Solar eclipse of March 9, 1997

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Solar eclipse of March 9, 1997
Total eclipse from Chita, Russia
Map
Type of eclipse
NatureTotal
Gamma0.9183
Magnitude1.042
Maximum eclipse
Duration170 s (2 min 50 s)
Coordinates57°48′N 130°42′E / 57.8°N 130.7°E / 57.8; 130.7
Max. width of band356 km (221 mi)
Times (UTC)
Greatest eclipse1:24:51
References
Saros120 (60 of 71)
Catalog # (SE5000)9501

A total solar eclipse occurred on Sunday, March 9, 1997. 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. A total solar eclipse occurs when the Moon's apparent diameter is larger than the Sun's, blocking all direct sunlight, turning day into darkness. Totality occurs in a narrow path across Earth's surface, with the partial solar eclipse visible over a surrounding region thousands of kilometres wide. Totality was visible in eastern Russia, Northern Mongolia, northern tip of Xinjiang and Northeastern China and eastern tip of Kazakhstan.

Unusual gravity variations[edit]

This solar eclipse is somewhat special in the sense that some unexplained gravity anomalies of about 7 10−8 m/s2 during the solar eclipse were observed. Attempts (e.g., Van Flandern–Yang hypothesis) to explain these anomalies have not been able to reach a definite conclusion.[1]

Images[edit]

Related eclipses[edit]

Eclipses of 1997[edit]

Solar eclipses 1997–2000[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.[2]

Solar eclipse series sets from 1997 to 2000
Descending node   Ascending node
Saros Map Gamma Saros Map Gamma
120

Chita, Russia
1997 March 09

Total
0.91830 125 1997 September 02

Partial (south)
−1.03521
130

Total eclipse near Guadeloupe
1998 February 26

Total
0.23909 135 1998 August 22

Annular
−0.26441
140 1999 February 16

Annular
−0.47260 145

Totality from France
1999 August 11

Total
0.50623
150 2000 February 05

Partial (south)
−1.22325 155 2000 July 31

Partial (north)
1.21664

Partial solar eclipses on July 1, 2000 and December 25, 2000 occur in the next lunar year eclipse set.

Saros 120[edit]

This eclipse is a part of Saros cycle 120, repeating every 18 years, 11 days, containing 71 events. The series started with partial solar eclipse on May 27, 933 AD, and reached an annular eclipse on August 11, 1059. It was a hybrid event for 3 dates: May 8, 1510, through May 29, 1546, and total eclipses from June 8, 1564, through March 30, 2033. The series ends at member 71 as a partial eclipse on July 7, 2195. The longest duration of totality was 2 minutes, 50 seconds on March 9, 1997. All eclipses in this series occurs at the Moon’s descending node.

Series members 55–65 occur between 1901 and 2100
55 56 57

January 14, 1907

January 24, 1925

February 4, 1943
58 59 60

February 15, 1961

February 26, 1979

March 9, 1997
61 62 63

March 20, 2015

March 30, 2033

April 11, 2051
64 65

April 21, 2069

May 2, 2087

Metonic series[edit]

The metonic series repeats eclipses every 19 years (6939.69 days), lasting about 5 cycles. Eclipses occur in nearly the same calendar date. In addition, the octon subseries repeats 1/5 of that or every 3.8 years (1387.94 days). All eclipses in this table occur at the Moon's descending node.[3]

Octon series with 21 events between May 21, 1993 and August 2, 2065
May 20–21 March 8–9 December 25–26 October 13–14 August 1–2
98 100 102 104 106
May 21, 1955 March 9, 1959 December 26, 1962 October 14, 1966 August 2, 1970
108 110 112 114 116
May 21, 1974 March 9, 1978 December 26, 1981 October 14, 1985 August 1, 1989
118 120 122 124 126

May 21, 1993

March 9, 1997

December 25, 2000

October 14, 2004

August 1, 2008
128 130 132 134 136

May 20, 2012

March 9, 2016

December 26, 2019

October 14, 2023

August 2, 2027
138 140 142 144 146

May 21, 2031

March 9, 2035

December 26, 2038

October 14, 2042

August 2, 2046
148 150 152 154 156

May 20, 2050

March 9, 2054

December 26, 2057

October 13, 2061

August 2, 2065
158 160 162 164 166

May 20, 2069
March 8, 2073 December 26, 2076 October 13, 2080 August 1, 2084

See also[edit]

References[edit]

  1. ^ Wang, Qian-shen; Yang, Xin-she; Wu, Chuan-zhen; Guo, Hong-gang; Liu, Hong-chen; Hua, Chang-chai (2000-07-14). "Precise measurement of gravity variations during a total solar eclipse". Physical Review D. 62 (4): 041101(R). arXiv:1003.4947. Bibcode:2000PhRvD..62d1101W. doi:10.1103/physrevd.62.041101. ISSN 0556-2821. S2CID 6846335.
  2. ^ 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.
  3. ^ Note S1: Eclipses & Predictions in Freeth, Tony (2014). "Eclipse Prediction on the Ancient Greek Astronomical Calculating Machine Known as the Antikythera Mechanism". PLOS ONE. 9 (7): e103275. Bibcode:2014PLoSO...9j3275F. doi:10.1371/journal.pone.0103275. PMC 4116162. PMID 25075747.

External links[edit]

Photos: