2025 PN7 is a recently discovered and highly intriguing celestial object that has captured the attention of scientists across the world. This small asteroid moves in such a way relative to Earth that it appears to be a “second moon.” In astronomical terms, such objects are called quasi-satellites or quasi-moons because they seem to orbit Earth, but in reality, they revolve around the Sun.
The object was first detected on August 2, 2025, by the Pan-STARRS Observatory of the University of Hawai‘i, using its advanced telescopes. Astronomers from the university sent detailed findings of this discovery to the American Astronomical Society and NASA, both of which have officially confirmed it.
2025 PN7 is a kind of co-traveler of Earth, moving around the Sun at almost the same speed as our planet — a phenomenon known as 1:1 orbital resonance. It always remains near Earth, sometimes slightly ahead, sometimes behind, but it completes its solar orbit in the same time as Earth does. The tiny asteroid has an estimated diameter of 18–19 meters, roughly the size of a large bus — detecting such a small object from Earth is a remarkable scientific achievement.
Its orbit is unique. On average, it stays 1.003 astronomical units from the Sun — just a little farther than Earth. The orbital inclination is only 2 degrees, meaning it moves almost in the same plane as Earth. Its eccentricity is 0.108, showing that its path is not a perfect circle but a slightly elongated ellipse.
When it comes closest to Earth, 2025 PN7 is about 300,000 kilometers away — roughly the same as the average distance to the Moon. Sometimes, it drifts several hundred thousand kilometers farther away, so it is not constantly near Earth but periodically returns to proximity. According to astronomical studies, it has been accompanying Earth in this co-orbital path for the past sixty years and will likely continue until around 2083. After that, minor gravitational influences may alter its orbit, sending it away from Earth.
Unlike the Moon, this object is not a permanent satellite, because it is not gravitationally bound to Earth. The Moon has been orbiting Earth for nearly four billion years, held firmly by Earth’s gravity, whereas 2025 PN7 is not. It independently revolves around the Sun, but its motion is synchronized in such a way that it appears to circle Earth. This temporary relationship is what defines a “quasi-moon.”
One of the most important facts about 2025 PN7 is that it poses no threat to Earth. NASA and University of Hawai‘i scientists have clarified that the asteroid never approaches closer than 400,000 kilometers and there is no chance of it entering Earth’s atmosphere. Therefore, it is considered completely harmless and an ideal subject for study.
From a scientific standpoint, this discovery is of great significance. Such objects help astronomers better understand the dynamics of near-Earth asteroids and the history of the Solar System. They reveal how subtle gravitational interactions maintain delicate orbital balances. Moreover, these co-orbital asteroids could serve as excellent targets for future space missions, since they stay close to Earth and require relatively low fuel to reach.
2025 PN7 belongs to the “Arjuna asteroid group” — a class of small bodies with orbits similar to Earth’s. Several other quasi-moons have been discovered before, such as 3753 Cruithne, 2003 YN107, and 469219 Kamoʻoalewa, all of which have shown similar co-orbital behavior. 2025 PN7 is the newest addition to this fascinating list.
Discoveries like this remind humanity that space around us still holds countless mysteries. Asteroids like 2025 PN7 show that Earth’s cosmic neighborhood is not just filled with the Moon and artificial satellites — it also hosts these tiny cosmic dancers, moving gracefully to the rhythm of the universe. Though small in size, 2025 PN7 greatly expands our astronomical understanding and rekindles human curiosity. It is a temporary yet remarkable companion of Earth, reminding us that in astronomy, the frontier of discovery is truly endless.
