An annular solar eclipse will occur on October 14, 2088. 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.
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]
It is a part of Saros cycle 135, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on July 5, 1331. It contains annular eclipses from October 21, 1511 through February 24, 2305, hybrid eclipses on March 8, 2323 and March 18, 2341 and total eclipses from March 29, 2359 through May 22, 2449. The series ends at member 71 as a partial eclipse on August 17, 2593. The longest duration of totality will be 2 minutes, 27 seconds on May 12, 2431.
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.
^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.
External linksedit
Earth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak, NASA/GSFC
Google interactive map
Besselian elements
This solar eclipse–related article is a stub. You can help Wikipedia by expanding it.
solar, eclipse, october, 2088, annular, solar, eclipse, will, occur, october, 2088, solar, eclipse, occurs, when, moon, passes, between, earth, thereby, totally, partly, obscuring, image, viewer, earth, annular, solar, eclipse, occurs, when, moon, apparent, di. An annular solar eclipse will occur on October 14 2088 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 Solar eclipse of October 14 2088MapType of eclipseNatureAnnularGamma 0 5349Magnitude0 9727Maximum eclipseDuration158 sec 2 m 38 s Coordinates39 42 S 56 00 W 39 7 S 56 W 39 7 56Max width of band115 km 71 mi Times UTC Greatest eclipse14 48 05ReferencesSaros135 43 of 71 Catalog SE5000 9707 Contents 1 Related eclipses 1 1 Solar eclipses 2087 2090 1 2 Saros 135 1 3 Tritos series 2 References 3 External linksRelated eclipses editSolar eclipses 2087 2090 edit 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 1 120 May 2 2087 nbsp Partial 125 October 26 2087 nbsp Partial130 April 21 2088 nbsp Total 135 October 14 2088 nbsp Annular140 April 10 2089 nbsp Annular 145 October 4 2089 nbsp Total150 March 31 2090 nbsp Partial 155 September 23 2090 nbsp TotalSaros 135 edit It is a part of Saros cycle 135 repeating every 18 years 11 days containing 71 events The series started with partial solar eclipse on July 5 1331 It contains annular eclipses from October 21 1511 through February 24 2305 hybrid eclipses on March 8 2323 and March 18 2341 and total eclipses from March 29 2359 through May 22 2449 The series ends at member 71 as a partial eclipse on August 17 2593 The longest duration of totality will be 2 minutes 27 seconds on May 12 2431 Series members 27 43 occur between 1800 and 2100 27 28 29 nbsp Apr 24 1800 nbsp May 5 1818 nbsp May 15 183630 31 32 nbsp May 26 1854 nbsp Jun 6 1872 nbsp Jun 17 189033 34 35 nbsp Jun 28 1908 nbsp Jul 9 1926 nbsp Jul 20 194436 37 38 nbsp Jul 31 1962 nbsp Aug 10 1980 nbsp Aug 22 199839 40 41 nbsp Sep 1 2016 nbsp Sep 12 2034 nbsp Sep 22 205242 43 nbsp Oct 4 2070 nbsp Oct 14 2088Tritos series edit 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 Series members between 1901 and 2100 nbsp March 29 1903 Saros 118 nbsp February 25 1914 Saros 119 nbsp January 24 1925 Saros 120 nbsp December 25 1935 Saros 121 nbsp November 23 1946 Saros 122 nbsp October 23 1957 Saros 123 nbsp September 22 1968 Saros 124 nbsp August 22 1979 Saros 125 nbsp July 22 1990 Saros 126 nbsp June 21 2001 Saros 127 nbsp May 20 2012 Saros 128 nbsp April 20 2023 Saros 129 nbsp March 20 2034 Saros 130 nbsp February 16 2045 Saros 131 nbsp January 16 2056 Saros 132 nbsp December 17 2066 Saros 133 nbsp November 15 2077 Saros 134 nbsp October 14 2088 Saros 135 nbsp September 14 2099 Saros 136 References edit 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 External links editEarth visibility chart and eclipse statistics Eclipse Predictions by Fred Espenak NASA GSFC Google interactive map Besselian elements nbsp This solar eclipse related article is a stub You can help Wikipedia by expanding it vte Retrieved from https en wikipedia org w index php title Solar eclipse of October 14 2088 amp oldid 1047606955, wikipedia, wiki, book, books, library,
