Notebookcheck Logo

NASA’s StarBurst mission passes critical tests

NASA's StarBurst intrument outside a thermal vacuum chamber (Image source: NASA/Daniel Kocevski)
NASA's StarBurst intrument outside a thermal vacuum chamber (Image source: NASA/Daniel Kocevski)
NASA’s StarBurst mission has passed thermal and vibration tests and is now closer to being launch-ready. The mission will study some of the most powerful events in the universe — events from which heavy metals like gold and platinum form.

StarBurst is a NASA-led mission that is designed to detect the initial emission of short gamma-ray bursts produced from neutron star mergers. These gamma-ray bursts are among the most powerful explosions in the universe. Most of the heavy metals in the universe are formed from neutron star mergers. Gold and platinum are two of such metals that these powerful events give birth to.

Observatories on Earth already detect the gravitational waves from neutron star mergers. StarBurst is set to detect the gamma-rays simultaneously with the gravitational waves.

StarBurst passed its thermal and vibration testing at NASA Marshall. The thermal testing occurred in a vacuum chamber. This test simulated the hottest and coldest conditions the instrument will encounter during operations in space. The vibration testing simulated the vibration and turbulence that StarBurst will face during launch.

StarBurst is now awaiting instrument calibration as the next step towards launch readiness. NASA aims to launch StarBurst as early as 2027 during the next run of the Laser-Interferometer Gravitational Wave Observatory. This will maximize the chances of detecting gamma-ray bursts simultaneously with gravitational waves.

Astronomers have only observed one neutron star merger where a gamma-ray burst and gravitational waves were detected at the same time. With StarBurst, they expect to find up to 10 per year.

Source(s)

Please share our article, every link counts!
Mail Logo
Google Logo Add as a preferred
source on Google
static version load dynamic
Loading Comments
Comment on this article
Chibuike Okpara, 2026-01-15 (Update: 2026-01-15)