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Hermit Eclipse

Eclipse Search



Listing of Eclipses:

- of Saros series 142
- of types: Lunar: penumbral partial total
 Date       Time  Type   Sar   P-Mag  U-Mag  Gamma  P-Durn  T-Durn Lat    Long
 1709/09/19 00:30 L,N    142B  0.091 -1.008  1.544                             
 1727/09/30 07:40 L,N    142   0.183 -0.921  1.495                             
 1745/10/10 14:57 L,N    142   0.265 -0.844  1.451                             
 1763/10/21 22:22 L,N    142   0.334 -0.779  1.415                             
 1781/11/01 05:56 L,N    142   0.391 -0.726  1.385                             
 1799/11/12 13:38 L,N    142   0.436 -0.685  1.362                             
 1817/11/23 21:27 L,N    142   0.471 -0.653  1.343                             
 1835/12/05 05:20 L,N    142   0.498 -0.628  1.329                             
 1853/12/15 13:19 L,N    142   0.518 -0.609  1.319                             
 1871/12/26 21:19 L,N    142   0.533 -0.595  1.311                             
 1890/01/06 05:21 L,N    142   0.547 -0.581  1.303                             
 1908/01/18 13:21 L,N    142   0.564 -0.564  1.294                             
 1926/01/28 21:20 L,N    142   0.582 -0.544  1.284                             
 1944/02/09 05:15 L,N    142   0.606 -0.518  1.270                             
 1962/02/19 13:03 L,N    142   0.638 -0.482  1.251                             
 1980/03/01 20:45 L,N    142   0.681 -0.436  1.227                             
 1998/03/13 04:20 L,N    142   0.735 -0.378  1.196                             
 2016/03/23 11:47 L,N    142   0.801 -0.308  1.159                             
 2034/04/03 19:05 L,N    142   0.881 -0.223  1.115                             
 2052/04/14 02:16 L,N    142   0.972 -0.126  1.063                             
 2070/04/25 09:19 L,N    142   1.077 -0.017  1.005                             
 2088/05/05 16:14 L,P    142   1.195  0.106  0.939  78m00s                     
 2106/05/17 23:03 L,P    142   1.323  0.239  0.868 116m00s                     
 2124/05/28 05:47 L,P    142   1.461  0.381  0.792 142m00s                     
 2142/06/08 12:28 L,P    142   1.605  0.529  0.712 164m00s                     
 2160/06/18 19:05 L,P    142   1.757  0.685  0.628 182m00s                     
 2178/06/30 01:42 L,P    142   1.909  0.841  0.544 196m00s                     
 2196/07/10 08:19 L,T    142   2.066  1.000  0.458 206m00s   4m00s             
 2214/07/22 14:59 L,T    142   2.219  1.156  0.374 214m00s  62m00s             
 2232/08/01 21:42 L,T    142   2.372  1.310  0.290 222m00s  82m00s             
 2250/08/13 04:31 L,T/S- 142   2.516  1.456  0.211 226m00s  94m00s             
 2268/08/23 11:25 L,T/S- 142   2.654  1.596  0.135 228m00s 100m00s             
 2286/09/03 18:27 L,T/S- 142   2.782  1.725  0.065 228m00s 104m00s             
 2304/09/15 01:37 L,T/S- 142   2.901  1.844  0.001 228m00s 104m00s             
 2322/09/26 08:57 L,T/N- 142   2.798  1.742 -0.056 228m00s 104m00s             
 2340/10/06 16:26 L,T/N- 142   2.705  1.649 -0.107 226m00s 102m00s             
 2358/10/18 00:05 L,T/N- 142   2.626  1.569 -0.150 224m00s  98m00s             
 2376/10/28 07:54 L,T    142M  2.559  1.503 -0.187 222m00s  94m00s             
 2394/11/08 15:52 L,T/N- 142   2.506  1.450 -0.215 220m00s  92m00s             
 2412/11/18 23:58 L,T/N- 142   2.464  1.409 -0.238 218m00s  88m00s             
 2430/11/30 08:13 L,T/N- 142   2.434  1.379 -0.254 216m00s  86m00s             
 2448/12/10 16:33 L,T/N- 142   2.412  1.358 -0.266 214m00s  84m00s             
 2466/12/22 01:01 L,T    142   2.398  1.346 -0.273 214m00s  82m00s             
 2485/01/01 09:30 L,T    142   2.385  1.336 -0.280 212m00s  82m00s             
 2503/01/13 18:04 L,T    142   2.378  1.331 -0.283 212m00s  80m00s             
 2521/01/24 02:37 L,T    142   2.369  1.326 -0.287 212m00s  80m00s             
 2539/02/04 11:10 L,T    142   2.358  1.319 -0.291 210m00s  80m00s             
 2557/02/14 19:39 L,T    142   2.340  1.305 -0.300 210m00s  78m00s             
 2575/02/26 04:06 L,T    142   2.317  1.287 -0.311 208m00s  76m00s             
 2593/03/08 12:27 L,T    142   2.284  1.259 -0.328 208m00s  72m00s             

Displayed matches 1 - 50 of 72

Note that the database does not contain the whole of lunar Saros series 142, 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 $)