In 2052, there are 2 solar eclipses and 2 lunar eclipses:

Eclipses During 2052
2052 Mar 30: Total Solar Eclipse
2052 Apr 14: Penumbral Lunar Eclipse
2052 Sep 22: Annular Solar Eclipse
2052 Oct 08: Partial Lunar Eclipse

Eclipses During 2052
Total Solar Eclipse 2052 Mar 30	Penumbral Lunar Eclipse 2052 Apr 14	Annular Solar Eclipse 2052 Sep 22	Partial Lunar Eclipse 2052 Oct 08

World maps show the regions of visibility for each eclipse. The lunar eclipse diagrams also include the path of the Moon through Earth’s shadow. Contact times for each principal phase are tabulated along with the magnitudes and geocentric coordinates of the Sun and the Moon at greatest eclipse.

Unless otherwise stated, all times and dates used in this publication are in Universal Time or UT1 [1]. This astronomically derived time system is colloquially referred to as Greenwich Mean Time or GMT. To learn more about UT1 and how to convert UT1 to your own local time, see Time Zones and Universal Time.

Click for larger more detailed figure

Total Solar Eclipse of 2052 Mar 30

Under Construction

Map of the eclipse (Figure 1).

Local circumstances for a number of cities are given in Table 1.

The 2052 Mar 30 Solar Eclipse Circumstances Calculator is an interactive web page that can quickly calculate the local circumstances for the eclipse from any geographic location not included in the table.

The path of the eclipse is plotted on an interactive map at Google Map of the 2052 Mar 30 Solar Eclipse . This map permits zooming and scrolling as desired. Clicking the cursor on any location calculates the eclipse circumstances for that location. For more information see Key to Google Eclipse Maps.

This is the xx th eclipse of Saros [6] series 130.

Complete details for the xx eclipses in the series may be found at Saros 130.

For more information about this eclipse, see the EclipseWise Prime Page at Total Solar Eclipse of 2052 Mar 30.

Click for larger more detailed figure

Penumbral Lunar Eclipse of 2052 Apr 14

Under Construction

Diagram and map of the eclipse (Figure 2).

Table 2 lists predicted umbral immersion and emersion times for 25 well-defined lunar craters. The timing of craters is useful in determining the atmospheric enlargement of Earth's shadow (see Crater Timings During Lunar Eclipses).

This is the xx th eclipse of Saros [6] series 142

Complete details for the xx eclipses in the series may be found at Saros 142.

For more information about this eclipse, see the EclipseWise Prime Page at Penumbral Lunar Eclipse of 2052 Apr 14

Click for larger more detailed figure

Annular Solar Eclipse of 2052 Sep 22

Under Construction

Map of the eclipse (Figure 3).

Local circumstances for a number of cities are given in Table 3.

The 2052 Sep 22 Solar Eclipse Circumstances Calculator is an interactive web page that can quickly calculate the local circumstances for the eclipse from any geographic location not included in the table.

The path of the eclipse is plotted on an interactive map at Google Map of the 2052 Sep 22 Solar Eclipse . This map permits zooming and scrolling as desired. Clicking the cursor on any location calculates the eclipse circumstances for that location. For more information see Key to Google Eclipse Maps.

This is the xx th eclipse of Saros [6] series 135.

Complete details for the xx eclipses in the series may be found at Saros 135.

For more information about this eclipse, see the EclipseWise Prime Page at Annular Solar Eclipse of 2052 Sep 22.

Click for larger more detailed figure

Partial Lunar Eclipse of 2052 Oct 08

Under Construction

Diagram and map of the eclipse (Figure 4).

Table 4 lists predicted umbral immersion and emersion times for 25 well-defined lunar craters. The timing of craters is useful in determining the atmospheric enlargement of Earth's shadow (see Crater Timings During Lunar Eclipses).

This is the xx th eclipse of Saros [6] series 147

Complete details for the xx eclipses in the series may be found at Saros 147.

