Solar eclipse of May 9, 1967

{{Infobox solar eclipse|1967May09

| previous = Solar eclipse of November 12, 1966

| next = Solar eclipse of November 2, 1967

}}

A partial solar eclipse occurred at the Moon's ascending node of orbit on Tuesday, May 9, 1967,{{cite web|title=May 9, 1967 Partial Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/1967-may-9|publisher=timeanddate|access-date=7 August 2024}} with a magnitude of 0.7201. 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 partial solar eclipse occurs in the polar regions of the Earth when the center of the Moon's shadow misses the Earth.

A partial eclipse was visible for parts of North America and Northern Europe.

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=Partial Solar Eclipse of 1967 May 09|url=https://eclipsewise.com/solar/SEprime/1901-2000/SE1967May09Pprime.html|publisher=EclipseWise.com|access-date=7 August 2024}}

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|+May 9, 1967 Solar Eclipse Times

! Event

! Time (UTC)

First Penumbral External Contact

| 1967 May 09 at 12:37:20.4 UTC

Greatest Eclipse

| 1967 May 09 at 14:42:47.7 UTC

Ecliptic Conjunction

| 1967 May 09 at 14:55:56.3 UTC

Equatorial Conjunction

| 1967 May 09 at 15:36:05.9 UTC

Last Penumbral External Contact

| 1967 May 09 at 16:47:49.8 UTC

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|+May 9, 1967 Solar Eclipse Parameters

! Parameter

! Value

Eclipse Magnitude

| 0.72009

Eclipse Obscuration

| 0.63352

Gamma

| 1.14218

Sun Right Ascension

| 03h03m17.2s

Sun Declination

| +17°16'38.0"

Sun Semi-Diameter

| 15'50.5"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 03h01m40.6s

Moon Declination

| +18°14'18.0"

Moon Semi-Diameter

| 14'51.1"

Moon Equatorial Horizontal Parallax

| 0°54'30.4"

ΔT

| 37.7 s

Eclipse season

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.

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|+ Eclipse season of April–May 1967

! April 24
Descending node (full moon)
!! May 9
Ascending node (new moon)

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| Total lunar eclipse
Lunar Saros 121

Partial solar eclipse
Solar Saros 147