A space rock named 2024 PT5, resembling the size of a school bus, lingered near Earth for almost two months last year. The asteroid, which returned in January and passed safely at a distance of 1.1 million miles, is believed to have originated from the moon. New research suggests it may have been ejected from the lunar surface thousands of years ago due to a significant impact. This insight offers a deeper understanding of near-Earth objects and their potential origins.

Study Findings Reveal Lunar Connection

According to a study published in The Astrophysical Journal Letters, observations using the Lowell Discovery Telescope in Arizona and NASA’s Infrared Telescope Facility in Hawai’i linked 2024 PT5’s surface material to lunar rocks. The asteroid’s spectral properties closely matched samples retrieved during the Apollo 14 mission, indicating its origin in the lunar highlands. Teddy Kareta, an astronomer at Lowell Observatory, highlighted in a statement, posted by the JPL that the presence of silicate minerals, which are uncommon in other asteroids but consistent with lunar material. These findings were confirmed through comparisons with extensive meteorite and terrestrial databases.

Evidence Rules Out Artificial Origins

As reported by space.com, It was determined that 2024 PT5 had a rocky composition with characteristics influenced by solar radiation, ruling out artificial origins such as space debris. Kareta noted the asteroid’s distinct trajectory and makeup, further confirming its natural formation. This is only the second recorded case of an asteroid likely originating from the moon, following the earlier discovery of 469219 Kamo’oalewa.

Implications for Planetary Defense and Future Research

The study suggests a potentially larger population of lunar-origin asteroids awaiting discovery. Researchers propose that 16 near-Earth objects in current catalogs may share similar origins. Enhanced detection capabilities, such as the upcoming Vera C. Rubin Observatory, could improve the identification and monitoring of smaller asteroids. This could provide valuable insights for planetary defense strategies, particularly in assessing impact risks from near-Earth objects of lunar origin.