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Eclipse Search



Listing of Eclipses:

- of Saros series 138
- of types: Lunar: penumbral partial total
 Date       Time  Type   Sar   P-Mag  U-Mag  Gamma  P-Durn  T-Durn Lat    Long
 1503/10/05 15:16 L,N    138B  0.021 -0.967  1.551                             
 1521/10/15 23:39 L,N    138   0.065 -0.928  1.529                             
 1539/10/27 08:08 L,N    138   0.097 -0.900  1.512                             
 1557/11/06 16:43 L,N    138   0.122 -0.879  1.500                             
 1575/11/18 01:23 L,N    138   0.136 -0.869  1.493                             
 1593/12/08 10:06 L,N    138   0.144 -0.864  1.490                             
 1611/12/19 18:53 L,N    138   0.147 -0.864  1.489                             
 1629/12/30 03:39 L,N    138   0.148 -0.865  1.489                             
 1648/01/10 12:25 L,N    138   0.148 -0.867  1.489                             
 1666/01/20 21:09 L,N    138   0.151 -0.866  1.488                             
 1684/02/01 05:48 L,N    138   0.158 -0.859  1.485                             
 1702/02/12 14:21 L,N    138   0.171 -0.847  1.478                             
 1720/02/23 22:48 L,N    138   0.192 -0.826  1.466                             
 1738/03/06 07:07 L,N    138   0.224 -0.794  1.449                             
 1756/03/16 15:18 L,N    138   0.266 -0.752  1.426                             
 1774/03/27 23:19 L,N    138   0.321 -0.697  1.396                             
 1792/04/07 07:12 L,N    138   0.387 -0.631  1.360                             
 1810/04/19 14:54 L,N    138   0.467 -0.551  1.316                             
 1828/04/29 22:28 L,N    138   0.557 -0.462  1.267                             
 1846/05/11 05:54 L,N    138   0.661 -0.359  1.211                             
 1864/05/21 13:12 L,N    138   0.773 -0.248  1.150                             
 1882/06/01 20:22 L,N    138   0.897 -0.126  1.083                             
 1900/06/13 03:28 L,P    138   1.026  0.001  1.013   8m00s                     
 1918/06/24 10:28 L,P    138   1.163  0.135  0.940  84m00s                     
 1936/07/04 17:25 L,P    138   1.303  0.272  0.864 118m00s                     
 1954/07/16 00:20 L,P    138   1.446  0.411  0.788 142m00s                     
 1972/07/26 07:16 L,P    138   1.587  0.548  0.712 162m00s                     
 1990/08/06 14:12 L,P    138   1.726  0.681  0.638 176m00s                     
 2008/08/16 21:10 L,P    138   1.862  0.812  0.565 188m00s                     
 2026/08/28 04:13 L,P    138   1.990  0.935  0.497 198m00s                     
 2044/09/07 11:19 L,T    138   2.111  1.050  0.432 206m00s  36m00s             
 2062/09/18 18:32 L,T    138   2.221  1.154  0.374 214m00s  60m00s             
 2080/09/29 01:50 L,T    138   2.322  1.249  0.321 218m00s  74m00s             
 2098/10/10 09:16 L,T    138   2.409  1.329  0.275 222m00s  84m00s             
 2116/10/21 16:49 L,T/S- 138   2.484  1.399  0.236 224m00s  90m00s             
 2134/11/02 00:30 L,T/S- 138   2.548  1.456  0.202 226m00s  94m00s             
 2152/11/12 08:16 L,T/S- 138   2.600  1.503  0.176 228m00s  96m00s             
 2170/11/23 16:10 L,T/S- 138   2.639  1.537  0.156 230m00s  98m00s             
 2188/12/04 00:09 L,T/S- 138   2.670  1.564  0.140 230m00s 100m00s             
 2206/12/16 08:12 L,T/S- 138   2.694  1.584  0.128 230m00s 100m00s             
 2224/12/26 16:17 L,T/S- 138   2.713  1.600  0.119 232m00s 102m00s             
 2243/01/07 00:25 L,T    138M  2.726  1.611  0.112 232m00s 102m00s             
 2261/01/17 08:30 L,T/S- 138   2.741  1.625  0.104 232m00s 102m00s             
 2279/01/28 16:35 L,T/S- 138   2.757  1.639  0.096 234m00s 102m00s             
 2297/02/08 00:35 L,T/S- 138   2.779  1.661  0.084 234m00s 104m00s             
 2315/02/20 08:31 L,T/S- 138   2.806  1.689  0.069 234m00s 104m00s             
 2333/03/02 16:17 L,T/S- 138   2.845  1.730  0.047 234m00s 106m00s             
 2351/03/13 23:59 L,T/S- 138   2.892  1.778  0.021 236m00s 106m00s             
 2369/03/24 07:29 L,T/N- 138   2.906  1.794 -0.013 236m00s 106m00s             
 2387/04/04 14:52 L,T/N- 138   2.830  1.721 -0.054 236m00s 106m00s             

