Triple
T17474943
| Position | Surface form | Disambiguated ID | Type / Status |
|---|---|---|---|
| Subject | Isidis Planitia |
E425514
|
entity |
| Predicate | formsBoundaryWith |
P224
|
FINISHED |
| Object |
Martian highlands
The Martian highlands are the ancient, heavily cratered, and topographically elevated regions of Mars that dominate much of the planet’s southern hemisphere.
|
E1168420
|
NE FINISHED |
How this triple was built (4 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 highlands | Statement: [Isidis Planitia, formsBoundaryWith, Martian highlands]
NED1
Entity disambiguation (via context triple)
gpt-5-mini-2025-08-07
Target entity: Martian highlands Context triple: [Isidis Planitia, formsBoundaryWith, Martian highlands]
-
A.
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.
-
B.
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.
-
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.
Noachis Terra
Noachis Terra is a heavily cratered, ancient highland region in Mars’s southern hemisphere, notable for preserving some of the planet’s oldest geological features.
-
E.
Oxia Planum
Oxia Planum is a region on Mars characterized by ancient, clay-rich terrains that make it a prime site for investigating past habitability and the potential for preserved biosignatures.
- F. None of above. chosen
- G. Unsure - the case is ambiguous/there is not enough information to decide.
NEDg
Description generation
gpt-5.1
Instruction
Generate a one-sentence description of the target entity. You are given a context triple in the form (subject, predicate, object), where the object is the target entity. # Instructions Use the triple to infer relevant information about the entity. Describe the entity based on what is most defining, well-known. Avoid repeating the information from the triple, unless really essential. # Response Format Return only the sentence: "Description: [one-sentence description of the target entity]"
Input
Entity: Martian highlands Triple: [Isidis Planitia, formsBoundaryWith, Martian highlands]
Generated description
The Martian highlands are the ancient, heavily cratered, and topographically elevated regions of Mars that dominate much of the planet’s southern hemisphere.
NED2
Entity disambiguation (via description)
gpt-5-mini-2025-08-07
Target entity: Martian highlands Target entity description: The Martian highlands are the ancient, heavily cratered, and topographically elevated regions of Mars that dominate much of the planet’s southern hemisphere.
-
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.
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.
-
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.
Noachis Terra
Noachis Terra is a heavily cratered, ancient highland region in Mars’s southern hemisphere, notable for preserving some of the planet’s oldest geological features.
-
E.
Oxia Planum
Oxia Planum is a region on Mars characterized by ancient, clay-rich terrains that make it a prime site for investigating past habitability and the potential for preserved biosignatures.
- F. None of above.
Provenance (5 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_69d889dbc2e88190b18ea6115e819258 |
completed | April 10, 2026, 5:25 a.m. |
| NER | Named-entity recognition | batch_69e451baa7b0819092035fec42305397 |
completed | April 19, 2026, 3:53 a.m. |
| NED1 | Entity disambiguation (via context triple) | batch_6a01b82d9ec081908fe296115af1729e |
completed | May 11, 2026, 11:06 a.m. |
| NEDg | Description generation | batch_6a01b97319388190a7cd0b4f667ef16b |
completed | May 11, 2026, 11:11 a.m. |
| NED2 | Entity disambiguation (via description) | batch_6a01ba2390c08190b4077b1fe679eade |
completed | May 11, 2026, 11:14 a.m. |
Created at: April 10, 2026, 5:47 a.m.