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Hermit Eclipse

Eclipse Search



Listing of Eclipses:

- of Saros series 146
- of types: Lunar: penumbral partial total
 Date       Time  Type   Sar   P-Mag  U-Mag  Gamma  P-Durn  T-Durn Lat    Long
 1843/07/11 16:50 L,N    146B  0.048 -0.978  1.547                             
 1861/07/21 23:50 L,N    146   0.195 -0.828  1.466                             
 1879/08/02 06:58 L,N    146   0.335 -0.686  1.389                             
 1897/08/12 14:09 L,N    146   0.473 -0.546  1.314                             
 1915/08/24 21:27 L,N    146   0.600 -0.417  1.244                             
 1933/09/04 04:52 L,N    146   0.721 -0.296  1.178                             
 1951/09/15 12:27 L,N    146   0.828 -0.188  1.119                             
 1969/09/25 20:10 L,N    146   0.926 -0.090  1.066                             
 1987/10/07 04:02 L,N    146   1.011 -0.004  1.019                             
 2005/10/17 12:03 L,P    146   1.084  0.068  0.980  58m00s                     
 2023/10/28 20:14 L,P    146   1.143  0.127  0.947  80m00s                     
 2041/11/08 04:33 L,P    146   1.191  0.175  0.921  92m00s                     
 2059/11/19 12:59 L,P    146   1.229  0.213  0.900 100m00s                     
 2077/11/29 21:33 L,P    146   1.256  0.241  0.886 106m00s                     
 2095/12/11 06:12 L,P    146   1.276  0.262  0.874 110m00s                     
 2113/12/22 14:55 L,P    146   1.289  0.276  0.867 112m00s                     
 2132/01/02 23:40 L,P    146   1.300  0.289  0.861 114m00s                     
 2150/01/13 08:26 L,P    146   1.308  0.299  0.856 116m00s                     
 2168/01/24 17:12 L,P    146   1.319  0.312  0.849 118m00s                     
 2186/02/04 01:55 L,P    146   1.333  0.329  0.841 122m00s                     
 2204/02/16 10:34 L,P    146   1.352  0.352  0.829 124m00s                     
 2222/02/26 19:10 L,P    146   1.377  0.381  0.814 128m00s                     
 2240/03/09 03:38 L,P    146   1.414  0.422  0.793 134m00s                     
 2258/03/20 12:01 L,P    146   1.460  0.473  0.767 142m00s                     
 2276/03/30 20:16 L,P    146   1.518  0.535  0.734 148m00s                     
 2294/04/11 04:25 L,P    146   1.585  0.606  0.696 156m00s                     
 2312/04/22 12:25 L,P    146   1.667  0.692  0.650 164m00s                     
 2330/05/03 20:20 L,P    146   1.757  0.786  0.600 172m00s                     
 2348/05/14 04:07 L,P    146   1.861  0.893  0.543 180m00s                     
 2366/05/25 11:50 L,T    146   1.971  1.006  0.482 188m00s  12m00s             
 2384/06/04 19:26 L,T    146   2.092  1.129  0.415 194m00s  52m00s             
 2402/06/16 03:00 L,T    146   2.217  1.256  0.347 200m00s  70m00s             
 2420/06/26 10:30 L,T    146   2.350  1.390  0.274 204m00s  82m00s             
 2438/07/07 17:58 L,T/S- 146   2.484  1.525  0.201 208m00s  92m00s             
 2456/07/18 01:25 L,T/S- 146   2.621  1.662  0.126 210m00s  96m00s             
 2474/07/29 08:54 L,T/S- 146   2.756  1.796  0.053 212m00s 100m00s             
 2492/08/08 16:25 L,T    146M  2.819  1.858 -0.019 212m00s 100m00s             
 2510/08/20 23:58 L,T/N- 146   2.693  1.729 -0.088 212m00s  98m00s             
 2528/08/31 07:35 L,T/N- 146   2.573  1.607 -0.154 210m00s  94m00s             
 2546/09/11 15:17 L,T/N- 146   2.461  1.492 -0.216 208m00s  90m00s             
 2564/09/21 23:05 L,T    146   2.359  1.386 -0.273 206m00s  82m00s             
 2582/10/03 07:00 L,T    146   2.268  1.291 -0.324 202m00s  74m00s             
 2600/10/14 15:01 L,T    146   2.188  1.207 -0.368 198m00s  64m00s             
 2618/10/25 23:10 L,T    146   2.120  1.135 -0.407 196m00s  52m00s             
 2636/11/05 07:25 L,T    146   2.061  1.072 -0.440 192m00s  40m00s             
 2654/11/16 15:48 L,T    146   2.016  1.022 -0.466 190m00s  22m00s             
 2672/11/27 00:16 L,P    146   1.980  0.982 -0.486 188m00s                     
 2690/12/08 08:51 L,P    146   1.954  0.952 -0.501 186m00s                     
 2708/12/19 17:29 L,P    146   1.933  0.928 -0.514 186m00s                     
 2726/12/31 02:11 L,P    146   1.920  0.912 -0.522 184m00s                     

Displayed matches 1 - 50 of 65

Note that the database does not contain the whole of lunar Saros series 146, 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 $)