Solar Eclipse Prime Page

Annular Solar Eclipse of 1935 Dec 25

Fred Espenak

Key to Solar Eclipse Figure (below)

Introduction


The Annular Solar Eclipse of 1935 Dec 25 is visible from the following geographic regions:

  • Partial Eclipse: Antarctica, south South America
  • Annular Eclipse: Antarctica

The map to the right depicts the geographic regions of eclipse visibility. Click on the map to enlarge it. For an explanation of the features appearing in the map, see Key to Solar Eclipse Maps.

The instant of greatest eclipse takes place on 1935 Dec 25 at 17:59:52 TD (17:59:28 UT1). This is 4.9 days before the Moon reaches perigee. During the eclipse, the Sun is in the constellation Sagittarius. The synodic month in which the eclipse takes place has a Brown Lunation Number of 161.

The eclipse belongs to Saros 121 and is number 56 of 71 eclipses in the series. All eclipses in this series occur at the Moon’s ascending node. The Moon moves southward with respect to the node with each succeeding eclipse in the series and gamma decreases.

The annular solar eclipse of 1935 Dec 25 is followed two weeks later by a total lunar eclipse on 1936 Jan 08.

These eclipses all take place during a single eclipse season.

The eclipse predictions are given in both Terrestrial Dynamical Time (TD) and Universal Time (UT1). The parameter ΔT is used to convert between these two times (i.e., UT1 = TD - ΔT). ΔT has a value of 23.7 seconds for this eclipse.

The following links provide maps and data for the eclipse.

Eclipse Data: Annular Solar Eclipse of 1935 Dec 25

Eclipse Characteristics
Parameter Value
Eclipse Magnitude 0.97525
Eclipse Obscuration 0.95112
Gamma-0.92279
Conjunction Times
Event Calendar Date and Time Julian Date
Greatest Eclipse 1935 Dec 25 at 17:59:51.8 TD (17:59:28.1 UT1) 2428162.249631
Ecliptic Conjunction 1935 Dec 25 at 17:49:48.0 TD (17:49:24.2 UT1) 2428162.242642
Equatorial Conjunction 1935 Dec 25 at 17:47:27.1 TD (17:47:03.4 UT1) 2428162.241011
Geocentric Coordinates of Sun and Moon
1935 Dec 25 at 17:59:51.8 TD (17:59:28.1 UT1)
Coordinate Sun Moon
Right Ascension18h13m12.8s18h13m41.2s
Declination-23°24'47.6"-24°17'40.0"
Semi-Diameter 16'15.8" 15'46.2"
Eq. Hor. Parallax 08.9" 0°57'52.6"
Geocentric Libration of Moon
Angle Value
l -4.8°
b 1.2°
c 0.1°
Prediction Parameters
Paramater Value
Ephemerides JPL DE405
ΔT 23.7 s
k (penumbra) 0.2725076
k (umbra) 0.2722810
Saros Series 121 (56/71)

Explanation of Solar Eclipse Data Tables

Penumbral Shadow Contacts and Extremes: Annular Solar Eclipse of 1935 Dec 25

Contacts of Penumbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactP115:42:21.215:41:57.439°11.5'S166°11.2'W
Last External ContactP420:17:22.020:16:58.226°54.2'S021°33.6'W
Extreme Northern and Southern Path Limits of Penumbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N116:07:54.816:07:31.126°32.0'S164°23.3'W
South Extreme Path Limit 1S119:51:48.819:51:25.113°51.9'S021°43.7'W

Explanation of Penumbral Shadow Contacts and Extremes Tables

Umbral Shadow Contacts and Extremes: Annular Solar Eclipse of 1935 Dec 25

Contacts of Umbral Shadow with Earth
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
First External ContactU117:15:44.817:15:21.061°39.5'S137°45.1'E
First Internal ContactU217:20:52.117:20:28.362°56.1'S131°55.9'E
Last Internal ContactU318:39:02.718:38:39.054°08.8'S027°07.9'E
Last External ContactU418:44:04.018:43:40.352°20.2'S023°11.4'E
Extreme Northern and Southern Path Limits of Umbra
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
North Extreme Path Limit 1N117:15:53.317:15:29.661°36.2'S137°53.7'E
South Extreme Path Limit 1S117:20:44.417:20:20.762°58.8'S131°47.3'E
North Extreme Path Limit 2N218:43:55.718:43:32.052°15.6'S023°07.0'E
South Extreme Path Limit 2S218:39:10.218:38:46.554°12.8'S027°12.3'E

