Triple
T19298366
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Zhurong rover |
E482626
|
entity |
| Predicate | landingHemisphere |
P70356
|
FINISHED |
| Object | Northern hemisphere of Mars |
—
|
NE NERFINISHED |
How this triple was built (2 steps)
Every LLM step that produced this triple, in pipeline order — named-entity classification, the disambiguation choices (the exact options shown, with the pick highlighted), and the generated description. The batch + timestamp of each is in the Provenance table below.
NER
Named-entity recognition
gpt-5-mini
Instruction
Given a phrase, classify it is english named entity (e.g., persons, organizations, works of art) in Latin script, or not (e.g., literals, dates, URLs, verbose phrases). For disambiguation, the statement where the phrase occurs as object is also given. Please return a JSON object with `phrase` (string, the phrase being analyzed) and `is_ne` (boolean, indicating whether the phrase is a Named Entity).
Input
Phrase: Northern hemisphere of Mars | Statement: [Zhurong rover, landingHemisphere, Northern hemisphere of Mars]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Northern hemisphere of Mars Context triple: [Zhurong rover, landingHemisphere, Northern hemisphere of Mars]
-
A.
Elysium Planitia
Elysium Planitia is a broad, relatively flat plain near Mars’s equator, notable as a geologically young volcanic region and the landing site of NASA’s InSight mission.
-
B.
Martian southern highlands
The Martian southern highlands are an ancient, heavily cratered region of Mars characterized by high elevations, rugged terrain, and some of the planet’s oldest exposed surfaces.
-
C.
Isidis Planitia region
The Isidis Planitia region is a vast impact basin on Mars that hosts diverse geological features, including the Jezero Crater landing site of NASA’s Perseverance rover.
-
D.
Procellarum region
The Procellarum region is a vast, geologically complex area on the Moon dominated by the dark basaltic plains of Oceanus Procellarum and marked by extensive volcanic and tectonic features.
-
E.
Martian lowlands
chosen
The Martian lowlands are vast, relatively smooth and low-lying regions of Mars that contrast with the heavily cratered highlands and include major plains thought to have been shaped by ancient volcanic, fluvial, and possibly oceanic processes.
- F. None of above.
- G. Unsure - the case is ambiguous/there is not enough information to decide.
Provenance (2 batches)
The batch behind each pipeline step, in order, with when it ran. Timestamps are batch-level — stages were processed in waves, so the object chain (NER → NED1 → NEDg → NED2) reads in order, but predicate / elicitation batches can sit in a different wave.
| Step | Stage | Batch ID | Status | When |
|---|---|---|---|---|
| creating | Elicitation | batch_69d8e8cf61b0819096fe3e4107827c4e |
completed | April 10, 2026, 12:10 p.m. |
| NER | Named-entity recognition | batch_69e5fc86f8648190920d122bb141c6e5 |
completed | April 20, 2026, 10:14 a.m. |
Created at: April 10, 2026, 1:31 p.m.