Solar eclipse of March 17, 1904 Contents Related eclipses Notes References Navigation menu5°36′N 94°42′E / 5.6°N 94.7°E / 5.6; 94.79290"Solar- and Lunar-Eclipse Predictions from Antiquity to the Present"Earth visibility chart and eclipse statisticsGoogle interactive mapBesselian elementsRussia expedition for solar eclipse of March 17, 1904eexpanding ite

Annular solar eclipses1904 in science20th-century solar eclipsesMarch 1904 eventsSolar eclipse stubs


solar eclipseSt. Patrick's Daysolar eclipseMoonEarthSunapparent diameterannulussemester seriesnodestritossynodic monthsanomalistic month






















Solar eclipse of March 17, 1904

SE1904Mar17A.png
Map

Type of eclipse
NatureAnnular
Gamma0.1299
Magnitude0.9367
Maximum eclipse
Duration487 sec (8 m 7 s)
Coordinates5°36′N 94°42′E / 5.6°N 94.7°E / 5.6; 94.7
Max. width of band237 km (147 mi)
Times (UTC)
Greatest eclipse5:40:44
References
Saros
128 (52 of 73)
Catalog # (SE5000)9290

An annular solar eclipse occurred on March 17, 1904, also known as the "1904 St. Patrick's Day eclipse". 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.




Contents





  • 1 Related eclipses

    • 1.1 Solar eclipses 1902-1907


    • 1.2 Tritos series



  • 2 Notes


  • 3 References




Related eclipses



Solar eclipses 1902-1907


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.[1]
























Tritos series


This eclipse is a part of a tritos cycle, repeating at alternating nodes every 135 synodic months (≈ 3986.63 days, or 11 years minus 1 month). Their appearance and longitude are irregular due to a lack of synchronization with the anomalistic month (period of perigee), but groupings of 3 tritos cycles (≈ 33 years minus 3 months) come close (≈ 434.044 anomalistic months), so eclipses are similar in these groupings.
































Notes




  1. ^ van Gent, R.H. "Solar- and Lunar-Eclipse Predictions from Antiquity to the Present". A Catalogue of Eclipse Cycles. Utrecht University. Retrieved 6 October 2018..mw-parser-output cite.citationfont-style:inherit.mw-parser-output .citation qquotes:"""""""'""'".mw-parser-output .citation .cs1-lock-free abackground:url("//upload.wikimedia.org/wikipedia/commons/thumb/6/65/Lock-green.svg/9px-Lock-green.svg.png")no-repeat;background-position:right .1em center.mw-parser-output .citation .cs1-lock-limited a,.mw-parser-output .citation .cs1-lock-registration abackground:url("//upload.wikimedia.org/wikipedia/commons/thumb/d/d6/Lock-gray-alt-2.svg/9px-Lock-gray-alt-2.svg.png")no-repeat;background-position:right .1em center.mw-parser-output .citation .cs1-lock-subscription abackground:url("//upload.wikimedia.org/wikipedia/commons/thumb/a/aa/Lock-red-alt-2.svg/9px-Lock-red-alt-2.svg.png")no-repeat;background-position:right .1em center.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registrationcolor:#555.mw-parser-output .cs1-subscription span,.mw-parser-output .cs1-registration spanborder-bottom:1px dotted;cursor:help.mw-parser-output .cs1-ws-icon abackground:url("//upload.wikimedia.org/wikipedia/commons/thumb/4/4c/Wikisource-logo.svg/12px-Wikisource-logo.svg.png")no-repeat;background-position:right .1em center.mw-parser-output code.cs1-codecolor:inherit;background:inherit;border:inherit;padding:inherit.mw-parser-output .cs1-hidden-errordisplay:none;font-size:100%.mw-parser-output .cs1-visible-errorfont-size:100%.mw-parser-output .cs1-maintdisplay:none;color:#33aa33;margin-left:0.3em.mw-parser-output .cs1-subscription,.mw-parser-output .cs1-registration,.mw-parser-output .cs1-formatfont-size:95%.mw-parser-output .cs1-kern-left,.mw-parser-output .cs1-kern-wl-leftpadding-left:0.2em.mw-parser-output .cs1-kern-right,.mw-parser-output .cs1-kern-wl-rightpadding-right:0.2em




References



  • Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
    • Google interactive map

    • Besselian elements


  • Russia expedition for solar eclipse of March 17, 1904







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