Solar eclipse of August 10, 1980

{{short description|20th-century annular solar eclipse}}

{{Infobox solar eclipse|1980Aug10

| previous = Solar eclipse of February 16, 1980

| next = Solar eclipse of February 4, 1981

}}

An annular solar eclipse occurred at the Moon's ascending node of orbit on Sunday, August 10, 1980,{{cite web|title=August 10, 1980 Annular Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/1980-august-10|publisher=timeanddate|access-date=8 August 2024}} with a magnitude of 0.9727. 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. Occurring about 5 days before apogee (on August 15, 1980, at 19:00 UTC), the Moon's apparent diameter was smaller.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=1980&n=136|publisher=timeanddate|access-date=8 August 2024}}

Annularity was visible in Tabuaeran of Kiribati, Peru, Bolivia, northern Paraguay and Brazil. The whole path of annularity was east of the 180th meridian, seeing the eclipse on August 10. (However, time zone of the Line Islands including Tabuaeran was changed from UTC−10 to UTC+14 in 1995. The date of the eclipse would be August 11 if observing the present day's time zone.)

A partial eclipse was visible for parts of eastern Oceania, Hawaii, the southern United States, Mexico, Central America, the Caribbean, and South America. Most of these areas are east of the 180th meridian, seeing the eclipse on August 10, while very few islands in the Pacific Ocean are west of the 180th meridian, seeing the eclipse on August 11.

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=Annular Solar Eclipse of 1980 Aug 10|url=https://eclipsewise.com/solar/SEprime/1901-2000/SE1980Aug10Aprime.html|publisher=EclipseWise.com|access-date=8 August 2024}}

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|+August 10, 1980 Solar Eclipse Times

! Event

! Time (UTC)

First Penumbral External Contact

| 1980 August 10 at 16:14:41.9 UTC

First Umbral External Contact

| 1980 August 10 at 17:18:11.1 UTC

First Central Line

| 1980 August 10 at 17:19:35.0 UTC

First Umbral Internal Contact

| 1980 August 10 at 17:20:59.0 UTC

First Penumbral Internal Contact

| 1980 August 10 at 18:26:38.7 UTC

Greatest Duration

| 1980 August 10 at 19:04:16.8 UTC

Ecliptic Conjunction

| 1980 August 10 at 19:10:08.9 UTC

Greatest Eclipse

| 1980 August 10 at 19:12:21.1 UTC

Equatorial Conjunction

| 1980 August 10 at 19:17:07.0 UTC

Last Penumbral Internal Contact

| 1980 August 10 at 19:57:54.5 UTC

Last Umbral Internal Contact

| 1980 August 10 at 21:03:37.7 UTC

Last Central Line

| 1980 August 10 at 21:05:04.4 UTC

Last Umbral External Contact

| 1980 August 10 at 21:06:31.0 UTC

Last Penumbral External Contact

| 1980 August 10 at 22:10:03.9 UTC

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|+August 10, 1980 Solar Eclipse Parameters

! Parameter

! Value

Eclipse Magnitude

| 0.97267

Eclipse Obscuration

| 0.94609

Gamma

| −0.19154

Sun Right Ascension

| 09h22m51.8s

Sun Declination

| +15°21'02.2"

Sun Semi-Diameter

| 15'46.9"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 09h22m42.5s

Moon Declination

| +15°10'40.6"

Moon Semi-Diameter

| 15'07.1"

Moon Equatorial Horizontal Parallax

| 0°55'29.1"

ΔT

| 51.0 s

{{clear}}

Eclipse season

{{See also|Eclipse cycle}}

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. The first and last eclipse in this sequence is separated by one synodic month.

class="wikitable"

|+ Eclipse season of July–August 1980

! July 27
Descending node (full moon)
!! August 10
Ascending node (new moon)
!! August 26
Descending node (full moon)

200px200px200px
align=center

| Penumbral lunar eclipse
Lunar Saros 109

Annular solar eclipse
Solar Saros 135
Penumbral lunar eclipse
Lunar Saros 147

Related eclipses

= Eclipses in 1980 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Solar Saros 135 =

= Inex =

= Triad =

= Solar eclipses of 1979–1982 =

{{Solar eclipse set 1979–1982}}

= Saros 135 =

{{Solar Saros series 135}}

= Metonic series =

{{Solar Metonic series 1935–2018}}

= Tritos series =

{{Solar Trito series 2002 June 10}}

= Inex series =

{{Solar Inex series 2009 July 22}}

Notes

{{reflist}}

References

{{Solar eclipse NASA reference|1951/SE1980Aug10A|19800810}}

{{Solar eclipses}}

1980 8 10

Category:1980 in science

1980 8 10

Category:August 1980