Solar eclipse of March 17, 1904

{{short description|20th-century annular solar eclipse}}

{{Infobox solar eclipse|1904Mar17

| previous = Solar eclipse of September 21, 1903

| next = Solar eclipse of September 9, 1904

}}

An annular solar eclipse occurred at the Moon's descending node of orbit on Thursday, March 17, 1904,{{cite web|title=March 17, 1904 Total Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/1904-march-17|publisher=timeanddate|access-date=30 July 2024}}{{Cite news

| url = https://newspapers.com/article/americus-times-recorder-this-eclipse-ski/134153507/

| date = 1904-03-17

| page = 4

| title = THIS ECLIPSE SKIPS AMERICUS

| newspaper = Americus Times-Recorder

| location = Americus, Georgia

| via = Newspapers.com

| access-date = 2023-10-27

}}{{Cite news

| url = https://newspapers.com/article/the-kansas-city-star-an-eclipse-of-the-s/134153518/

| date = 1904-03-17

| page = 3

| title = An eclipse of the sun.

| newspaper = The Kansas City Star

| location = Kansas City, Missouri

| via = Newspapers.com

| access-date = 2023-10-27

}}{{Cite news

| url = https://newspapers.com/article/the-daily-journal-erin-go-braugh/134153548/

| date = 1904-03-17

| page = 4

| title = ERIN GO BRAUGH.

| newspaper = The Daily Journal

| location = Freeport, Illinois

| via = Newspapers.com

| access-date = 2023-10-27

}}{{Cite news

| url = https://newspapers.com/article/the-brunswick-news-sun-to-be-eclipsed-to/134153553/

| date = 1904-03-17

| page = 1

| title = Sun to be eclipsed today.

| newspaper = The Brunswick News

| location = Brunswick, Georgia

| via = Newspapers.com

| access-date = 2023-10-27

}} with a magnitude of 0.9367. 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. An annular solar eclipse occurs when the Moon's apparent diameter is smaller than the Sun's, blocking most of the Sun's light and causing the Sun to look like an annulus (ring). An annular eclipse appears as a partial eclipse over a region of the Earth thousands of kilometres wide. Occurring about 3 days after apogee (on March 14, 1904, at 6:00 UTC), the Moon's apparent diameter was smaller.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1904&n=136|publisher=timeanddate|access-date=30 July 2024}}

The path of annularity covered southern German East Africa (now southern Tanzania), northeastern tip of Portuguese East Africa (now Mozambique), northern Grande Comore Island in French Comoros (now Comoros), southern British Seychelles (now Seychelles), British Mauritius (now Mauritius), most of the British Indian Ocean Territory (excluding the southern part of Diego Garcia), northwestern Sumatra in the Dutch East Indies (now Indonesia), southern Siam (now renamed as Thailand), French Indochina (the part now belonging to Cambodia, the southern tip of Laos and southern Vietnam, including the major city Phnom Penh, now capital of Cambodia), all of the Paracel Islands, the northern tip of the American Philippines (now Philippines) and Japanese islands of Iwo Jima, South Iwo Jima and Minamitorishima.

In addition, a partial solar eclipse was seen within a much larger area, including the eastern half of Africa, southern West Asia, southern Afghanistan, South Asia except the northernmost tip of British Raj (now the northernmost tip of Pakistan), most of China except the northwest border, Korean Peninsula, Japan, Southeast Asia, the extreme northern coast of Australia, northwestern Melanesia, central and western Micronesia, and southeastern Russian Empire.

