Seven asteroids are Earth's quasi-moons: they orbit the Sun but stay near Earth for decades to centuries
A quasi-moon, or quasi-satellite, orbits the Sun in a year, just as Earth does, but on a slightly more stretched or tilted orbit. Seen from Earth it seems to loop around us once a year, moving backward, yet Earth's gravity does not hold it; it would follow almost the same path if Earth were not there. The arrangement lasts decades to thousands of years before the asteroid drifts away. Seven are generally listed; some lists add 2022 YG. Sizes are estimated from brightness, and orbital values are approximate.
| Quasi-moon | Size, m | Eccentricity | Tilt | Quasi-moon for | Note |
|---|---|---|---|---|---|
| Kamoʻoalewa | 40 to 100 | 0.10 | 7.8° | about 1910 to 2290 | The most stable; possibly a fragment of the Moon. China's Tianwen-2 has flown alongside it since July 2026. |
| 2025 PN7 | 19 to 30 | 0.11 | 2° | about 1965 to 2083 | The newest and smallest, found by Pan-STARRS in August 2025. |
| Cardea | 160 to 360 | 0.14 | 13.7° | a few centuries | Formally 164207 (2004 GU9). |
| 2023 FW13 | 10 to 20 | 0.18 | 14.8° | about 100 BCE to 3700 CE | Found by Pan-STARRS in March 2023; one of the longest-lived. |
| 2006 FV35 | 140 to 320 | 0.38 | 7.1° | a few thousand years | Formally 277810; its stretched orbit swings it far from Earth. |
| 2013 LX28 | 130 to 300 | 0.45 | 49.9° | about 1,000 years | Tilted about 50° to Earth's orbit. |
| 2014 OL339 | 150 to 340 | 0.46 | 10.2° | a few hundred years | Strays more than 1 AU from Earth on its widest loops. |
Kamoʻoalewa may be a piece of the Moon, and China's Tianwen-2 is bringing a sample home
Found by Pan-STARRS in Hawaii in 2016 and named from a Hawaiian chant, Kamoʻoalewa stays 38 to 100 times the Moon's distance from Earth. In 2021 its reddish spectrum turned out to match space-weathered lunar rock, and a 2024 study traced it to the impact that made the Giordano Bruno crater on the Moon's far side 1 to 10 million years ago; other researchers dispute the link. China's Tianwen-2 launched on May 29, 2025, reached it in early July 2026 and is mapping it before collecting a sample. It leaves in April 2027, drops its capsule in the Gobi Desert in November 2027, then heads for the comet 311P/PANSTARRS, arriving around 2035.
Mini-moons are truly captured by Earth, but only for weeks to months
A mini-moon is a small asteroid that Earth's gravity actually captures for a while, usually one of the Arjunas, asteroids on orbits almost the same as Earth's. Most are a meter or two across and stay a few months; models suggest Earth usually has at least one. Only five have been seen:
| Mini-moon | Captured | Size | Note |
|---|---|---|---|
| 2006 RH120 | September 2006 to June 2007 | a few meters | The first mini-moon found, by the Catalina Sky Survey; it looped around Earth about four times. |
| 2020 CD3 | about 2018 to April 2020 | 1 to 6 m | Found by Catalina in February 2020, weeks before it escaped. |
| 2022 NX1 | 1981, and again in 2022 | 5 to 15 m | Captured twice, briefly each time. |
| 2024 PT5 | September 29 to November 25, 2024 | about 10 m | Its spectrum matches lunar rock, so it may be a chip of the Moon. |
| 2026 QQ8 | April 2026 to about January 2027 | 1 to 2 m | Found by Krisztián Sárneczky in Hungary in August 2026 and confirmed as natural in October; it next passes close in 2058. |
Trojans and horseshoe orbits are other ways to share Earth's orbit
- Earth trojans lead or trail Earth by 60°, near the L4 or L5 points: 2010 TK7, found by NASA's WISE in 2010, and 2020 XL5, about 1 km across.
- Horseshoe orbits: 3753 Cruithne, sometimes called Earth's second moon, creeps up on Earth along its orbit, turns back and repeats over centuries. It never loops around Earth, so it is not a moon.
- Kordylewski clouds, faint clouds of dust at the Earth-Moon L4 and L5 points, were reported in 1961 and again by Hungarian astronomers in 2018; they remain unconfirmed.
The Rubin Observatory should find many more, and they are the easiest asteroids to reach
Quasi-moons and mini-moons are small and faint, and many sit near the Sun in the sky, so few are known. The Vera C. Rubin Observatory and NASA's NEO Surveyor should find many more. Because their orbits are so like Earth's, they take less energy to reach than the Moon's surface, which makes them targets for sample-return missions and for testing asteroid mining. Near-Earth objects · Asteroids · Moons of the planets