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Detected from this, among other things
Total duration . . . . . . . 3 h. 34' 50''
Delay . . . . . . . . . . . . 1 h. 25' 30''
Time of incidence . . . . 1 h. 5' 10''
Quantity . . . . . . . . . . . 10 Digits 28'
Geometric diagram showing the "Path of the center of the shadow" and various phases labeled: "Start VIII," "Total immersion," "Total emersion," "Ecliptic end." Specific points are marked: "Point of initial eastern contact," "Point of total loss," "Point of total emergence," "Point of final western contact."
| Calculation moments. | h. | ' | '' |
|---|---|---|---|
| True time of the plenilunium full moon at Nuremberg, year 1750, June 19, in the afternoon | 8 | 58 | 21 |
| True place of the Sun | 28 | 32 | 36 Gemini |
| True place of the Moon in orbit | 28 | 16 | 52 Sagittarius |
| True longitude of the Moon | 28 | 16 | 52 Sagittarius |
| True southern latitude of the Moon, decreasing | 0 | 12 | 11 |
| Semidiameter of the Sun | 15 | 50 | |
| Horizontal semidiameter of the Moon | 15 | 24 | |
| Horizontal parallax of the Moon | 56 | 4 | |
| Parallax of the Sun | 9 | ||
| Semidiameter of the Earth's shadow | 41 | 16 | |
| Hourly movement of the Sun | 2 | 23 | |
| True hourly movement of the Moon in orbit | 31 | 14 | |
| Hourly movement of the Moon from the Sun | 28 | 51 | |
| Inclination of the path of the Moon's orbit to the ecliptic | 5 | 8 | |
| Northern declination of the Sun | 23 | 28 | 13 |
| Wittenberg | Paris | Berlin | London | Gdansk | Bologna | |
|---|---|---|---|---|---|---|
| Beginning | 7h 26' 28'' | 6h 34' 15'' | 7h 23' 5'' | 6h 24' 15'' | 7h 44' 35'' | 7h 7' 5'' |
| Immersion | 8h 31' 38'' | 7h 39' 25'' | 8h 28' 15'' | 7h 29' 25'' | 8h 49' 45'' | 8h 12' 15'' |
| Delay | 9h 14' 23'' | 8h 22' 10'' | 9h 11' 0'' | 8h 12' 10'' | 9h 32' 30'' | 8h 54' 50'' |
| Emersion | 9h 57' 8'' | 9h 4' 55'' | 9h 53' 45'' | 8h 54' 55'' | 10h 15' 15'' | 9h 37' 45'' |
| End | 11h 2' 18'' | 10h 10' 5'' | 10h 58' 55'' | 10h 0' 5'' | 11h 20' 25'' | 10h 42' 55'' |
| Quantity | 20 4/5 dig. | everywhere |
| Dig. | Time | Features | Dig. | Time | Features | ||
|---|---|---|---|---|---|---|---|
| In | 1. | 7. 21. 30 | Aristarchus | Ex | 1. | 10. 10. 30 | Grimaldi |
| 2. | 7. 26. 15 | Grimaldi | 2. | 10. 13. 5 | Aristarchus | ||
| 3. | 7. 32. 0 | Mareotis Sea | 3. | 10. 16. 25 | Kepler | ||
| 4. | 7. 38. 50 | Helicon | 4. | 10. 19. 40 | Porphyrites Sea | ||
| 5. | 7. 43. 30 | Island of Error and Sinai Sea | 5. | 10. 25. 10 | Gassendi | ||
| 6. | 7. 52. 40 | Sinai Sea | 6. | 10. 29. 25 | Sinai Sea | ||
| 7. | 8. 1. 20 | Lebanon Sea | 7. | 10. 36. 35 | Sinai Sea | ||
| 8. | 8. 10. 30 | Lip. Major Sea | 8. | 10. 43. 40 | Copernicus | ||
| 9. | 8. 14. 0 | Astronomers' Promontory | 9. | 10. 48. 10 | Tycho | ||
| 10. | 8. 20. 20 | Tycho | 10. | 10. 53. 5 | Carpathus Sea | ||
| 11. | 8. 23. 15 | Plato | 11. | 10. 57. 30 | Etna Sea | ||
| 12. | 8. 26. 45 | Etna Sea | 12. | 11. 1. 10 | Menelaus |
Semidiameter of the Earth's shadow . . . . 41'. 16''.
Hourly movement of Moon from Sun in orbit . . . . 28. 51.
Scale of the whole degree or sixty individual minutes
Ecliptic digits
North
A circular diagram representing the Earth's shadow ("Earth's shadow") with the moon's path crossing it. The moon is shown at the point of "Beginning" (start) on the right and "End" (end) on the left. The celestial coordinates are marked: "North," "South," "East," "West." The "Ecliptic" line passes through the shadow.