19-meter asteroid follows Earth’s orbit as a quasi-moon for the next six decades

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Lua, Planeta Terra Foto: Lua, Planeta Terra - Foto: Alones/ iStock

Astronomers at the Pan-STARRS observatory in Hawaii identified asteroid 2025 PN7 in August 2025. The object, with an estimated diameter of 19 meters, shares an orbit similar to that of Earth around the Sun. This configuration creates an illusion of planetary tracking, although it is not a gravitationally bound satellite.

The American Astronomical Society published initial data, confirming the detection. The asteroid belongs to the Arjuna group, formed by bodies close to Earth. Researchers monitor its trajectory to map orbital variations.

This discovery occurred during routine scans of the night sky. Telescopes like Pan-STARRS 1 have captured the asteroid’s faint glow, allowing precise calculations of its position.

Orbital characteristics of 2025 PN7

The asteroid maintains a 1:1 resonance with the Earth, completing one revolution around the Sun in the same annual period. This synchrony results in an apparent horseshoe-shaped or figure-eight pattern of movement, seen from the terrestrial perspective. However, its actual orbit follows the Sun, with minimal gravitational influence from Earth.

Arjuna Group and nearby asteroids

Asteroids from the Arjuna group have orbits of low eccentricity and inclination, approaching the Earth’s ellipse. 2025 PN7 exemplifies this class, with a semi-major axis of about 1.003 astronomical units. These objects number in the thousands, but few enter into stable resonance.

The origin of the group dates back to fragments of the main belt between Mars and Jupiter. FootGravitational disturbances from inner planets direct them towards trajectories close to Earth.

Studies indicate that 2025 PN7 entered this configuration about 60 years ago, since the mid-1960s. Simulations predict stability until 2083, when perturbations from Venus or Jupiter could alter its path.

Probable origin and composition

The asteroid likely formed in the main asteroid belt billions of years ago. Collisions and gravitational forces ejected it into an inner orbit. Its rocky composition, typical of S-type asteroids, reflects primitive material from the Solar System.

Initial spectral analyzes suggest the presence of silicates and metals. Ground-based and space-based telescopes, such as James Webb, may provide more detailed data in the coming months.

Watch Earth’s newest quasi-moon in motion. 🌍🌀 The new paper “Meet Arjuna 2025 PN7” confirms #asteroid 2025 PN7 is trapped in a quasi-satellite orbit, looping around Earth (in a rotating frame) from the 1960s to the 2080s. iopscience.iop.org/article/10.3…

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— Tony Dunn (@tony873004.bsky.social) October 212025 at 16:13

Variable distances during the cycle

2025 PN7 varies its proximity to Earth throughout the year. At closest points, it reaches around 299 thousand kilometers, similar to the average distance to the Moon. At oppositions, it moves up to 17 million kilometers away.

This fluctuation occurs due to the orbital eccentricity of 0.108 degrees. Regular observations track these changes to refine predictive models.

Astronomers plan observation campaigns in 2026, during a close approach. Infrared equipment will help measure its albedo and rotation.

No risks to the Earth

Scientists say the asteroid poses no threat of collision. Its stable trajectory maintains a minimum distance above the Earth’s atmosphere. Continuous monitoring by NASA and international agencies ensures early warnings for similar objects.

The phenomenon reinforces the importance of programs such as Near-Earth Object Observations. These efforts catalog more than 30,000 nearby asteroids, enhancing planetary defenses.

Observation with specialized equipment

Quasi-satellites like 2025 PN7 serve as accessible targets for probes. Its proximity reduces launch costs and travel time. Space agencies consider sampling missions to study nearby materialsto Earth.

Similar projects, such as the OSIRIS-REx probe, demonstrate feasibility. 2025 PN7 could provide insights into planetary formation without distant travel.

Researchers estimate that at least six known quasi-moons currently orbit Earth. Additional discoveries expand the catalog, making exploration planning easier.

Luís Henrique Costa é jornalista formado pela FMU, editor-chefe e fundador do Mix Vale, portal de notícias em atividade desde 2013. Responde pela direção editorial do veículo, que cobre Brasil e mundo em economia, benefícios sociais, esportes, tecnologia, ciência e entretenimento. Atua na área há mais de 15 anos e lidera uma equipe de cerca de 15 colaboradores.

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