solar eclipse of March 29, 2025
{{short description|Partial solar eclipse}}
{{Use mdy dates|date=March 2025}}
{{Infobox solar eclipse|2025Mar29
| previous = Solar eclipse of October 2, 2024
| next = Solar eclipse of September 21, 2025
}}
A partial solar eclipse occurred at the Moon’s ascending node (new moon) of orbit on Saturday, March 29, 2025,{{cite web|title=March 29, 2025 Partial Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/2025-march-29|publisher=timeanddate|access-date=August 13, 2024}} with a magnitude of 0.9376. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image of the Sun for a viewer on Earth. A partial solar eclipse occurred in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.
The partial eclipse was visible for parts of the northeastern United States, eastern Canada, Greenland, Europe, Northwest Africa, and northwestern Russia.
Eclipse details
Shown below are two tables displaying details about this particular solar eclipse. The first table outlines times at which the moon's penumbra or umbra attains the specific parameter, and the second table describes various other parameters pertaining to this eclipse.{{cite web|title=Partial Solar Eclipse of 2025 Mar 29|url=https://eclipsewise.com/solar/SEprime/2001-2100/SE2025Mar29Pprime.html|publisher=EclipseWise.com|access-date=August 13, 2024}}
valign=top|
{| class="wikitable" |+Times ! Event ! Time |
First penumbral external contact
| 08:51:52.5 UTC |
Greatest eclipse |
Ecliptic conjunction
| 10:58:59.4 UTC |
Equatorial conjunction
| 11:47:27.0 UTC |
Last penumbral external contact
| 12:44:54.0 UTC |
File:Map of the March 29, 2025 Partial Solar Eclipse (SVS5510).tiff|access-date=March 28, 2025|url-status=|archive-url=|archive-date=}}]]
|width=20|
|valign=top|
class="wikitable"
|+Parameters ! Parameter ! Value |
Eclipse magnitude
| 0.93760 |
Eclipse obscuration
| 0.93057 |
Gamma |
Sun right ascension
| 00h 33m 03.1s |
Sun declination
| +03° 33' 55.0" |
Sun semi-diameter
| 16' 01.1" |
Sun equatorial horizontal parallax
| 08.8" |
Moon right ascension
| 00h 31m 00.8s |
Moon declination
| +04° 29' 34.1" |
Moon semi-diameter
| 16'39.4" |
Moon equatorial horizontal parallax
| 1° 01' 07.8" |
ΔT (which is TD – UT {{cite web|url=https://eclipse.gsfc.nasa.gov/LEcat5/deltat.html|website=eclipse.gsfc.nasa.gov|title=Delta T (ΔT)|author=Michael S. Kirk|publisher=Heliophysics Science Division, Code 670 NASA Goddard Space Flight Center Greenbelt, MD 20771, USA|access-date=March 28, 2025|date=January 29, 2009|archive-url=|archive-date=}}) |
|}
{{clear}}
Images
File:Partial solar eclipse of 29 March 2025 in Tuntorp, Brastad.webm|Through clouds at 10:55 to 12:01 UTC in Brastad, Sweden
File:Sonnenfinsternis 2025-03-29.tif|alt=A photo of the 2025-03-29 partial solar eclipse, showing one larger and several smaller sunspots|In Hilden, Germany 11:18 UTC
File:Devils Horns.jpg|Devil’s Horns Phenomenon Halifax, Nova Scotia, Canada 10:20 UTC
File:29.03.2025 Solar Eclipse Maximum West Midlands England.jpg|At maximum (11:05 UTC), West Midlands, England
File:Solar eclipse of 2025 March 29 Poland.jpg|Roughly at maximum, Lutkówka, Poland
File:Solar eclipse 2025-03-29 Prague.jpg|At 12:50 p.m. in Prague, Czech Republic
File:Solar eclipse 2025, Klin, Moscow Oblast, Russia, 14.49MSK.jpg|From Klin, Russia, 11:49 UTC
File:A partial solar eclipse projected on a telescope at boating pool.jpg|Projected on a telescope from Ramsgate, Kent
File:2025, 29th March partial solar eclipse. Projected in Torquay, Devon. 05.jpg|Projected on a telescope from Torquay, Devon
Solar eclipses of 2022–2025
This eclipse is a member of a semester series. An eclipse in a semester series of solar eclipses repeats approximately every 177 days and 4 hours (a semester) at alternating nodes of the Moon's orbit.
van Gent, R.H. [https://webspace.science.uu.nl/~gent0113/eclipse/eclipsecycles.htm#Sar%20%28Half%20Saros%29 "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present".] A Catalogue of Eclipse Cycles. Utrecht University. Retrieved October 6, 2018.
