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Hermit Eclipse

Eclipse Search



Listing of Eclipses:

- of Saros series 134
- of types: Lunar: penumbral partial total
 Date       Time  Type   Sar   P-Mag  U-Mag  Gamma  P-Durn  T-Durn Lat    Long
 1550/04/01 12:52 L,N    134B  0.028 -0.971  1.550                             
 1568/04/11 20:37 L,N    134   0.123 -0.870  1.497                             
 1586/05/03 04:15 L,N    134   0.231 -0.758  1.437                             
 1604/05/13 11:48 L,N    134   0.346 -0.638  1.373                             
 1622/05/24 19:17 L,N    134   0.469 -0.510  1.304                             
 1640/06/04 02:44 L,N    134   0.597 -0.379  1.234                             
 1658/06/15 10:07 L,N    134   0.732 -0.240  1.159                             
 1676/06/25 17:32 L,N    134   0.868 -0.103  1.085                             
 1694/07/07 00:55 L,P    134   1.006  0.038  1.009  42m00s                     
 1712/07/18 08:22 L,P    134   1.141  0.174  0.935  90m00s                     
 1730/07/29 15:50 L,P    134   1.275  0.308  0.862 116m00s                     
 1748/08/08 23:23 L,P    134   1.402  0.435  0.793 136m00s                     
 1766/08/20 07:01 L,P    134   1.523  0.555  0.727 150m00s                     
 1784/08/30 14:46 L,P    134   1.635  0.666  0.666 162m00s                     
 1802/09/11 22:36 L,P    134   1.738  0.768  0.610 170m00s                     
 1820/09/22 06:35 L,P    134   1.830  0.857  0.561 178m00s                     
 1838/10/03 14:41 L,P    134   1.910  0.935  0.518 182m00s                     
 1856/10/13 22:54 L,T    134   1.980  1.002  0.481 186m00s   6m00s             
 1874/10/25 07:16 L,T    134   2.036  1.056  0.451 190m00s  34m00s             
 1892/11/04 15:45 L,T    134   2.082  1.099  0.427 192m00s  46m00s             
 1910/11/17 00:21 L,T    134   2.116  1.131  0.409 194m00s  52m00s             
 1928/11/27 09:01 L,T    134   2.142  1.155  0.395 194m00s  56m00s             
 1946/12/08 17:48 L,T    134   2.159  1.170  0.386 196m00s  58m00s             
 1964/12/19 02:37 L,T    134   2.171  1.180  0.380 196m00s  60m00s             
 1982/12/30 11:29 L,T    134   2.180  1.188  0.376 196m00s  62m00s             
 2001/01/09 20:21 L,T    134   2.187  1.194  0.372 198m00s  62m00s             
 2019/01/21 05:12 L,T    134   2.193  1.201  0.369 198m00s  62m00s             
 2037/01/31 14:00 L,T    134   2.205  1.213  0.362 198m00s  64m00s             
 2055/02/11 22:44 L,T    134   2.222  1.230  0.353 200m00s  66m00s             
 2073/02/22 07:22 L,T    134   2.247  1.256  0.339 200m00s  70m00s             
 2091/03/05 15:55 L,T    134   2.278  1.288  0.322 202m00s  74m00s             
 2109/03/17 00:19 L,T    134   2.324  1.335  0.296 204m00s  78m00s             
 2127/03/28 08:36 L,T/S- 134   2.378  1.390  0.267 206m00s  84m00s             
 2145/04/07 16:43 L,T/S- 134   2.447  1.460  0.229 208m00s  88m00s             
 2163/04/19 00:44 L,T/S- 134   2.524  1.539  0.186 210m00s  92m00s             
 2181/04/29 08:34 L,T/S- 134   2.618  1.633  0.135 214m00s  96m00s             
 2199/05/10 16:18 L,T    134M  2.719  1.735  0.080 214m00s 100m00s             
 2217/05/21 23:54 L,T/S- 134   2.834  1.849  0.017 216m00s 102m00s             
 2235/06/02 07:24 L,T/N- 134   2.776  1.790 -0.049 216m00s 100m00s             
 2253/06/12 14:48 L,T/N- 134   2.645  1.658 -0.121 216m00s  98m00s             
 2271/06/23 22:09 L,T/N- 134   2.512  1.523 -0.194 214m00s  94m00s             
 2289/07/04 05:26 L,T/N- 134   2.373  1.382 -0.270 210m00s  84m00s             
 2307/07/16 12:40 L,T    134   2.233  1.239 -0.347 206m00s  70m00s             
 2325/07/26 19:54 L,T    134   2.094  1.096 -0.424 200m00s  46m00s             
 2343/08/07 03:08 L,P    134   1.957  0.955 -0.500 192m00s                     
 2361/08/17 10:24 L,P    134   1.824  0.817 -0.574 182m00s                     
 2379/08/28 17:43 L,P    134   1.697  0.686 -0.644 172m00s                     
 2397/09/08 01:05 L,P    134   1.579  0.562 -0.710 158m00s                     
 2415/09/19 08:33 L,P    134   1.471  0.447 -0.771 144m00s                     
 2433/09/29 16:06 L,P    134   1.371  0.341 -0.827 128m00s                     

Displayed matches 1 - 50 of 73


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 $)