Important caveat: The China National Space Administration (CNSA) has not yet officially confirmed the June 7 rendezvous, but major tracking data and independent analysts, including The Planetary Society and AMSAT-DL, align with that date . The spacecraft is in excellent health and performing nominally .
Tianwen-2 carries three distinct sampling modes to maximize success on this small, fast-rotating body :
The target is to collect 200–1,000 grams of regolith — significantly more than JAXA's Hayabusa2 (~5.4 g) or NASA's OSIRIS-REx (~121.6 g) .
| Phase | Date / Window |
|---|---|
| Launch | May 28, 2025 |
| Rendezvous with Kamoʻoalewa | June 7, 2026 (probable) |
| Remote sensing & site selection | July 2026 – April 2027 |
| Sample collection | Late 2026 – early 2027 |
| Departure from Kamoʻoalewa | April 24, 2027 |
| Sample capsule Earth return | ~November 2027 (capsule lands in Gobi Desert) |
| Earth gravity assist / slingshot | Late 2027 (mothership continues) |
| Arrival at comet 311P/PanSTARRS | ~2034–2035 |
| End of extended mission | ~2035 |
After dropping the sample return capsule to Earth, the mothership will use an Earth gravity assist to slingshot toward the main-belt comet 311P/PanSTARRS (P/2013 P5) — an active, dust-emitting object in the asteroid belt. It will arrive around 2034–2035 for orbital insertion and flyby studies, making this a decade-long dual-object mission .
One of the most compelling questions Tianwen-2 is designed to answer is where Kamoʻoalewa came from. The evidence so far points in two directions.
Multiple peer-reviewed studies (including Nature Communications and Communications Earth & Environment) show that Kamoʻoalewa's reflectance spectrum is a near-perfect match for space-weathered lunar silicates, not typical main-belt asteroids . Its reddened spectrum, Earth-like orbit, and proximity to the Earth-Moon system strongly suggest it is a lunar ejecta fragment — likely from the Copernicus or Giordano Bruno craters — blasted off the Moon by an impact and captured into Earth's 1:1 resonance . It is one of only a handful of known "quasi-satellites" of Earth .
A new study published in Nature Communications in June 2026 has challenged the lunar origin, proposing instead that Kamoʻoalewa's spectral properties could be consistent with certain S-type asteroids from the inner main belt, including the Flora family, and that its current orbit does not definitively require a lunar origin . The study argues that the fast rotation and small size of the asteroid could produce similar spectral reddening through space weathering alone .
Bottom line: The lunar origin hypothesis remains the leading explanation, but the debate is active. Tianwen-2's returned samples will provide the definitive answer by comparing isotope ratios, mineralogy, and noble gas signatures to known lunar samples .
Tianwen-2 is strategically important on several fronts: