The basic characteristics of solar and lunar eclipses from –2999 to +3000 have been calculated by Fred Espenak and can be accessed from his comprehensive eclipse website:
Fred Espenak’s website also provides global maps of solar eclipse paths from 2000 BCE to 3000 CE in 20-year period intervals:
Similar eclipse catalogues have been prepared by Felix Verbelen (Mira Public Observatory, Grimbergen, Belgium) and can be accessed from his Ancient Astronomy Home Page:
The following printed works provide tables of solar and lunar eclipses with maps of solar eclipse paths covering extended geographical regions and historical periods:
| Whole World | Solar eclipses | Lunar eclipses |
| Lacaille & Pingré (1770) [northern hemisphere only] | +1 to +1900 | +1 to +1900 |
| Duvauchel (1783) [northern hemisphere only] | +1900 to +2000 | +1900 to +2000 |
| Pingré (1787) [northern hemisphere only] | –999 to 0 | –999 to 0 |
| Mahler (1885) | +1901 to +2000 | – |
| Von Oppolzer (1887) | –1207 to +2161 | –1206 to +2163 |
| Van den Bergh (1954) | –1600 to –1207 | –1600 to –1207 |
| Meeus et al. (1966) | +1898 to +2510 | – |
| Mucke & Meeus (1983) | –2003 to +2526 | – |
| Meeus & Mucke (1983) | – | –2003 to +2526 |
| Espenak (1987) | +1986 to +2035 | – |
| Espenak (1989) | – | +1986 to +2035 |
| Meeus (1989) | +1950 to +2200 | – |
| Bao-Lin Liu & Fiala (1992) | – | –1499 to +3000 |
| Espenak & Meeus (2006) | –1999 to +3000 | – |
| Espenak & Meeus (2009) | – | –1999 to +3000 |
| Ancient Near East | Solar eclipses | Lunar eclipses |
| Neugebauer & Hiller (1931) | –4199 to –899 | – |
| Neugebauer & Hiller (1934) | – | –3449 to 0 |
| Dubs (1947) | – | –1400 to –1000 |
| Kudlek & Mickler (1971) | –2999 to 0 | –2999 to 0 |
| Steele & Stephenson (1997/98) | –749 to +1 | –749 to +1 |
| Mediterranean region | Solar eclipses | Lunar eclipses |
| Ginzel (1887) | –799 to 0 | –399 to 0 |
| Ginzel (1899) | –899 to +600 | –899 to +600 |
| Europe | Solar eclipses | Lunar eclipses |
| Lacaille (1750) | +1 to +1800 | +1 to +1800 |
| Schroeter (1923) | +600 to +1800 | +600 to +1800 |
| Ireland | Solar eclipses | Lunar eclipses |
| O’Connor (1952) | +400 to +1000 | – |
| Africa | Solar eclipses | Lunar eclipses |
| Gray (1965, 1968) | +1000 to +2000 | – |
| East Asia | Solar eclipses | Lunar eclipses |
| Dubs (1947) | – | –1400 to –1000 |
| Newton (1972, 1977) | –1500 to –1000 | –1500 to –1000 |
| Stephenson & Houlden (1986) | –1499 to +1900 | – |
| Central America | Solar eclipses | Lunar eclipses |
| Willson (1924) | +638 to +728 | – |
Shinobu Takesako’s freeware programs EmapWin and LmapWin also provide very accurate calculations for the circumstances of solar and lunar eclipses from 3000 B.C. to A.D. 3000.