Triple

T1403822
Position Surface form Disambiguated ID Type / Status
Subject Kepler’s second law E31644 entity
Predicate alsoKnownAs P39 FINISHED
Object law of equal areas E31644 NE FINISHED

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: law of equal areas | Statement: [Kepler’s second law, alsoKnownAs, law of equal areas]
NED1 Entity disambiguation (via context triple) gpt-5-mini-2025-08-07
Target entity: law of equal areas
Context triple: [Kepler’s second law, alsoKnownAs, law of equal areas]
  • A. Kepler’s laws of planetary motion chosen
    Kepler’s laws of planetary motion are three fundamental principles that mathematically describe how planets orbit the Sun in ellipses, sweep out equal areas in equal times, and relate their orbital periods to their distances from the Sun.
  • B. law of universal gravitation
    The law of universal gravitation is Newton’s fundamental physical law stating that every pair of masses in the universe attracts each other with a force proportional to the product of their masses and inversely proportional to the square of the distance between them.
  • C. Lagrange’s planetary equations
    Lagrange’s planetary equations are a set of differential equations in celestial mechanics that describe how the orbital elements of a body evolve over time under perturbing forces.
  • D. Newton's laws of motion
    Newton's laws of motion are three fundamental principles in classical mechanics that describe the relationship between forces acting on a body and its resulting motion.
  • E. Gauss’s planetary equations
    Gauss’s planetary equations are a set of differential equations in celestial mechanics that describe how a planet’s orbital elements change over time under the influence of perturbing forces.
  • F. None of above.
  • G. Unsure - the case is ambiguous/there is not enough information to decide.

Provenance (3 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_69a49918e1f88190ba610f9dc8114578 completed March 1, 2026, 7:52 p.m.
NER Named-entity recognition batch_69a4c3a0330c8190b22452d29c79fcf4 completed March 1, 2026, 10:54 p.m.
NED1 Entity disambiguation (via context triple) batch_69ace57125a4819089216bbc75c36bb9 completed March 8, 2026, 2:56 a.m.
Created at: March 1, 2026, 7:59 p.m.