{{Solar eclipse set 2022–2025}}
= Eclipse season =
{{See also|Eclipse cycle}}
This eclipse is part of an eclipse season, a period, roughly every six months, when eclipses occur. Only two (or occasionally three) eclipse seasons occur each year, and each season lasts about 35 days and repeats just short of six months (173 days) later; thus two full eclipse seasons always occur each year. Either two or three eclipses happen each eclipse season. In the sequence below, each eclipse is separated by a fortnight.
class="wikitable"
|+ Other eclipse of March 2025 season ! March 14 |
200px |
align=center |
= Other eclipses in 2025 =
- Total: September 7
- Partial: September 21
Related eclipses
{{Main|List of solar eclipses in the 20th century|List of solar eclipses in the 21st century}}
= Tzolkinex =
The tzolkinex is equal to 2598.691 days (about 7 years, 1 month and 12 days).
Before-After
Solar: February 15, 2018 – May 9, 2032
= Tritos series =
= Saros 149 =
This eclipse is a part of Saros series 149, repeating every 18 years, 11 days, 8 hours {{cite book|last1= Aveni|first1=Anthony|author-link1=Anthony Aveni|chapter=5. Babylonian Decryptions|chapter-url=https://books.google.com/books?id=TiSMDgAAQBAJ&dq=eclipse+semester+series&pg=PT70|location=|editor-last1=|editor-first1= |editor-last2=|editor-first2=|title=In the Shadow of the Moon The Science, Magic, and Mystery of Solar Eclipses|url=https://books.google.com/books?id=TiSMDgAAQBAJ|series=|language=|volume=|edition=|publication-place=|publisher=Yale University Press|publication-date=April 25, 2017 |isbn=9780300227574|issn=|url-status=|access-date=|via=}} and containing 71 events. The series started with a partial solar eclipse on August 21, 1664. It contains total eclipses from April 9, 2043 through October 2, 2331; hybrid eclipses from October 13, 2349, through November 3, 2385; and annular eclipses from November 15, 2403, through July 13, 2800. The series ends at member 71 as a partial eclipse on September 28, 2926. Its eclipses are tabulated in three columns; every third eclipse in the same column is one exeligmos apart, so they all cast shadows over approximately the same parts of the Earth.
The longest duration of totality will be produced by member 31 at 4 minutes, 10 seconds on July 17, 2205, and the longest duration of annularity will be produced by member 62 at 5 minutes, 6 seconds on June 21, 2764. All eclipses in this series occur at the Moon’s ascending node of orbit.{{Cite web|url=https://eclipse.gsfc.nasa.gov/SEsaros/SEsaros149.html|title=NASA – Catalog of Solar Eclipses of Saros 149|website=eclipse.gsfc.nasa.gov}}
class="wikitable mw-collapsible mw-collapsed"
!colspan=3|Series members 9–30 occur between 1801 and 2200: |
9
!10 !11 |
---|
style="text-align:center;"
|150px |150px |150px |
12
!13 !14 |
style="text-align:center;"
|150px |150px |150px |
15
!16 !17 |
style="text-align:center;" |
18
!19 !20 |
style="text-align:center;" |
21
!22 !23 |
style="text-align:center;" |
24
!25 !26 |
style="text-align:center;"
|150px |
27
!28 !29 |
style="text-align:center;"
|150px |150px |150px |
30 |
style="text-align:center;"
|150px |
Before-After
Solar: March 19, 2007 – April 9, 2043
Before-After: Half-Saros
Lunar: March 23, 2016 – April 3, 2034
= Metonic series =
= Inex series =
= Triad =
References
{{reflist}}
{{commons category|Solar eclipse of 2025 March 29}}
External links
{{Solar eclipse NASA reference|2001/SE2025Mar29P|20250329}}
{{Solar eclipses}}
{{Portal bar|Stars|Outer space|Physics|Science}}