A collaborative French-Chinese satellite was launched on Saturday, marking a significant instance of cooperation between a Western nation and China. The mission aims to investigate the universe's most powerful explosions. The Space Variable Objects Monitor (SVOM), engineered by teams from both countries, is designed to detect gamma-ray bursts. These bursts are ancient light signals that have traversed billions of light years to reach Earth.
The satellite, weighing
930 kilograms and equipped with four instruments—two French and two Chinese—was
launched at approximately 3 PM from the Xichang space base in Sichuan province,
aboard a Chinese Long March 2-C rocket. This event was observed by journalists
present at the site.
Gamma-ray bursts are
typically triggered by the cataclysmic explosion of massive stars, those
exceeding 20 times the mass of the sun, or by the merging of compact stars.
These bursts emit extraordinarily bright cosmic beams, releasing energy on a
scale that surpasses the combined output of a billion billion suns. Observing
these bursts allows scientists to "look back in time," according to
Ore Gottlieb, an astrophysicist at the Flatiron Institute’s Center for
Astrophysics in New York, because the light from these events takes a considerable
amount of time to reach us.
The gamma rays, as they
travel through space, carry with them clues about the gas clouds and galaxies
they encounter, providing valuable data that can enhance our understanding of
the universe's history and evolution. Gottlieb emphasized that SVOM has the
potential to solve many enigmas related to gamma-ray bursts, including
detecting the most distant bursts in the universe, which correspond to the
earliest ones. The most remote gamma-ray bursts detected so far occurred just
630 million years after the Big Bang, a period when the universe was still very
young.
Frederic Daigne, an
astrophysicist at the Institut d’Astrophysique de Paris, highlighted the
intrinsic interest in gamma-ray bursts due to their nature as extreme cosmic
explosions. These events offer critical insights into the processes involved in
the death of certain stars, thereby deepening our comprehension of stellar life
cycles.
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