Cleomedes ( el, Κλεομήδης) was a
Greek astronomer who is known chiefly for his book ''On the Circular Motions of the Celestial Bodies'' (Κυκλικὴ θεωρία μετεώρων), also known as ''The Heavens'' ( la, Caelestia).
Placing his work chronologically
His birth and death dates are not known—historians have suggested that he wrote his work sometime between the mid-1st century BC and 400 AD. The earlier estimates rely on the fact that Cleomedes refers extensively in his writing to the work of mathematician and astronomer
Posidonius of
Rhodes (c. 135 – c. 51 BC), and yet seemingly not at all to the work of
Ptolemy (c. 100 – c. 170 AD). (Cleomedes also refers to
Aristotle
Aristotle (; grc-gre, Ἀριστοτέλης ''Aristotélēs'', ; 384–322 BC) was a Greek philosopher and polymath during the Classical Greece, Classical period in Ancient Greece. Taught by Plato, he was the founder of the Peripatet ...
(384–322 BC),
Pytheas
Pytheas of Massalia (; Ancient Greek: Πυθέας ὁ Μασσαλιώτης ''Pythéas ho Massaliōtēs''; Latin: ''Pytheas Massiliensis''; born 350 BC, 320–306 BC) was a Greeks, Greek List of Graeco-Roman geographers, geographer, explor ...
of Massalia (310–306 BC),
Aratus (c. 315/310 BC – 240 BC),
Eratosthenes
Eratosthenes of Cyrene (; grc-gre, Ἐρατοσθένης ; – ) was a Greek polymath: a mathematician, geographer, poet, astronomer, and music theorist. He was a man of learning, becoming the chief librarian at the Library of Alexandria ...
(276–195 BC), and
Hipparchus (c. 190 – c. 120 BC). These conclusions have been challenged on the grounds that Cleomedes' work was in relatively elementary astronomy, and that reference to Ptolemy would not necessarily be expected. The 20th century mathematician
Otto Neugebauer, however, looked closely at the astronomical observations made by Cleomedes, and concluded that a date of 371 AD (±50 years) better explains what is found there. Neugebauer's estimate has been challenged on the grounds that Cleomedes makes observational errors with enough frequency that there is difficulty in deciding which observations to trust for the purpose of dating his work.
''On the Circular Motions of the Celestial Bodies''
The book for which Cleomedes is known is a fairly basic astronomy
textbook in two volumes. His purpose in writing seems to have been as philosophical as it was scientific—he spends an extensive amount of time criticizing the scientific ideas of the
Epicureans.
Cleomedes' book is valued primarily for preserving, apparently ''verbatim'', much of Posidonius' writings on astronomy (none of Posidonius' books have survived to the modern day). Cleomedes is accurate in some of his remarks on
lunar eclipse
A lunar eclipse occurs when the Moon moves into the Earth's shadow. Such alignment occurs during an eclipse season, approximately every six months, during the full moon phase, when the Moon's orbital plane is closest to the plane of the Earth ...
s, especially his conjecture that the shadow on the
Moon suggests a
spherical Earth
Earth is the third planet from the Sun and the only astronomical object known to harbor life. While large volumes of water can be found throughout the Solar System, only Earth sustains liquid surface water. About 71% of Earth's surf ...
. He also remarks presciently that the absolute size of many stars may exceed that of the
Sun (and that the Earth might appear as a very small star, if viewed from the surface of the Sun).
This book is the original source for the well-known story of how
Eratosthenes
Eratosthenes of Cyrene (; grc-gre, Ἐρατοσθένης ; – ) was a Greek polymath: a mathematician, geographer, poet, astronomer, and music theorist. He was a man of learning, becoming the chief librarian at the Library of Alexandria ...
measured the
Earth's circumference. Many modern mathematicians and astronomers believe the description to be reasonable (and believe Eratosthenes' achievement to be one of the more impressive accomplishments of ancient astronomy).
Cleomedes deserves credit for the earliest clear statement of the apparent distance explanation of the Sun Illusion or
Moon Illusion. He argued that the sun appeared farther away on the horizon than in the zenith, and therefore larger (since its angular size was constant). He attributed this explanation to Posidonius.
Optics
As a disciple of
Posidonius, Cleomedes noted some elementary qualitative properties of
refraction, such as the bending of a ray toward the perpendicular in passing from a less dense to a more dense medium, and suggested that due to
atmospheric refraction
Atmospheric refraction is the deviation of light or other electromagnetic wave from a straight line as it passes through the atmosphere due to the variation in air density as a function of height. This refraction is due to the velocity of ligh ...
, the Sun and its rainbow may be visible when the Sun is below the horizon.
[ Carl Benjamin Boyer, ''The Rainbow: From Myth to Mathematics'' (1959)]
Legacy
Cleomedes is now memorialized by the crater
Cleomedes
Cleomedes ( el, Κλεομήδης) was a Greek astronomer who is known chiefly for his book ''On the Circular Motions of the Celestial Bodies'' (Κυκλικὴ θεωρία μετεώρων), also known as ''The Heavens'' ( la, Caelestia).
Pla ...
in the northeastern portion of the visible Moon.
References
Further reading
* Alan C. Bowen, Robert B. Todd, ''Cleomedes' Lectures on Astronomy. A Translation of The Heavens with an Introduction and Commentary''. University of California Press, 2004.
* Helen E. Ross, "Cleomedes (c. 1st century AD) on the celestial illusion, atmospheric enlargement, and size-distance invariance". ''Perception'', 2000, 29, 863–871.
External links
''On the Circular Motions of the Celestial Bodies'', original text online and biographyEnglish translation of the section on Eratosthenes and the size of the earthat Roger Pearse.
*
*
ttps://archive.org/details/Cleomedes-DeMotuCirculari-TheHeavens Edicion Bilingue Griego Español
{{Authority control
Roman-era Greeks
Ancient Greek astronomers
Ancient Greek mathematicians