Solar Eclipse Of March 17, 1904
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An annular
solar eclipse A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season i ...
occurred at the Moon's
descending node An orbital node is either of the two points where an orbit intersects a plane of reference to which it is inclined. A non-inclined orbit, which is contained in the reference plane, has no nodes. Planes of reference Common planes of referenc ...
of orbit on Thursday, March 17, 1904, with a
magnitude Magnitude may refer to: Mathematics *Euclidean vector, a quantity defined by both its magnitude and its direction *Magnitude (mathematics), the relative size of an object *Norm (mathematics), a term for the size or length of a vector *Order of ...
of 0.9367. A
solar eclipse A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby obscuring the view of the Sun from a small part of Earth, totally or partially. Such an alignment occurs approximately every six months, during the eclipse season i ...
occurs when the
Moon The Moon is Earth's only natural satellite. It Orbit of the Moon, orbits around Earth at Lunar distance, an average distance of (; about 30 times Earth diameter, Earth's diameter). The Moon rotation, rotates, with a rotation period (lunar ...
passes between
Earth Earth is the third planet from the Sun and the only astronomical object known to Planetary habitability, harbor life. This is enabled by Earth being an ocean world, the only one in the Solar System sustaining liquid surface water. Almost all ...
and the
Sun The Sun is the star at the centre of the Solar System. It is a massive, nearly perfect sphere of hot plasma, heated to incandescence by nuclear fusion reactions in its core, radiating the energy from its surface mainly as visible light a ...
, 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 The angular diameter, angular size, apparent diameter, or apparent size is an angular separation (in units of angle) describing how large a sphere or circle appears from a given point of view. In the vision sciences, it is called the '' visual ...
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 An apsis (; ) is the farthest or nearest point in the orbit of a planetary body about its primary body. The line of apsides (also called apse line, or major axis of the orbit) is the line connecting the two extreme values. Apsides perta ...
(on March 14, 1904, at 6:00 UTC), the Moon's apparent diameter was smaller. The path of annularity covered southern
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(now southern
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), northeastern tip of
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(now
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), northern
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Island in French Comoros (now
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), southern British Seychelles (now
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which is located far away from the main island of
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), most of the
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(excluding the southern part of
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), northwestern
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in the
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), southern Siam (now renamed as
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),
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(the part now belonging to
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, the southern tip of
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and southern
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, including the major city
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, now capital of Cambodia), all of the
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, the northern tip of the American Philippines (now
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) and
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ese islands of
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, South Iwo Jima and
Minamitorishima sometimes Minami-Tori-shima or Minami-Torishima, also known as Marcus Island, is an isolated Islands of Japan, Japanese coral atoll in the northwestern Pacific Ocean, located some southeast of Tokyo and east of the closest Japanese island, Sout ...
. In addition, a partial solar eclipse was seen within a much larger area, including the eastern half of
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,
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except the northernmost tip of
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), most of
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except the northwest border,
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, Japan,
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, the extreme northern coast of
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, northwestern
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.


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 Ho Chi Minh City (HCMC) ('','' TP.HCM; ), commonly known as Saigon (; ), is the most populous city in Vietnam with a population of around 14 million in 2025. The city's geography is defined by rivers and canals, of which the largest is Saigo ...
, 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 A spectrometer () is a scientific instrument used to separate and measure Spectrum, spectral components of a physical phenomenon. Spectrometer is a broad term often used to describe instruments that measure a continuous variable of a phenomeno ...
and recorded changes in the temperature in about 2.5 hours, which dropped for about 3 °C.


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.


Eclipse season

This eclipse is part of an
eclipse season An eclipse season is a period, roughly every six months, when eclipses occur. Eclipse seasons are the result of the axial parallelism of the Orbit of the Moon, Moon's orbital plane (orbital inclination, tilted five degrees to the ecliptic, Earth ...
, 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 A fortnight is a unit of time equal to 14 days (two weeks). The word derives from the Old English term , meaning "" (or "fourteen days", since the Anglo-Saxons counted by nights). Astronomy and tides In astronomy, a ''lunar fortnight'' is hal ...
. The first and last eclipse in this sequence is separated by one
synodic month In lunar calendars, a lunar month is the time between two successive Syzygy (astronomy), syzygies of the same type: new moons or full moons. The precise definition varies, especially for the beginning of the month. Variations In Shona people, S ...
.


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 A total solar eclipse occurred at the Moon's Lunar node, descending node of orbit between Friday, January 3 and Saturday, January 4, 1908, with a Magnitude of eclipse, magnitude of 1.0437. A solar eclipse occurs when the Moon passes between Earth ...


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 An annular solar eclipse occurred at the Moon's descending node of orbit on Tuesday, March 28, 1922, with a magnitude of 0.9381. A solar eclipse occurs when the Moon passes between Earth and the Sun, thereby totally or partly obscuring the image o ...


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


Saros 128


Metonic series


Tritos series


Inex series


Notes


References


Russia expedition for solar eclipse of March 17, 1904
{{Solar eclipses 1904 3 17 1904 in science 1904 03 17 March 1904