Astronomer in the context of "Aristyllus"


Aristyllus, a Greek astronomer active around 261 BC, is notable for his highly accurate measurements of stellar declinations using meridian-astronomy. Initially misdated to around 300 BC, later analysis revealed his data to be exceptionally precise, surpassing that of many other ancient astronomers, and suggesting he likely worked in Alexandria.

⭐ In the context of Aristyllus, an astronomer of antiquity, what significant discovery impacted the assessment of his astronomical work?


⭐ Core Definition: Astronomer

An astronomer is a scientist in the field of astronomy who focuses on a specific question or field outside the scope of Earth. Astronomers observe astronomical objects, such as stars, planets, moons, comets and galaxies – in either observational (by analyzing the data) or theoretical astronomy. Examples of topics or fields astronomers study include planetary science, solar astronomy, the origin or evolution of stars, or the formation of galaxies. A related but distinct subject is physical cosmology, which studies the universe as a whole.

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HINT: Aristyllus was initially believed to have lived around 300 BC, which made his data appear less accurate compared to others; however, a revised dating to approximately 261 BC revealed his measurements of stellar declinations were remarkably precise for his time.

👉 Astronomer in the context of Aristyllus

Aristyllus (Greek: Ἀρίστυλλος; fl. c. 261 BC) was a Greek astronomer, presumably of the school of Timocharis (c. 300 BC). He was among the earliest meridian-astronomy observers. Six of his stellar declinations are preserved at Almajest 7.3. All are exactly correct within his over-cautious rounding to 1/4 degree. See discussion (and lessons) at DIO 7.1 ‡1 p. 13 (2007).

Aristyllus was long mis-dated to c. 300 BC (which made his data look among the poorest of the ancients); but when his correct date was found by least-squares (Isis 73:259-265 [1982] p. 263), it was realized that his star declinations' accuracy was unexcelled in antiquity. His data suggest that he worked in Alexandria: see DIO 4.1 ‡3 Table 3 p. 45 (2004).

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