SpaceMiningData
SpacecraftMoonEnded

Chang'e-6

Chinese lunar far-side sample-return mission launched on 3 May 2024 that landed in the South Pole-Aitken basin on 2 June 2024 and returned 1,935.3 grams on 25 June 2024. A 2025 peer-reviewed laboratory study of impact glass beads in the returned soil measured equivalent water abundances of roughly 10–1,070 micrograms per gram. Solar-wind hydration profiles were found in mare glass beads; the full numerical range is not attributed solely to solar-wind water. These are findings from returned material, not extraction on the Moon.

Objective. Return samples from the lunar far side; the volatile evidence comes from laboratory analysis of collected impact glass beads, not resource extraction on the Moon.

Listed for scientific context. This mission published a resource finding but is not counted as a resource mission.

Sampled

See Apollo basin on the 3D Moon

Facts

Kind
Spacecraft
Mission type
Sample return
Target
MoonApollo basin within the South Pole-Aitken basin, lunar far sideOn the Moon map: Apollo basin
Launch
2024-05-03
Launch vehicle
Long March 5
Phase
EndedCNSA/Xinhua timeline (2024-06-26) and sample-mass release (2024-06-28).
Outcome
SuccessBasis: agency statement
Why it is included
Published resource finding (science context)

Outcome statement (agency statement)

China's Chang'e-6 mission collected 1,935.3 grams of samples from the far side of the moon, preliminary measurement by the China National Space Administration (CNSA) showed Friday.

What comes next

This mission has ended.

Participants

Operators, payload owners, carriers and customers are recorded separately.

OrganizationRole
China National Space AdministrationOperator

Resources and evidence

ResourceEvidence
RegolithSampled
VolatilesSampled

Open evidence gaps

  • 'Apollo basin' comes from peer-reviewed literature (PNAS 2025) rather than the CNSA timeline, which says only 'South Pole-Aitken (SPA) Basin'.

Sources

6 excerpts from 3 publications

One web address counts as one publication.

  1. CNSA (Xinhua)Government recordPublished 2024-06-28Accessed 2026-09-25Supports: outcome, resources
    China's Chang'e-6 mission collected 1,935.3 grams of samples from the far side of the moon, preliminary measurement by the China National Space Administration (CNSA) showed Friday.
    Quote matched the source text when accessed.
  2. CNSA (Xinhua)Government recordPublished 2024-06-26Accessed 2026-09-25Supports: launch date, launch vehicle
    The Chang'e-6 probe was launched by a Long March-5 rocket from the Wenchang Space Launch Site on May 3.
    Quote matched the source text when accessed.
  3. CNSA (Xinhua)Government recordPublished 2024-06-26Accessed 2026-09-25Supports: target site, summary
    successfully landed at the designated landing area in the South Pole-Aitken (SPA) Basin on June 2
    Quote matched the source text when accessed.
  4. Nature Communications (via PubMed Central)Peer-reviewedPublished 2025-05-29Accessed 2026-11-03Supports: why it is included, resources, summary
    Here, we report the water abundances and hydrogen isotope compositions and their distribution in farside IGBs collected by the Chang’e-6 mission to investigate the role of IGBs in the lunar surface water cycle.
    Quote matched the source text when accessed.
  5. Nature Communications (via PubMed Central)Peer-reviewedPublished 2025-05-29Accessed 2026-11-03Supports: why it is included, resources, summary
    Farside IGBs are found to have water abundances of ~10–1,070 μg.g −1 with hydrogen isotopes (δD) ranging from –988‰ to >2000‰ and display typical SW-H 2 O hydration profiles. The SW-H 2 O hydration depths in farside IGBs are strikingly shallower than in nearside IGBs. Moreover, the hydration profiles are only found in mare IGBs, with none observed in non-mare IGBs, indicating that SW-H 2 O hydration in IGBs is likely composition dependent.
    Quote matched the source text when accessed.
  6. Nature Communications (via PubMed Central)Peer-reviewedPublished 2025-05-29Accessed 2026-11-03Supports: resources, summary
    The CE6 Homo-IGBs were measured to have equivalent water abundances of ~10–1070 μg.g −1 with H isotope compositions (in notation of δD, δD = 1000 × (D/H sample /D/H SMOW -1), where D/H SMOW is the D/H ratio of the standard mean ocean water; Methods) ranging from – 988 ± 61 to 3718 ± 535‰ after spallation correction at a cosmic ray exposure age of 108 million years ago (Fig.  3 and Supplementary Data  3 ; Methods).
    Quote matched the source text when accessed.

Cite this record

SpaceMiningData, “Chang'e-6”, dataset version a00fa2c68a45, built 2026-11-11, https://spaceminingdata.com/missions/cnsa-change-6.html. Record checked 2026-09-25.