Intuitive Machines’ second lunar mission, IM-2, which landed on the surface of the Moon, Thursday, March 6th.
Next-Generation Very Large Array Antenna Design to be Used By German Astronomers
The U.S. National Science Foundation National Radio Astronomy Observatory has announced a significant collaboration with the Bavarian State Government to construct a cutting-edge radio telescope atop Germany’s highest mountain. This radio telescope will use the design of the proposed NSF NRAO’s Next Generation Very Large Array (ngVLA).
NSF VLA Contributes Crucial Puzzle Piece to ‘Peculiar’ High Energy Transient
High-energy transient signals are most often determined to be gamma-ray burst events, but the recently-launched Einstein Probe has expanded astronomers’ ability to quickly respond to similar signals occurring at X-ray wavelengths. Now, a multi-wavelength study of EP240408a concludes that while many of the signal’s characteristics might lead to the conclusion that it is a gamma-ray burst, the non-detection at radio wavelengths precludes that possibility.