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Mean motions and longitudes in indian astronomy
| Content Provider | Semantic Scholar |
|---|---|
| Author | Duke, Dennis W. |
| Copyright Year | 2008 |
| Abstract | The astronomy we find in texts from ancient India is similar to that we know from ancient Greco-Roman sources, so much so that the prevailing view is that astronomy in India was in large part adapted from Greco-Roman sources transmitted to India. However, there are sometimes differences in the details of how fundamental ideas are implemented. One such area is the technique for dealing with mean motions and longitudes. The Greek methods explained by Ptolemy are essentially identical to what we use today: one specifies a mean longitude 0 λ for some specific day and time – the epoch |
| Starting Page | 489 |
| Ending Page | 509 |
| Page Count | 21 |
| File Format | PDF HTM / HTML |
| DOI | 10.1007/s00407-008-0022-1 |
| Volume Number | 62 |
| Alternate Webpage(s) | http://people.sc.fsu.edu/~dduke/ndviii1.pdf |
| Alternate Webpage(s) | http://people.sc.fsu.edu/~dduke/MeanLongs.pdf |
| Language | English |
| Access Restriction | Open |
| Content Type | Text |
| Resource Type | Article |