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Hermit Eclipse

Eclipse Search



Listing of Eclipses:

- of Saros series 149
- of types: Lunar: penumbral partial total
 Date       Time  Type   Sar   P-Mag  U-Mag  Gamma  P-Durn  T-Durn Lat    Long
 1984/06/13 14:26 L,N    149B  0.090 -0.936 -1.524                             
 2002/06/24 21:27 L,N    149   0.235 -0.787 -1.444                             
 2020/07/05 04:30 L,N    149   0.380 -0.638 -1.364                             
 2038/07/16 11:34 L,N    149   0.525 -0.490 -1.284                             
 2056/07/26 18:41 L,N    149   0.669 -0.344 -1.205                             
 2074/08/07 01:53 L,N    149   0.806 -0.204 -1.129                             
 2092/08/17 09:11 L,N    149   0.938 -0.071 -1.057                             
 2110/08/29 16:35 L,P    149   1.061  0.054 -0.990  52m00s                     
 2128/09/09 00:06 L,P    149   1.176  0.169 -0.927  92m00s                     
 2146/09/20 07:46 L,P    149   1.278  0.272 -0.871 114m00s                     
 2164/09/30 15:35 L,P    149   1.370  0.363 -0.821 130m00s                     
 2182/10/11 23:32 L,P    149   1.449  0.442 -0.778 140m00s                     
 2200/10/23 07:38 L,P    149   1.516  0.509 -0.741 148m00s                     
 2218/11/03 15:53 L,P    149   1.571  0.564 -0.712 154m00s                     
 2236/11/14 00:16 L,P    149   1.614  0.607 -0.688 158m00s                     
 2254/11/25 08:46 L,P    149   1.648  0.640 -0.670 162m00s                     
 2272/12/05 17:22 L,P    149   1.672  0.664 -0.657 164m00s                     
 2290/12/17 02:05 L,P    149   1.688  0.681 -0.648 166m00s                     
 2308/12/28 10:50 L,P    149   1.701  0.695 -0.641 166m00s                     
 2327/01/08 19:38 L,P    149   1.710  0.706 -0.635 168m00s                     
 2345/01/19 04:25 L,P    149   1.719  0.717 -0.629 168m00s                     
 2363/01/30 13:13 L,P    149   1.729  0.729 -0.624 168m00s                     
 2381/02/09 21:56 L,P    149   1.746  0.749 -0.614 170m00s                     
 2399/02/21 06:37 L,P    149   1.766  0.772 -0.602 172m00s                     
 2417/03/03 15:11 L,P    149   1.796  0.806 -0.584 174m00s                     
 2435/03/14 23:40 L,P    149   1.834  0.848 -0.563 178m00s                     
 2453/03/25 08:01 L,P    149   1.885  0.903 -0.534 182m00s                     
 2471/04/05 16:17 L,P    149   1.945  0.966 -0.500 186m00s                     
 2489/04/16 00:24 L,T    149   2.018  1.043 -0.459 190m00s  30m00s             
 2507/04/28 08:24 L,T    149   2.102  1.131 -0.412 194m00s  52m00s             
 2525/05/08 16:17 L,T    149   2.198  1.229 -0.360 198m00s  66m00s             
 2543/05/20 00:05 L,T    149   2.302  1.336 -0.302 202m00s  78m00s             
 2561/05/30 07:46 L,T/N- 149   2.417  1.453 -0.239 206m00s  88m00s             
 2579/06/10 15:22 L,T/N- 149   2.539  1.577 -0.172 210m00s  94m00s             
 2597/06/20 22:55 L,T/N- 149   2.668  1.707 -0.101 212m00s  98m00s             
 2615/07/03 06:25 L,T    149M  2.799  1.839 -0.029 212m00s 100m00s             
 2633/07/13 13:53 L,T/S- 149   2.771  1.810  0.045 212m00s 100m00s             
 2651/07/24 21:21 L,T/S- 149   2.636  1.675  0.118 212m00s  98m00s             
 2669/08/04 04:49 L,T/S- 149   2.502  1.540  0.192 208m00s  92m00s             
 2687/08/15 12:20 L,T/S- 149   2.373  1.409  0.263 206m00s  84m00s             
 2705/08/26 19:51 L,T    149   2.247  1.280  0.332 202m00s  74m00s             
 2723/09/07 03:29 L,T    149   2.131  1.161  0.396 196m00s  58m00s             
 2741/09/17 11:10 L,T    149   2.022  1.048  0.457 192m00s  32m00s             
 2759/09/28 18:58 L,P    149   1.924  0.946  0.511 186m00s                     
 2777/10/09 02:51 L,P    149   1.834  0.852  0.561 178m00s                     
 2795/10/20 10:53 L,P    149   1.759  0.772  0.604 172m00s                     
 2813/10/30 19:00 L,P    149   1.693  0.701  0.641 166m00s                     
 2831/11/11 03:15 L,P    149   1.638  0.642  0.672 162m00s                     
 2849/11/21 11:36 L,P    149   1.594  0.593  0.697 156m00s                     
 2867/12/02 20:04 L,P    149   1.560  0.555  0.717 152m00s                     

Displayed matches 1 - 50 of 57

Note that the database does not contain the whole of lunar Saros series 149, since it ends after year 3000.


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 $)