Scientists discover metal fragments from outside the solar system
Recently, scientists have made groundbreaking revelations regarding metal fragments retrieved from the Pacific Ocean that originated from outside our solar system. Led by the renowned Avi Loeb, a Harvard physicist with an avid interest in alien phenomena, the team published a preprint study that sheds light on the properties and origins of a meteor crash that occurred in 2014.
During a June expedition, researchers surveyed the seafloor off the coast of New Guinea, where they stumbled upon approximately 700 small metallic spheres. Upon analyzing 57 of these spheres, they found compositions that deviated from anything present in our solar system.
According to the published paper, the team posits that these unique properties emerged when an Earth-like planet deviated from its circular orbit around a dwarf star. This deviation caused a stream of debris to be propelled into interstellar space. As a result, the planet’s crust melted, leading to the formation of abundant beryllium, lanthanum, and uranium – elements that were discovered within the metallic spheres retrieved from the ocean’s depths.
While the new analysis primarily indicates a natural origin, Loeb suggests that these abundant rare elements may have had a technological purpose. For instance, lanthanum could have melted from semiconductors, while uranium could have functioned as fuel in a fission reactor.
Loeb and his team exhibit an unwavering commitment to unraveling the mysteries surrounding these metal fragments. In an interview with DailyMail.com, Loeb expressed their intention to discover the true nature of this interstellar matter by locating larger pieces during their subsequent expedition, anticipated to take place within the next nine months.
“Does this mean that IM1 definitely originated from a natural astrophysical environment and was not a technological Voyager-like meteor manufactured by another civilization? We do not know for sure,” Loeb stated in a Medium post.
The initial analysis conducted in August highlighted the remarkable attributes of this meteor-like object referred to as IM1. While the elements found within the fragments can be found on Earth, their patterns do not conform to the alloys present on our planet, Moon, Mars, or other natural meteorites within the solar system.
Building upon their previous findings, the team conducted calculations to determine the speed at which rocks were launched from the Earth-like planet’s crust during the tidal disruption event. Astonishingly, the rocks traveled at a speed equivalent to 37 miles per second – higher than 95 percent of the random speeds of stars near the Sun. Of particular interest, this speed aligns precisely with the speed recorded for the first reported interstellar meteor, IM1, by US government satellites on January 8, 2014.
The data from the initial analysis conducted in August unveiled the fragments to be rich in beryllium, lanthanum, and uranium, with a low content of elements with high affinity to iron, such as rhenium.
It is believed that these remnants originated from a meter-size object that crashed off the coast of Papua, New Guinea in 2014. Loeb boldly suggests that this object may have been an alien craft. The retrieval of around 700 metallic spheres further solidifies his claim, as these spheres contain alloys exclusive to interstellar space.
The peculiar ‘BeLaU’ composition found within the fragments is believed to have resulted from the rocky planet making numerous close-in passages around the dwarf star, which led to the melting of the planet’s surface. This melting facilitated the differentiation of the elements, causing those with an affinity to iron to sink into the planet’s iron core. Loeb explains that IM1’s unusually high material strength may have resulted from the hardening associated with repeated cycles of melting, crusting, and enhanced elemental differentiation, surpassing that observed in planets like Earth or Mars.
Despite the new analysis pointing towards a natural origin for IM1, Loeb remains open to the possibility that aliens may have been involved in its creation. To solve this enigma, Loeb and his team are preparing for a second expedition to the Pacific Ocean, during which they aim to uncover larger pieces of IM1 and determine whether it is a mere rock or a more exotic object.
For years, Avi Loeb has expressed his conviction that interstellar technology may have visited our planet. His groundbreaking theory regarding the interstellar object Oumuamua, which passed through our solar system in 2017, garnered immense attention. Although most scientists viewed it as a purely natural phenomenon, Loeb boldly argued that it could have been of alien origin. In 2019, his theory gained validation when a high-speed fireball in 2014, known as the IM1 meteor, was discovered to have interstellar origins predating Oumuamua.
The first expedition in search of remnants from the 2014 meteor lasted two weeks in June. A group consisting of Harvard’s Galileo Project Expedition scientists, the ship’s crew, and documentary filmmakers set sail from Lorengau, a small town located on an island. While navigating the Pacific, they meticulously combed the seabed for signs of IM1 debris, utilizing a deep-sea magnetic sled to traverse the fireball’s last known path. In total, they completed 26 runs along the seafloor.
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