January 2000 lunar eclipse

{{Short description|Total lunar eclipse of 21 January 2000}}

{{Use dmy dates|date=August 2018}}

{{Infobox lunar eclipse

| type = total

| image = Eclipse Lunar Total 21.01.2000 (cropped).jpg

| caption = Partial from Buenos Aires, 3:20 UTC

| date = January 21, 2000

| gamma = −0.2957

| magnitude = 1.3246

| saros_ser = 124

| saros_no = 48 of 74

| totality = 76 minutes, 59 seconds

| partiality = 203 minutes, 19 seconds

| penumbral = 318 minutes, 12 seconds

| p1 = 02:04:26

| u1 = 03:01:50

| u2 = 04:05:01

| greatest = 04:43:31

| u3 = 05:22:00

| u4 = 06:25:09

| p4 = 07:22:38

| previous = July 1999

| next = July 2000

}}

A total lunar eclipse occurred at the Moon’s ascending node of orbit on Friday, January 21, 2000,{{cite web|title=January 20–21, 2000 Total Lunar Eclipse (Blood Moon)|url=https://www.timeanddate.com/eclipse/lunar/2000-january-21|publisher=timeanddate|access-date=12 November 2024}} with an umbral magnitude of 1.3246. A lunar eclipse occurs when the Moon moves into the Earth's shadow, causing the Moon to be darkened. A total lunar eclipse occurs when the Moon's near side entirely passes into the Earth's umbral shadow. Unlike a solar eclipse, which can only be viewed from a relatively small area of the world, a lunar eclipse may be viewed from anywhere on the night side of Earth. A total lunar eclipse can last up to nearly two hours, while a total solar eclipse lasts only a few minutes at any given place, because the Moon's shadow is smaller. Occurring about 1.5 days after perigee (on January 19, 2000, at 17:50 UTC), the Moon's apparent diameter was larger.{{cite web|title=Moon Distances for London, United Kingdom, England|url=https://www.timeanddate.com/astronomy/moon/distance.html?year=2000&n=136|publisher=timeanddate|access-date=12 November 2024}}

Visibility

The eclipse was completely visible over most of North America, South America, and western Europe, seen rising over the Pacific Ocean and setting over Africa, Europe, and west Asia.{{cite web|title=Total Lunar Eclipse of 2000 Jan 21|url=https://eclipse.gsfc.nasa.gov/LEplot/LEplot1951/LE2000Jan21T.pdf|publisher=NASA|access-date=12 November 2024}}

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Hourly motion shown right to left

Eclipse details

Shown below is a table displaying details about this particular lunar eclipse. It describes various parameters pertaining to this eclipse.{{cite web|title=Total Lunar Eclipse of 2000 Jan 21|url=https://eclipsewise.com/lunar/LEprime/1901-2000/LE2000Jan21Tprime.html|publisher=EclipseWise.com|access-date=12 November 2024}}

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|+January 21, 2000 Lunar Eclipse Parameters

! Parameter

! Value

Penumbral Magnitude

| 2.30601

Umbral Magnitude

| 1.32459

Gamma

| −0.29571

Sun Right Ascension

| 20h10m32.9s

Sun Declination

| -20°03'20.2"

Sun Semi-Diameter

| 16'15.2"

Sun Equatorial Horizontal Parallax

| 08.9"

Moon Right Ascension

| 08h10m24.0s

Moon Declination

| +19°45'29.3"

Moon Semi-Diameter

| 16'33.7"

Moon Equatorial Horizontal Parallax

| 1°00'46.8"

ΔT

| 63.8 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.

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|+ Eclipse season of January–February 2000

! January 21
Ascending node (full moon)
!! February 5
Descending node (new moon)

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| Total lunar eclipse
Lunar Saros 124

Partial solar eclipse
Solar Saros 150

Related eclipses

= Eclipses in 2000 =

= Metonic =

= Tzolkinex =

= Half-Saros =

= Tritos =

= Lunar Saros 124 =

= Inex =

= Triad =

= Lunar eclipses of 1998–2002 =

{{Lunar_eclipse_set_1998-2002}}

= Saros 124 =

{{Lunar Saros series 124}}

= Tritos series =

{{Lunar Tritos series January 2000}}

= Inex series =

{{Lunar Inex series January 2000}}

= Half-Saros cycle=

A lunar eclipse will be preceded and followed by solar eclipses by 9 years and 5.5 days (a half-saros).Mathematical Astronomy Morsels, Jean Meeus, p.110, Chapter 18, The half-saros This lunar eclipse is related to two annular solar eclipses of Solar Saros 131.

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!January 15, 1991

!January 26, 2009

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See also

References