Moon’s far-side highlands region
E1084178
UNEXPLORED
The Moon’s far-side highlands region is a heavily cratered, mountainous area on the lunar hemisphere permanently turned away from Earth, characterized by its thick crust and scarcity of the dark basaltic maria seen on the near side.
All labels observed (1)
| Label | Occurrences |
|---|---|
| Moon’s far-side highlands region canonical | 1 |
How this entity was disambiguated
This entity first appeared as the object of triple T14160521 — resolving that mention is where its identity was fixed. The disambiguator weighed these candidate entities and picked the highlighted one (or “None”, minting a new entity). This is how homonymy is resolved: the same surface form can point to different entities.
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Moon’s far-side highlands region Context triple: [Schwarzschild C, belongsTo, Moon’s far-side highlands region]
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A.
Apollonius highlands
The Apollonius highlands are a rugged, heavily cratered lunar highland region near the Moon’s eastern limb, named after the crater Apollonius.
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B.
Imbrium Basin ejecta zone
The Imbrium Basin ejecta zone is the extensive region on the Moon blanketed by material blasted out during the formation of the large Imbrium impact basin, shaping much of the surrounding lunar surface geology.
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C.
Descartes Highlands
Descartes Highlands is a rugged, heavily cratered lunar highland region notable as the exploration site of NASA’s Apollo 16 mission.
-
D.
Mare Nubium
Mare Nubium is a large lunar mare located in the Moon’s southern near side, characterized by its dark basaltic plains formed from ancient volcanic activity.
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E.
Apennine Mountains (Moon)
Apennine Mountains (Moon) is a prominent lunar mountain range along the southeastern edge of Mare Imbrium, notable for its towering peaks and as the landing site region of Apollo 15.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Moon’s far-side highlands region Target entity description: The Moon’s far-side highlands region is a heavily cratered, mountainous area on the lunar hemisphere permanently turned away from Earth, characterized by its thick crust and scarcity of the dark basaltic maria seen on the near side.
-
A.
Apollonius highlands
The Apollonius highlands are a rugged, heavily cratered lunar highland region near the Moon’s eastern limb, named after the crater Apollonius.
-
B.
Imbrium Basin ejecta zone
The Imbrium Basin ejecta zone is the extensive region on the Moon blanketed by material blasted out during the formation of the large Imbrium impact basin, shaping much of the surrounding lunar surface geology.
-
C.
Descartes Highlands
Descartes Highlands is a rugged, heavily cratered lunar highland region notable as the exploration site of NASA’s Apollo 16 mission.
-
D.
Mare Nubium
Mare Nubium is a large lunar mare located in the Moon’s southern near side, characterized by its dark basaltic plains formed from ancient volcanic activity.
-
E.
Apennine Mountains (Moon)
Apennine Mountains (Moon) is a prominent lunar mountain range along the southeastern edge of Mare Imbrium, notable for its towering peaks and as the landing site region of Apollo 15.
- F. None of above. chosen
Referenced by (1)
Full triples — surface form annotated when it differs from this entity's canonical label.