Galileo Project Recovers Spherules from Interstellar Meteor – Possibile Evidence of Technological Aliens

Physicist Avi Loeb and his team have used NASA data of meteor impacts to identify interstellar meteors. The NASA data was so good they were able to pinpoint a candidate meteor that hit near Australia.

They believe have recovered pieces of that meteor and begun analyzing parts. They believe it is interstellar and has technological elements. They have found spherules.

The fundamental question is obvious: was this first recognized interstellar object from 2014 manufactured by a technological civilization? Upon their return, they could produce an alloy in the laboratory that has the same composition as they infer for the spherules and analyze the resulting material properties.

Finding more spherules will allow us to pinpoint the meteor path and potentially seek a large object that may represent its core at the end of the path. If such an object is retrieved, its structure could inform us of its technological purpose and design.

The metallic pearl-looking spherules are embedded in the volcanic ash and so our goal from now on is to retrieve all the magnetic material available on the sled magnets in the form of black powder and then identify the metallic pearls and separate them with tweezers. Ryan Weed, Jeff Wynn, Charles Hoskinson, J.J. Siler and Amir Siraj are all engaged in this effort.

Proving that they can get the magnetic sled on the ocean floor allowed us to do it again and again and find materials from IM1’s fireball site. Proving that they can retrieve the first spherule from that material allows us now to do it again and again and find a large number of spherules from IM1 in a consistent and systematic fashion.

They are now on their way back to IM1’s crash site in an attempt to retrieve as many spherules as possible. With a large enough sample, we can obtain a gamma-ray spectrum that will characterize its radioactive elements and potentially date the sample. Constraining the travel time might allow us to identify the distance and direction of its source star given its known velocity. Our preliminary analysis implies that the composition of mostly iron with a tenth of that in magnesium and some titanium does not resemble known human-made alloys or familiar asteroids.

Avi Loeb is the head of the Galileo Project, founding director of Harvard University’s — Black Hole Initiative, director of the Institute for Theory and Computation at the Harvard-Smithsonian Center for Astrophysics, and the former chair of the astronomy department at Harvard University (2011–2020). He chairs the advisory board for the Breakthrough Starshot project, and is a former member of the President’s Council of Advisors on Science and Technology and a former chair of the Board on Physics and Astronomy of the National Academies. He is the bestselling author of “Extraterrestrial: The First Sign of Intelligent Life Beyond Earth” and a co-author of the textbook “Life in the Cosmos”, both published in 2021. His new book, titled “Interstellar”, is scheduled for publication in August 2023.

Shock Resisting Steel in the Debrid Field of the First Recognized Interstellar Meteor

On Run 6 of the magnetic sled through the likely crash site of the first recognized interstellar meteor, IM1, the expedition research team recovered shards of corroded iron. At first, we thought it may be common industrial iron associated with human-made ocean trash. But when Ryan Weed ran the sample of shards through the X-ray Fluorescence (XRF) analyzer, the most likely alloy it flagged is S5 steel with titanium, which is also known as shock-resisting steel.

The yield strength of S5 steel, 1.7 GPa, is well above that of iron meteorites. This is consistent with the fact that IM1 was tougher in material strength than all other 272 meteors in the CNEOS catalog of NASA.

Most importantly, the shape of the recovered shards is nearly flat — as if they were surface layers broken off from a technological object which experienced extreme material stress. Iron meteorites break into small pieces which are melted by the fireball into spherules that rain down and are recovered in strewn fields as nearly spherical fragments.

It is possible that the fireball of IM1 resulted from the breakup of surface layers and the core of the object survived entry through the atmosphere, as expected for spacecraft.

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