For more information about this eclipse, see the EclipseWise Prime Page at Partial Lunar Eclipse of 2052 Oct 08

Explanatory Information

Solar Eclipse Figures

Lunar Eclipse Figures

Enlargement of Earth's Shadows and Lunar Eclipses

Danjon Scale of Lunar Eclipse Brightness

Moon's Apparent Magnitude During Total Lunar Eclipses

Crater Timings During Lunar Eclipses

Eclipse Altitudes and Azimuths

The altitude a and azimuth A of the Sun or Moon during an eclipse depend on the time and the observer's geographic coordinates. They are calculated as follows:

         h = 15 (GST + UT - α ) + λ
         a = arcsin [sin δ sin φ + cos δ cos h cos φ]
         A = arctan [-(cos δ sin h)/(sin δ cos φ - cos δ cos h sin φ)]

where

         h = hour angle of Sun or Moon
         a = altitude
         A = azimuth
         GST = Greenwich Sidereal Time at 0:00 UT
         UT = Universal Time
         α = right ascension of Sun or Moon
         δ = declination of Sun or Moon
         λ = observer's longitude (east +, west -)
         φ = observer's latitude (north +, south -)

During the eclipses of 2052 , the values for GST and the geocentric Right Ascension and Declination of the Sun or the Moon (at greatest eclipse) are as follows:

                  Eclipse               Date             GST          α            δ

                  Total Solar        2052 Mar 30   12.590    0.659    4.257
                  Penumbral Lunar        2052 Apr 14   13.531   13.553   -8.693
                  Annular Solar        2052 Sep 22    0.169   12.041   -0.265
                  Partial Lunar        2052 Oct 08    1.185    0.993    5.314

Two web based tools that can also be used to calculate the local circumstances for all solar and lunar eclipses visible from any location. They are the Javascript Solar Eclipse Explorer and the Javascript Lunar Eclipse Explorer. The URLs for these tools are:

Javascript Solar Eclipse Explorer: www.EclipseWise.com/solar/JSEX/JSEX-index.html

Javascript Lunar Eclipse Explorer: www.EclipseWise.com/lunar/JLEX/JLEX-index.html

Eclipses During 2053

In 2053, there are 2 solar eclipses and 2 lunar eclipses:

Eclipses During 2053
2053 Mar 04: Penumbral Lunar Eclipse
2053 Mar 20: Annular Solar Eclipse
2053 Aug 29: Penumbral Lunar Eclipse
2053 Sep 12: Total Solar Eclipse

Eclipses During 2053
Penumbral Lunar Eclipse 2053 Mar 04	Annular Solar Eclipse 2053 Mar 20	Penumbral Lunar Eclipse 2053 Aug 29	Total Solar Eclipse 2053 Sep 12

A full report Eclipses During 2053 will be published in Observer's Handbook:2053

Eclipse Web Sites

EclipseWise.com is a website dedicated to predictions and information on eclipses of the Sun and Moon. It offers a graphically intuitive interface and contains maps, diagrams, tables, and information about every solar and lunar eclipse from 2000 BCE to 3000 CE. This period includes 11898 solar eclipses and 12064 lunar eclipses.

Much of EclipseWise.com is based on the Thousand Year Canon of Solar Eclipses 1501 to 2500 (Espenak 2014a) and the Thousand Year Canon of Lunar Eclipses 1501 to 2500 (Espenak 2014b). These eclipse predictions use the Jet Propulsion Lab's DE406 — a computer ephemeris used for calculating high precision coordinates of the Sun and Moon for thousands of years into the past and future.

For eclipses over a larger time interval see Five Millennium Canon of Solar Eclipses –1999 to +3000 and Five Millennium Canon of Lunar Eclipses –-1999 to +3000.

The World Atlas of Solar Eclipses provides maps of all central eclipse paths from 2000 BCE to 3000 CE.

MrEclipse.com targets solar and lunar eclipse photography, with tips on eclipse observing and eye safety.

