Triple
T22056804
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Argyre Planitia |
E545041
|
entity |
| Predicate | partOf |
P40
|
FINISHED |
| Object | Martian southern highlands region |
—
|
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: Martian southern highlands region | Statement: [Argyre Planitia, partOf, Martian southern highlands region]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Martian southern highlands region Context triple: [Argyre Planitia, partOf, Martian southern highlands region]
-
A.
Martian southern highlands
chosen
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.
-
B.
Daedalia Planum region
The Daedalia Planum region is a vast, relatively smooth volcanic plain on Mars located southwest of the Tharsis rise and heavily shaped by lava flows from nearby giant volcanoes.
-
C.
Lunae Planum region
The Lunae Planum region is a broad, relatively smooth volcanic plain on Mars located near the Tharsis rise and shaped by extensive lava flows and tectonic activity.
-
D.
Argyre Planitia region
Argyre Planitia region is a large impact basin in Mars's southern hemisphere, characterized by its broad, low-lying plains and surrounding ring of rugged highlands.
-
E.
Martian lowlands
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_69e11e3377c48190890c17407b9527d6 |
completed | April 16, 2026, 5:36 p.m. |
| NER | Named-entity recognition | batch_69f128588e0081909056ac8251afe935 |
completed | April 28, 2026, 9:36 p.m. |
Created at: April 16, 2026, 8:27 p.m.