Explanation of Umbral Shadow Contacts and Extremes Tables

Central Line Extremes and Duration: Annular Solar Eclipse of 1935 Dec 25

Extreme Limits of the Central Line
Contact Event Contact Time
TD
Time
UT1
Latitude Longitude
Extreme Central Line Limit 1C117:18:14.417:17:50.762°17.6'S134°59.1'E
Extreme Central Line Limit 2C218:41:37.418:41:13.653°13.1'S025°04.1'E

Explanation of Central Line Extremes Table

Greatest Eclipse and Greatest Duration
Event Time
TD
Time
UT1
Latitude Longitude Sun
Altitude
Sun
Azimuth
Path Width Central
Duration
Greatest Eclipse17:59:51.817:59:28.183°30.0'S009°23.6'E 22.2° 258.0° 234.4 km01m30.35s
Greatest Duration17:18:14.417:17:50.762°17.6'S134°59.1'E 0.0° 148.7° 349.7 km01m38.45s

Explanation of Greatest Eclipse and Greatest Duration

Polynomial Besselian Elements: Annular Solar Eclipse of 1935 Dec 25

Polynomial Besselian Elements
1935 Dec 25 at 18:00:00.0 TD (=t0)
n x y d l1 l2 μ
0 0.11332 -0.91581 -23.4109 0.55491 0.00871 90.0158
1 0.54185 0.06631 0.0008 -0.00012 -0.00012 14.9963
2 -0.00001 0.00021 0.0000 -0.00001 -0.00001 0.0000
3 -0.00001 -0.00000 - - - -
Tan ƒ1 0.0047548
Tan ƒ2 0.0047311

At time t1 (decimal hours), each besselian element is evaluated by:

x = x0 + x1*t + x2*t2 + x3*t3 (or x = Σ [xn*tn]; n = 0 to 3)

where: t = t1 - t0 (decimal hours) and t0 = 18.000

Explanation of Polynomial Besselian Elements

Eclipse Publications

jpeg jpeg
jpeg jpeg
jpeg

For more visit: AstroPixels Publishing

Links for the Annular Solar Eclipse of 1935 Dec 25

Links to Additional Solar Eclipse Information

  • Home - home page of EclipseWise with predictions for both solar and lunar eclipses

Decade Tables of Solar Eclipses:
| 1901 - 1910 | 1911 - 1919 | 1921 - 1930 | 1931 - 1940 | 1941 - 1950 |
| 1951 - 1960 | 1961 - 1970 | 1971 - 1980 | 1981 - 1990 | 1991 - 2000 |
| 2001 - 2010 | 2011 - 2020 | 2021 - 2030 | 2031 - 2040 | 2041 - 2050 |
| 2051 - 2060 | 2061 - 2070 | 2071 - 2080 | 2081 - 2090 | 2091 - 2100 |

Solar Eclipse Publications

Eclipse Publications

jpeg jpeg
jpeg jpeg
jpeg jpeg

For more visit: AstroPixels Publishing

Eclipse Predictions

Predictions for the Annular Solar Eclipse of 1935 Dec 25 were generated using the JPL DE405 solar and lunar ephemerides. The lunar coordinates were calculated with respect to the Moon's Center of Mass. The predictions are given in both Terrestrial Dynamical Time (TD) and Universal Time (UT1). The parameter ΔT is used to convert between these two times (i.e., UT1 = TD - ΔT). ΔT has a value of 23.7 seconds for this eclipse.

Acknowledgments

Some of the content on this website is based on the books 21st Century Canon of Solar Eclipses and Thousand Year Canon of Solar Eclipses 1501 to 2500. All eclipse calculations are by Fred Espenak, and he assumes full responsibility for their accuracy.

Permission is granted to reproduce eclipse data when accompanied by a link to this page and an acknowledgment:

"Eclipse Predictions by Fred Espenak, www.EclipseWise.com"

The use of diagrams and maps is permitted provided that they are NOT altered (except for re-sizing) and the embedded credit line is NOT removed or concealed.