Asteroid Explodes “Bomb-Like” Over France in Rare Event

Asteroids Fragmenting in Unforeseen Ways

Wikimedia/CC-BY-SA-4.0

A rare asteroid explosion occurred in France two years ago, raising alarms regarding the planet’s defense against certain rocky bodies.

On February 13, 2023, a small asteroid named 2023 CX1 entered Earth’s atmosphere, creating a streak across the Normandy sky. This event marked one of the rare instances of meteors monitored before atmospheric entry, happening approximately 7 hours ago.

Bright fireballs resulted from the event, with multiple meteorites collected from the ground. Only two asteroids were monitored, and debris was recovered from their descent. The second one was located in Germany in 2024.

Analysis of footage capturing the asteroid’s descent by Aurian Egal from Western University of Ontario and her team revealed remarkable findings. While most asteroids disintegrate upon entering Earth’s atmosphere, the 2023 CX1 maintained its integrity almost entirely until it reached an altitude of 28 km, where it exploded with an energy equivalent to about 0.029 kilotons, resembling 29 tons of TNT.

“It resembled a bomb,” Egal noted, emphasizing that it was “a singular blast that generated a single spherical shockwave, rather than numerous explosions throughout its course.”

At just 72 centimeters, asteroid 2023 CX1 is roughly the size of a beach ball, which posed no significant threat to the ground. However, should a larger asteroid explode in a similar fashion, the potential for damage could be greater compared to one that disintegrates more gradually in the atmosphere.

In 2020, the Novomest Meteor in Slovenia lost around 80% of its mass due to a singular explosion.

This type of fragmentation poses an even greater threat,” Egal warned. “If a larger asteroid exhibits similar behavior, the consequences could be severe. Evacuations may be necessary for extensive areas surrounding the predicted impact site.”

Meteorite fragments of asteroid 2023 CX1 discovered in February 2023 near Dieppe, Normandy, northwest France

Lou Benoist/AFP via Getty Images

The exact reason for the asteroid’s survival at such lower altitudes in the atmosphere remains somewhat enigmatic but may pertain to its origin. 2023 CX1 belongs to the L-chondrite category, likely formed from a precursor body in the inner asteroid belt known as Massalia and contributing to approximately one-third of Earth’s rock samples.

“We observe multiple impact veins within the meteorite,” remarked the eyewitness, highlighting its significant collision history.

This implies that vigilance is imperative for monitoring similar L-chondrite asteroids, especially larger ones, according to Thomas Burbin from Mount Holyoke College, Massachusetts. “Given that this type of meteorite is quite prevalent, it raises considerable concern,” he elaborated. “L-chondrites can inflict more damage than one might anticipate.”

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Source: www.newscientist.com

A Breathtaking Supernova Image Unveils a Star That Explodes Twice After Its Death

Two concentric rings surrounding the supernova remnant SNR 0509-67.5 indicate it underwent two explosions.

ESO/p. Das et al. Background stars (Hubble): K. Noll et al.

A white dwarf star located approximately 160,000 light years away has been observed to have exploded not once, but twice. Astronomers have discovered the first proof of a supernova being linked to dual explosions.

The White Dwarf Star represents a dead stellar body, much like our Sun, which has exhausted its nuclear fuel, leaving an Earth-sized core. When a white dwarf siphons material from a companion star, it can accumulate enough mass to trigger an explosion as a Type IA supernova.

The process by which a white dwarf becomes a supernova remains largely unclear. Some astronomers have theorized that two separate explosions might occur, but until now, there has been no concrete evidence supporting this.

Priyam Das, from the University of New South Wales in Canberra, along with colleagues, examined spectra acquired by a large telescope at the European Southern Observatory in Chile. Their studies of the supernova remnant in the Large Magellanic Cloud reveal two distinct concentric shells resulting from the explosions.

Das theorizes that the white dwarf must have amassed helium on its surface, potentially from a nearby helium-rich white dwarf or a giant helium-rich star, leading to its eventual explosion.

“We witness the initial helium explosion occurring very quickly, within a mere few dozen seconds; it all happens in an instant,” states Das.

The material ejected during the first explosion was recorded to be traveling at 25,000 kilometers per second. Hence, despite the second explosion taking place only seconds later, the two events are still separated by a significant distance.

The light from this cosmic explosion is believed to have reached Earth somewhere between 310 and 350 years ago. It would have shone brightly in the southern hemisphere’s night sky, but human records indicate there was no sighting, likely due to it being obscured by the Sun.

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Source: www.newscientist.com