Eclipse Publications

Acknowledgments

All eclipse predictions were generated on a Macintosh G4 PowerPC using algorithms developed from the Explanatory Supplement [1974] with additional algorithms from Meeus, Grosjean, and Vanderleen [1966]. The solar and lunar coordinates used in the eclipse predictions are based on the JPL DE405. For lunar eclipses, the elliptical shape of the umbral and penumbral shadows were calculated using Herald and Sinnott (2014) method of enlarging Earth's radius to compensate for the opacity of the terrestrial atmosphere (including corrections for the oblateness of Earth).

All calculations, diagrams, tables, and opinions presented in this paper are those of the author, and he assumes full responsibility for their accuracy.

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

"Eclipse Predictions by Fred Espenak, EclipseWise.com"

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

Footnotes

[1] UT1 or Universal Time is the mean solar time on the Prime Meridian at Greenwich, England. Civil time signals are transmitted according to Coordinated Universal Time (UTC), which is based on International Atomic Time (TAI) with leap seconds added at irregular intervals to compensate for the slowing of Earth's rotation. The leap seconds keep UTC within 0.9 second of UT1.

[2] The instant of greatest eclipse for solar eclipses occurs when the distance between the Moon's shadow axis and Earth's geocenter reaches a minimum.

[3] Eclipse magnitude for solar eclipses is defined as the fraction of the Sun's diameter occulted by the Moon.

[4] Eclipse obscuration is defined as the fraction of the Sun's area occulted by the Moon.

[5] For solar eclipses, gamma is the distance of the Moon's shadow axis from Earth's center (in Earth radii) when it reaches its minimum absolute value.

[6] The Saros is a period of 6,585.3 days (18 years 11 days 8 hours) in which eclipses (both solar and lunar) repeat. The geometry isn't exact but close enough for a Saros series to last 12 or more centuries.

[7] The instant of greatest eclipse for lunar eclipses occurs when the distance between the Moon and Earth's shadow axis reaches a minimum.

[8] Umbral eclipse magnitude is defined as the fraction of the Moon's diameter occulted by Earth's umbral shadow.

[9] For lunar eclipses, gamma is the distance of the Moon's center from Earth's shadow axis (in Earth radii) when it reaches its minimum absolute value.

[10] Penumbral eclipse magnitude is defined as the fraction of the Moon's diameter occulted by Earth's penumbral shadow.

References

Chauvenet, W., Manual of Spherical and Practical Astronomy, Vol.1, 1891 (Dover edition 1961).

Danjon, A., "Les éclipses de Lune par la pénombre en 1951," L'Astronomie, 65, 51-53 (Feb. 1951).

Espenak, F., Meeus, J., Five Millennium Canon of Solar Eclipses –1999 to +3000, 2nd Edition, AstroPixels Publishing, Portal, AZ, 2021.

Espenak, F., Meeus, J., Five Millennium Canon of Lunar Eclipses –-1999 to +3000, 2nd Edition, AstroPixels Publishing, Portal, AZ, 2021.

Espenak, F., Thousand Year Canon of Solar Eclipses 1501 to 2500, AstroPixels Publishing, Portal, AZ, 2014.

Espenak, F., Thousand Year Canon of Lunar Eclipses 1501 to 2500, AstroPixels Publishing, Portal, AZ, 2014.

Espenak, F., 21st Century Canon of Solar Eclipses, AstroPixels Publishing, Portal, AZ, 2016.

Espenak, F., 21st Century Canon of Lunar Eclipses, AstroPixels Publishing, Portal, AZ, 2020.

Espenak, F., Atlas of Central Solar Eclipses in the USA, AstroPixels Publishing, Portal, AZ, 2016.

Explanatory Supplement to the Astronomical Ephemeris and the American Ephemeris and Nautical Almanac, Her Majesty's Nautical Almanac Office, London, 1974.

Herald, D., and Sinnott, R. W., “Analysis of Lunar Crater Timings, 1842–2011,” J. Br. Astron. Assoc., 124, 5, 2014.

Keen, R. A., "Volcanic Aerosols and Lunar Eclipses", Science, vol. 222, p. 1011-1013, Dec. 2, 1983.

Meeus, J., Elements of Solar Eclipses 1951-2200, Willmann-Bell, Richmond, VA (1989).

Eclipse Publications