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
| 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
| 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
| 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}}
class="wikitable" align="{{{align|left}}}" style="margin:{{#ifeq:{{{align}}}|left|0 0 0.5em 1em|0 1em 0.5em 0}}"
|+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 |
class="wikitable" align="{{{align|right}}}" style="margin:{{#ifeq:{{{align}}}|right|0 0 0.5em 1em|0 1em 0.5em 0}}"
|+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 | ||
200px | 200px | 200px |
align=center
| Penumbral lunar eclipse | Annular solar eclipse Solar Saros 128 | Penumbral lunar eclipse Lunar Saros 140 |
Related eclipses
= Eclipses in 1904 =
- A penumbral lunar eclipse on March 2.
- An annular solar eclipse on March 17.
- A penumbral lunar eclipse on March 31.
- A total solar eclipse on September 9.
- A penumbral lunar eclipse on September 24.
= Metonic =
- Preceded by: Solar eclipse of May 28, 1900
- Followed by: Solar eclipse of January 3, 1908
= Tzolkinex =
- Preceded by: Solar eclipse of February 1, 1897
- Followed by: Solar eclipse of April 28, 1911
= Half-Saros =
- Preceded by: Lunar eclipse of March 11, 1895
- Followed by: Lunar eclipse of March 22, 1913
= Tritos =
- Preceded by: Solar eclipse of April 16, 1893
- Followed by: Solar eclipse of February 14, 1915
= Solar Saros 128 =
- Preceded by: Solar eclipse of March 5, 1886
- Followed by: Solar eclipse of March 28, 1922
= Inex =
- Preceded by: Solar eclipse of April 6, 1875
- Followed by: Solar eclipse of February 24, 1933
= Triad =
- Preceded by: Solar eclipse of May 16, 1817
- Followed by: Solar eclipse of January 15, 1991
= 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}}