Solar eclipse of March 6, 1905

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

{{Infobox solar eclipse|1905Mar06

| previous = Solar eclipse of September 9, 1904

| next = Solar eclipse of August 30, 1905

}}

An annular solar eclipse occurred at the Moon's descending node of orbit on Monday, March 6, 1905,{{cite web|title=March 6, 1905 Annular Solar Eclipse|url=https://www.timeanddate.com/eclipse/solar/1905-march-6|publisher=timeanddate|access-date=30 July 2024}}{{Cite news

| url = https://newspapers.com/article/the-age-page-4/134153668/

| date = 1905-03-06

| page = 4

| title = Page 4

| newspaper = The Age

| location = Melbourne, Victoria, Victoria, Australia

| via = Newspapers.com

| access-date = 2023-10-27

}}{{Cite news

| url = https://newspapers.com/article/the-leader-eclipse-of-the-sun/134153676/

| date = 1905-03-06

| page = 3

| title = Eclipse of the sun.

| newspaper = The Leader

| location = Orange, New South Wales, Australia

| via = Newspapers.com

| access-date = 2023-10-27

}} with a magnitude of 0.9269. 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 2.1 days before apogee (on March 8, 1905, at 7:00 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=1905&n=136|publisher=timeanddate|access-date=30 July 2024}}

Annularity was visible from Heard Island and McDonald Islands (now an Australian external territory), Australia, New Caledonia, and New Hebrides (now Vanuatu). A partial eclipse was visible for parts of Madagascar, Antarctica, Australia, and Oceania.

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=Total Solar Eclipse of 1905 Mar 06|url=https://eclipsewise.com/solar/SEprime/1901-2000/SE1905Mar06Aprime.html|publisher=EclipseWise.com|access-date=30 July 2024}}

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

|+March 6, 1905 Solar Eclipse Times

! Event

! Time (UTC)

First Penumbral External Contact

| 1905 March 06 at 02:19:16.2 UTC

First Umbral External Contact

| 1905 March 06 at 03:32:13.3 UTC

First Central Line

| 1905 March 06 at 03:35:52.7 UTC

First Umbral Internal Contact

| 1905 March 06 at 03:39:35.1 UTC

Equatorial Conjunction

| 1905 March 06 at 04:51:33.7 UTC

Greatest Duration

| 1905 March 06 at 05:10:13.7 UTC

Greatest Eclipse

| 1905 March 06 at 05:12:25.7 UTC

Ecliptic Conjunction

| 1905 March 06 at 05:19:19.8 UTC

Last Umbral Internal Contact

| 1905 March 06 at 06:45:31.2 UTC

Last Central Line

| 1905 March 06 at 06:49:14.2 UTC

Last Umbral External Contact

| 1905 March 06 at 06:52:54.4 UTC

Last Penumbral External Contact

| 1905 March 06 at 08:05:47.3 UTC

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

|+March 6, 1905 Solar Eclipse Parameters

! Parameter

! Value

Eclipse Magnitude

| 0.92691

Eclipse Obscuration

| 0.85916

Gamma

| −0.57684

Sun Right Ascension

| 23h04m40.3s

Sun Declination

| -05°55'14.1"

Sun Semi-Diameter

| 16'07.0"

Sun Equatorial Horizontal Parallax

| 08.9"

Moon Right Ascension

| 23h05m16.9s

Moon Declination

| -06°25'02.0"

Moon Semi-Diameter

| 14'45.4"

Moon Equatorial Horizontal Parallax

| 0°54'09.6"

ΔT

| 4.1 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 February–March 1905

! February 19
Ascending node (full moon) !! March 6
Descending node (new moon)

200px200px
align=center

| Partial lunar eclipse
Lunar Saros 112

Annular solar eclipse
Solar Saros 138

Related eclipses

= Eclipses in 1905 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Solar Saros 138 =

= Inex =

= Triad =

= Solar eclipses of 1902–1906 =

{{Solar eclipse set 1902–1906}}

= Saros 138 =

{{Solar Saros series 138}}

= Metonic series =

{{Solar Metonic series 1848–1935}}

= Tritos series =

{{Solar Tritos series 2003 May 31}}

= Inex series =

{{Solar Inex series 2020 December 14}}

Notes

{{reflist}}

References

{{Solar eclipse NASA reference|1901/SE1905Mar06A|19050306}}

{{Solar eclipses}}

1905 3 6

Category:1905 in science

1905 3 6

Category:March 1905