-
1
-
-
0347543037
-
"On the function and probable origin of Ptolemy's equant"
-
James Evans, "on the function and probable origin of Ptolemy's equant", American journal of physics, lii (1984), 1080-9.
-
(1984)
American Journal of Physics
, vol.52
, pp. 1080-1089
-
-
Evans, J.1
-
2
-
-
84992792207
-
"The empirical foundations of Ptolemy's planetary theory"
-
Noel Swerdlow, "The empirical foundations of Ptolemy's planetary theory", Journal for the history of astronomy, xxxv (2004), 249-71.
-
(2004)
Journal for the History of Astronomy
, vol.35
, pp. 249-271
-
-
Swerdlow, N.1
-
3
-
-
84992861144
-
"A route to the discovery of non-uniform planetary motion"
-
Alexander Jones, "A route to the discovery of non-uniform planetary motion", ibid., 375-86.
-
(2004)
Journal for the History of Astronomy
, vol.35
, pp. 375-386
-
-
Jones, A.1
-
5
-
-
0039358136
-
-
The details of the calculation may be found in (Odense)
-
The details of the calculation may be found in Olaf Pedersen, A survey of the Almagest (Odense, 1974), 285-6,
-
(1974)
A Survey of the Almagest
, pp. 285-286
-
-
Pedersen, O.1
-
7
-
-
85039317958
-
-
note
-
Since the sidereal period of Mars is about 1.88 years, it will always pass perigee in just less than a year after it passes apogee, and vice versa. Thus, having analysed at least one trio, the analyst would be able to predict the dates of these apsidal line passings quite accurately.
-
-
-
-
9
-
-
26444556400
-
"Ausgleichspunkt, 'Methode der Perser, und indische Planetenrechnung"
-
made the original suggestion and offered a justification based on a power series analysis. More recently Dennis Duke, "The equant in India: The basis of ancient Indian planetary models" (2004, submitted), has presented detailed numerical comparisons that remove any doubt that in fact the bisected equant underlies the Indian planetary models
-
B. L. van der Waerden, "Ausgleichspunkt, 'Methode der Perser, und indische Planetenrechnung", Archive for history of exact sciences, i (1961), 107-21, made the original suggestion and offered a justification based on a power series analysis. More recently Dennis Duke, "The equant in India: The basis of ancient Indian planetary models" (2004, submitted), has presented detailed numerical comparisons that remove any doubt that in fact the bisected equant underlies the Indian planetary models.
-
(1961)
Archive for History of Exact Sciences
, vol.1
, pp. 107-121
-
-
van der Waerden, B.L.1
-
10
-
-
4243993130
-
"The Paitamahasiddhanta of the Visnudharmottapurana"
-
D. Pingree, "The Paitamahasiddhanta of the Visnudharmottapurana", Brahmavidya, xxxi-xxxii (1967-68),472-510;
-
(1967)
Brahmavidya
, vol.31-32
, pp. 472-510
-
-
Pingree, D.1
-
14
-
-
26444493068
-
"On the Greek origin of the Indian planetary model employing a double epicycle"
-
D. Pingree, "On the Greek origin of the Indian planetary model employing a double epicycle", Journal for the history of astronomy, ii (1971), 80-85;
-
(1971)
Journal for the History of Astronomy
, vol.2
, pp. 80-85
-
-
Pingree, D.1
-
15
-
-
84965395238
-
"The recovery of early Greek astronomy from India"
-
idem, "The recovery of early Greek astronomy from India", Journal for the history of astronomy, vii (1976), 109-123;
-
(1976)
Journal for the History of Astronomy
, vol.7
, pp. 109-123
-
-
Pingree, D.1
-
16
-
-
0001027296
-
"History of mathematical astronomy in India"
-
and idem, "History of mathematical astronomy in India", Dictionary of scientific biography, xv (1978), 533-633.
-
(1978)
Dictionary of Scientific Biography
, vol.15
, pp. 533-633
-
-
Pingree, D.1
|