The China Nationwide Area Administration’s asteroid probe Tianwen-2 efficiently reached the asteroid Kamo’oalewa, which orbits the Solar in a path practically similar to Earth’s.
After present process a number of orbital changes in deep area, it first detected Kamo’oalewa on June 6, 2026. On July 2, it efficiently captured the first-ever photos of Kamo’oalewa from a distance of about 20 kilometers. This achievement comes on the finish of a 400 day journey overlaying a distance of roughly 1 billion kilometers.
Kamo’oalewa is essentially the most steady of Earth’s recognized quasi-satellites, and since it orbits the Solar in near-synchronous movement with Earth, it’s thought-about a comparatively accessible celestial physique.
However touchdown on the asteroid—not to mention gathering samples—will likely be a problem. Kamo’oalewa has a median diameter of solely about 41 meters and rotates at excessive pace. This implies the spacecraft should obtain steady contact and acquire samples inside a restricted timeframe. If it manages to assemble samples, it’s going to then launch them in a capsule throughout an Earth flyby in November 2027.
Tianwen-2 is provided with a number of cameras with totally different focal lengths. Along with switching between a narrow-field-of-view digicam and a wide-field-of-view digicam relying on the state of affairs, it additionally encompasses a removable digicam that will likely be used throughout pattern assortment. Because the probe’s orientation have to be finely adjusted when capturing photos, seizing these restricted home windows of alternative is an especially tough process. Tianwen-2 plans to conduct extra detailed scientific observations of Kamo’oalewa’s form, materials composition, and inner construction.
If this mission is profitable, it’s going to mark one other achievement in asteroid pattern return, following Japan’s Hayabusa and Hayabusa2 missions—the primary to return asteroid samples to Earth—and NASA’s OSIRIS-REx mission. Materials from small celestial our bodies orbiting close to Earth may present one of many few clues to understanding the formation of the photo voltaic system, together with Kamo’oalewa.
“It’s extremely prone to include primordial info from the early days of the photo voltaic system’s formation, and it holds nice scientific worth for finding out early materials composition, formation processes, and evolutionary historical past,” explains Han Siyuan, deputy director of the Lunar and Area Exploration Engineering Heart and spokesperson for the Tianwen-2 mission.
Researchers have beforehand theorized that Kamo’oalewa is a fraction of the Moon blown away by an asteroid affect thousands and thousands of years in the past has been broadly accepted till lately. It is because the spectrum of mirrored mild carefully resembles that of silicate minerals discovered on the Moon’s floor. Simulations additionally backed the idea up.
In Might, although, a global analysis crew—together with the Chinese language Academy of Sciences— revealed a paper that casts doubt on this main speculation. A reanalysis of obtainable information discovered that the central wavelength of the absorption band—the purpose the place mild weakens at a particular wavelength—matched the traits of LL chondrites (a sort of meteorite with low iron and steel content material).
The analysis crew carried out an experiment by which they irradiated LL chondrite meteorite powder with a laser to simulate area weathering brought on by photo voltaic wind and micrometeorites. The outcomes carefully matched observational information of Kamo’oalewa. The researchers posit that Kamo’oalewa doubtless migrated to the Earth’s neighborhood from the Flora household—a gaggle of celestial our bodies within the asteroid belt.
If Tianwen-2 efficiently completes its mission to take samples and return to Earth, it’s going to doubtless assist reply questions on Kamo’oalewa’s origins. However first, it has to achieve the asteroid’s floor.
This story initially appeared in WIRED Japan and has been translated from Japanese.
