Our Swift satellite just detected its 1,500th gamma-ray burst! 🛰💥 This powerful explosion was observed on Oct. 23 in the constellation Ursa Major. To celebrate, let’s explore 3 other extra-special Swift observations from over 16 years of science. 🥳
Soon after launch, Swift was the first to spy a short gamma-ray burst with an afterglow — GRB 050509B lasted only 0.03 seconds! ⏱ Other telescopes followed up to continue the hunt for the cause of these bursts, later confirmed to be neutron star mergers. go.nasa.gov/2ZruPGO
Nearly all gamma-ray bursts have to be observed with telescopes. But in 2008, Swift caught a burst so powerful that its afterglow was briefly visible without any magnification. GRB 080319B may be the most distant object visible to unaided eyes! 👁 More: go.nasa.gov/3mePTIY
In 2009, Swift saw a 10-second-long gamma-ray burst that turned out to be the most distant cosmic explosion seen so far. The star that created GRB 090423 died when the universe was only 630 million years old, or less than 5% of its present age. 👶 More: go.nasa.gov/3BfpW03
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The Burst Alert Telescope, or BAT, on our Swift satellite just surpassed 1 million triggers! 🎉 The BAT constantly watches for gamma-ray bursts — powerful but fleeting explosions signaling a black hole’s birth. 💥 Get up to speed on gamma-ray bursts here: tmblr.co/Zz_Uqj2aNmOwb
☑️ The BAT’s onboard algorithms review each trigger to see if it’s a cosmic source or a statistical fluctuation. In sifting through those many triggers, Swift’s BAT has detected about 1,400 bona fide bursts along with a number of other notable discoveries.
👀 Let’s look at some.
The initial flash in some gamma-ray bursts lasts less than two seconds, making it hard to lock on to them for follow-up observations. ⏱️ Swift was designed to do just that and pinpointed its first “short” gamma-ray burst afterglow in May 2005. Learn more: go.nasa.gov/371jmip
#OTD in 2008, @NASA’s Fermi Gamma-ray Space Telescope began its science operations. In these 12 years, Fermi helps open our eyes to better understand some of the most powerful cosmic sources like these:
On Aug 4, 2017, Fermi detected a powerful, short gamma-ray burst located 130 million light-years away. Those gamma rays had friends! @NSF’s LIGO also detected gravitational waves from this pair of colliding neutron stars. go.nasa.gov/31lcAzw
Almost every day Fermi detects gamma-ray bursts lasting from a fraction of a second to over 1,000 seconds. Many of these events signal the birth of a black hole. nasa.tumblr.com/post/176492220…
This week, the stars of Eta Carinae made their closest approach — about the distance between Mars & the Sun — to each other occurring every 5.5 years. As the most massive, radiant & unstable star system within 10,000 light-years, it could even be the next bright supernova.
The larger of the two stars in Eta Carinae is a luminous blue variable about 90 times the mass of our Sun. Though rare now, we think these “superstars” were common in the early universe, when they were fundamental in forming the first black holes.
The smaller star (about 30 times the mass of the Sun) is outshone by its larger companion making it tough to directly detect. But it has found a way to make itself known! Its stellar wind collides with the wind of its comrade which creates very hot gas and a strong X-ray signal.