July 15, 2026, Mountain View, CA — On July 16, 2024, a daytime meteor rattled New York City, producing a sonic boom as it skimmed south of the Statue of Liberty. Shortly afterward, an international research team reports in Science Advances that the same event also delivered a substantial meteorite: more than two pounds of rock crashing through a house roof in Hillsborough, New Jersey.
The entry occurred at roughly 32,000 miles per hour (14.4 kilometers per second). Dozens of observers across the region documented the fireball, while additional witnesses confirmed a shockwave sensation. Trajectory reconstruction, supported by multiple camera feeds including a doorbell video, traced the path back toward the asteroid belt.
The meteor disintegrated high in the atmosphere, becoming invisible at about 22 miles (35 kilometers) altitude. Afterward, a Doppler weather radar at Newark Airport briefly detected a stretching cloud of falling debris. Hillsborough lay at the far end of the precipitation corridor, explaining why the largest surviving piece came down at that specific location.
Fragments recovered from the crash site underwent forensic mineralogical study. The material matches the class of CM-type carbonaceous chondrites, where “M” refers to the Mighei meteorite, but the Hillsborough sample shows more extensive water-driven alteration than typical members of the CM2 subgroup.
Crucially, the team classifies the specimen as CM1/2—an intermediate petrographic type between CM1 and CM2. Hillsborough becomes only the second witnessed fall in this narrow category, following a 2020 event in North Sumatra, Indonesia. Researchers emphasize the exceptional preservation made possible by rapid, careful recovery at the impact site.
Analysis also points to salt-rich, briny fluids near the parent asteroid’s surface. Small fragments enriched in salts suggest evaporative concentration processes, potentially occurring just below the surface where liquid water was transient and chemistry could evolve quickly.
The meteorite contains carbon and nitrogen with isotopic signatures characteristic of CM meteorites, alongside a high fraction of soluble organics. Among them are amino acids and carboxylic acids—molecules relevant to prebiotic chemistry. The study argues that brine-associated mineral-organic interactions likely shaped the observed organic distribution inside the parent body.
“These findings refine how we think primitive asteroids transported both organics and aqueous alteration products,” the authors conclude, highlighting Hillsborough as a rare laboratory for early Solar System chemistry.
Some fragments will be curated at the American Museum of Natural History in New York City. The team notes that continued mineral and isotopic comparisons will help link Hillsborough’s salt phases and organics to samples returned from asteroids Ryugu and Bennu.
Subject of Research: CM1/2 carbonaceous chondrite meteorite; briny fluid alteration; prebiotic organic chemistry
Article Title: Not provided in the supplied text
News Publication Date: 15-Jul-2026
Web References: http://www.science.org/doi/10.1126/sciadv.ea2105
References: 10.1126/sciadv.ea2105
Image Credits: SETI Institute
Keywords
Meteorites, CM-type carbonaceous chondrites, CM1/2, brines, amino acids, prebiotic chemistry, asteroid belt, organic molecules, Science Advances, Hillsborough meteorite
