Astrophysics (Index)About

GUSTO

(Galactic / Extragalactic ULDB Spectroscopic Terahertz Observatory)
(balloon-borne 0.9-m far-infrared telescope)

GUSTO (for Galactic / Extragalactic ULDB Spectroscopic Terahertz Observatory, ULDB for Ultralong-Duration Balloon) is a balloon-borne 0.9-meter far infrared reflector telescope in development for a flight over Antarctica of 2-4 months at about 120,000 feet. It was launched December 31, 2023. It has a cryogenically-cooled three-channel camera, to map oxygen, nitrogen and carbon lines in the Milky Way and Large Magellanic Cloud (LMC). It builds on two previous such missions to test the concept, STO (for Spectroscopic Terahertz Observatory) in 2012, and STO2 in 2016.


(telescope,reflector,airborne,infrared,construction)
Further reading:
https://en.wikipedia.org/wiki/GUSTO_(telescope)
https://science.nasa.gov/mission/gusto/
https://ui.adsabs.harvard.edu/abs/2018cosp...42E.304B/abstract
https://ui.adsabs.harvard.edu/abs/2022SPIE12190E..0EW/abstract
https://www.jhuapl.edu/news/news-releases/170329-nasa-selects-apl-mission-untangle-complexities-interstellar-medium
https://www.sron.nl/missions-astrophysics/gusto
https://www.hou.usra.edu/meetings/landscape2019/pdf/5019.pdf
https://www.foxweather.com/earth-space/balloon-tracker-world-space-gusto
https://stratocat.com.ar/fichas-e/2023/MCM-20231231.htm
https://stratocat.com.ar/globos/2023e.htm
https://stratocat.com.ar/bases/41e.htm
WaveLFreqPhoton
Energy
  
64μm4.7THz19meVbeginGUSTO
214μm1.4THz5.8meVendGUSTO

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