Observations

N. Donitch of the Royal Russian Academy of Sciences (the predecessor of today's Russian Academy of Sciences) traveled to Phnom Penh (now capital of Cambodia) via Saigon (now Ho Chi Minh City, Vietnam) in French Indochina and made observations there. The weather was clear on the eclipse day, with only some fog in the morning. Donitch used a spectrometer and recorded changes in the temperature in about 2.5 hours, which dropped for about 3°C.{{cite journal|author=Donitch, N.|title=On the observation of the Annular Solar eclipse in Indo-China on 16 march 1904|journal=Izv. Russ.Astron.Ob-va|url=http://adsabs.harvard.edu/abs/1905IzRAO..10..276D|year=1905|number=8/9|pages=276-279|archive-date=29 August 2019|archive-url=https://web.archive.org/web/20190829205403/http://adsabs.harvard.edu/abs/1905IzRAO..10..276D}}

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=Annular Solar Eclipse of 1904 Mar 17|url=https://eclipsewise.com/solar/SEprime/1901-2000/SE1904Mar17Aprime.html|publisher=EclipseWise.com|access-date=30 July 2024}}

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|+March 17, 1904 Solar Eclipse Times

! Event

! Time (UTC)

First Penumbral External Contact

| 1904 March 17 at 02:36:24.1 UTC

First Umbral External Contact

| 1904 March 17 at 03:41:08.2 UTC

First Central Line

| 1904 March 17 at 03:43:53.3 UTC

First Umbral Internal Contact

| 1904 March 17 at 03:46:38.6 UTC

First Penumbral Internal Contact

| 1904 March 17 at 04:52:21.2 UTC

Greatest Duration

| 1904 March 17 at 05:37:38.0 UTC

Ecliptic Conjunction

| 1904 March 17 at 05:39:11.3 UTC

Greatest Eclipse

| 1904 March 17 at 05:40:44.1 UTC

Equatorial Conjunction

| 1904 March 17 at 05:45:36.1 UTC

Last Penumbral Internal Contact

| 1904 March 17 at 06:28:59.4 UTC

Last Umbral Internal Contact

| 1904 March 17 at 07:34:47.3 UTC

Last Central Line

| 1904 March 17 at 07:37:30.8 UTC

Last Umbral External Contact

| 1904 March 17 at 07:40:14.2 UTC

Last Penumbral External Contact

| 1904 March 17 at 08:44:57.8 UTC

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|+March 17, 1904 Solar Eclipse Parameters

! Parameter

! Value

Eclipse Magnitude

| 0.93675

Eclipse Obscuration

| 0.87751

Gamma

| 0.12993

Sun Right Ascension

| 23h46m07.3s

Sun Declination

| -01°30'13.7"

Sun Semi-Diameter

| 16'04.1"

Sun Equatorial Horizontal Parallax

| 08.8"

Moon Right Ascension

| 23h45m58.8s

Moon Declination

| -01°23'30.5"

Moon Semi-Diameter

| 14'49.6"

Moon Equatorial Horizontal Parallax

| 0°54'24.9"

ΔT

| 2.9 s

{{clear}}

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. The first and last eclipse in this sequence is separated by one synodic month.

class="wikitable"

|+ Eclipse season of March 1904

! March 2
Ascending node (full moon) !! March 17
Descending node (new moon) !! March 31
Ascending node (full moon)

200px200px200px
align=center

| Penumbral lunar eclipse
Lunar Saros 102

Annular solar eclipse
Solar Saros 128
Penumbral lunar eclipse
Lunar Saros 140

Related eclipses

= Eclipses in 1904 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Solar Saros 128 =

= Inex =

= Triad =

= Solar eclipses of 1902–1906 =

{{Solar eclipse set 1902–1906}}

= Saros 128 =

{{Solar Saros series 128}}

= Metonic series =

{{Solar Metonic series 1866–1953}}

= Tritos series =

{{Solar Trito series 2002 June 10}}

= Inex series =

{{Solar Inex series 2019 December 26}}

Notes

{{reflist}}

References

{{Solar eclipse NASA reference|1901/SE1904Mar17A|19040317}}

  • [http://www.eclipse-2008.ru/eclipse/1904.php Russia expedition for solar eclipse of March 17, 1904]

{{Solar eclipses}}

1904 3 17

Category:1904 in science

1904 03 17

Category:March 1904