Displayed matches 1 - 50 of 83


Query the Eclipse Database

Search from Year: To Year: inclusive

for all eclipses
for eclipses:
Solar: Partial Total Annular Hybrid
Lunar: Penumbral Partial Total
in Saros series:
of penumbral magnitude:
lunar eclipses only
of umbral magnitude:
of absolute gamma:
treats all gammas as +ve
of partial duration:
lunar eclipses only
m s
of total duration: m s
on day: in month:
for calendar years:
with at least: eclipses
with at least: total solar eclipses
with at least: total lunar eclipses

The database contains all solar and lunar eclipses from 2000 BC to 3000 AD inclusive. BC years are shown in negative notation, as used by astronomers; 1 BC is year 0, 2 BC is year -1, etc.; so 2000 BC is -1999.

To do a search, pick a range of years to search, or leave those fields blank to search the whole database. Then pick a search type:

you can search for all eclipses in the chosen range of years;
or for eclipses in a particular Saros series and/or of a given type;
or for years where a certain number of eclipses occur, or a certain number of total eclipses (for example, to find a year with 4 eclipses).

Bear in mind that if a Saros started before 2000 BC, or ends after 3000 AD, only part of the series will be shown.

Any field left blank will match all possible values for that field. Leaving all the fields blank, and selecting all the eclipse types, will return the whole database; since this is huge, the results are broken up into pages. Go to the eclipse stats page to see how you can get the whole database, and the search engine.

Key to Fields

Date / Time
The date and time of the moment of greatest eclipse. This is the instant when the axis of the Moon's shadow passes closest to the Earth's center. The date format is year/month/day, and the year is always shown in full; so, a date like "97/03/17" means the 17th of March, year 97 AD (not 1997); and bearing in mind the astronomical notation for BC years, "-19/03/17" means the 17th of March, year 20 BC.

All dates in the database up to Oct 04, 1582 are in the Julian calendar; all dates after Oct 15 1582 are Gregorian.

For total eclipses, the instant of greatest eclipse is virtually identical to the instants of greatest magnitude and greatest duration.

Type
The type of the eclipse. The first letter is one of:
S
A solar eclipse. The following letter is the type: P=partial; T=total; A=annular; H=hybrid.
L
A lunar eclipse. The following letter is the type: N=penumbral; P=partial; T=total.

The following notations may also appear:

N
The northern edge of the eclipse is off the north end of the Earth.
N-
The northern edge and the centre of the eclipse are off the north end of the Earth.
S
The southern edge of the eclipse is off the south end of the Earth.
S-
The southern edge and the centre of the eclipse are off the south end of the Earth.
Note that in a partial eclipse, the centre of the eclipse always misses the Earth.
Saros
The Saros series of the eclipse.

The following notations may also appear:

B
This is the first eclipse in this series.
M
This is the middle eclipse in this series.
E
This is the last eclipse in this series.
P-Mag
The penumbral magnitude of a lunar eclipse (doesn't apply to solar eclipses); the fraction of the Moon's diameter which is obscured by the penumbra.
U-Mag
The umbral magnitude of the eclipse. For a lunar eclipse, this is the fraction of the Moon's diameter obscured by the umbra; for a solar eclipse, it is the fraction of the Sun's diameter which is obscured at the moment of greatest eclipse.
Gamma
The distance of the the axis of the Moon's shadow from the Earth's center at maximum eclipse, measured as a fraction of the Earth's radius. A negative value indicates that the eclipse is below the centre of the Earth as seen from the Sun; this is not necessarily the same as being centred south of the equator, due to the Earth's tilt. The search form looks at absolute value of gamma -- ie. it treats all values as positive -- so that you can search for eg. all marginal eclipses without having to do two searches. Hence searching for values < 0 will return nothing.
P-Durn
For a lunar eclipse, this is the duration of the partial eclipse (if any) at the point of greatest eclipse (doesn't apply to solar eclipses).
T-Durn
For a lunar eclipse, this is the duration of the total (umbral) eclipse (if any); for a solar eclipse, it is the duration of the total or annular eclipse (if any) at the point of greatest eclipse.
Lat/Long
The location on the Earth's surface at which the greatest eclipse will be seen. This applies to solar eclipses only.

Copyright (C) 1995-2006 Ian Cameron Smith.
visits since 18Aug05. Last modified: Sat May 3 11:44:23 PDT 2008 ($Revision: 1.1 $)