Solar eclipse of April 29, 2014

{{short description|21st-century annular solar eclipse}}

{{Infobox solar eclipse|2014Apr29

| previous = Solar eclipse of November 3, 2013

| next = Solar eclipse of October 23, 2014

}}

An annular solar eclipse occurred at the Moon's descending node of orbit on Tuesday, April 29, 2014,{{cite web|title=April 29, 2014 Annular Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/2014-april-29|publisher=timeanddate|access-date=12 August 2024}}{{Cite news

| url = https://newspapers.com/article/the-brownsville-herald-antarctic-prime-s/134096158/

| date = 2014-04-30

| page = 21

| title = Antarctic prime spot for Tuesday's solar eclipse

| newspaper = The Brownsville Herald

| location =

| via = Newspapers.com

| access-date = 2023-10-26

}} with a magnitude of 0.9868. 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. The Moon's apparent diameter was near the average diameter because it occurred 6.2 days after perigee (on April 23, 2014, at 1:20 UTC) and 7.2 days before apogee (on May 6, 2014, at 11:20 UTC).{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2014&n=136|publisher=timeanddate|access-date=12 August 2024}}

This eclipse's gamma value was closer to 1 than any other eclipse from 2000 B.C. to 3000 A.D. This means the center of the Moon's shadow passed almost exactly at the surface of the Earth, barely missing the Antarctic continent by a few kilometers, but an annular eclipse was visible from a small part of Antarctica, and a partial eclipse was visible from parts of Antarctica and Australia.

Visibility

File:SolarEclipse2014Apr29A.GIF
Animation of eclipse path

Images

File:Annular solar eclipse April 29 2014.png|Simulated annularity from Victoria Land

File:Sun setting 29Apr2014 4= (14058106922).jpg|Partial from Scarborough, Queensland, 7:03 UTC

File:Solar Eclipse (13981729529).jpg|Partial from Lake Wendouree, Victoria, 7:04 UTC

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 2014 Apr 29|url=https://eclipsewise.com/solar/SEprime/2001-2100/SE2014Apr29Aprime.html|publisher=EclipseWise.com|access-date=12 August 2024}}

class="wikitable" align="{{{align|left}}}" style="margin:{{#ifeq:{{{align}}}|left|0 0 0.5em 1em|0 1em 0.5em 0}}"

|+April 29, 2014 Solar Eclipse Times

! Event

! Time (UTC)

First Penumbral External Contact

| 2014 April 29 at 03:53:46.0 UTC

Equatorial Conjunction

| 2014 April 29 at 05:38:58.2 UTC

First Umbral External Contact

| 2014 April 29 at 05:58:45.6 UTC

Greatest Eclipse

| 2014 April 29 at 06:04:32.9 UTC

Last Umbral Internal Contact

| 2014 April 29 at 06:10:41.3 UTC

Ecliptic Conjunction

| 2014 April 29 at 06:15:28.3 UTC

Last Penumbral External Contact

| 2014 April 29 at 08:15:37.1 UTC

class="wikitable" align="{{{align|right}}}" style="margin:{{#ifeq:{{{align}}}|right|0 0 0.5em 1em|0 1em 0.5em 0}}"

|+April 29, 2014 Solar Eclipse Parameters

! Parameter

! Value

Eclipse Magnitude

| 0.98679

Eclipse Obscuration

| -

Gamma

| -0.99996

Sun Right Ascension

| 02h25m52.9s

Sun Declination

| +14°26'54.2"

Sun Semi-Diameter

| 15'52.9"

Sun Equatorial Horizontal Parallax

| 08.7"

Moon Right Ascension

| 02h26m46.0s

Moon Declination

| +13°31'06.8"

Moon Semi-Diameter

| 15'38.4"

Moon Equatorial Horizontal Parallax

| 0°57'24.1"

ΔT

| 67.3 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.

class="wikitable"

|+ Eclipse season of April 2014

! April 15
Ascending node (full moon)
!! April 29
Descending node (new moon)

200px200px
align=center

| Total lunar eclipse
Lunar Saros 122

Annular solar eclipse
Solar Saros 148

Related eclipses

= Eclipses in 2014 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Solar Saros 148 =

= Inex =

= Triad =

= Solar eclipses of 2011–2014 =

{{Solar eclipse set 2011–2014}}

= Saros 148 =

{{Solar Saros series 148}}

= Metonic series =

{{Solar Metonic series 1953–2029}}

= Tritos series =

{{Solar Tritos series 2003 May 31}}

= Inex series =

{{Solar Inex series 2014 April 29}}

Notes

{{reflist|group=Note}}

References

{{reflist}}