Solar eclipse of February 28, 2044 explained

An annular solar eclipse will occur at the Moon's ascending node of orbit on Sunday, February 28, 2044,[1] with a magnitude of 0.96. 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 6.7 days after apogee (on February 22, 2044, at 5:20 UTC), the Moon's apparent diameter will be smaller.[2]

While the path of annularity will be not visible from any land areas, a partial solar eclipse will be visible for parts of Antarctica and much of South America. This will be the last of 55 umbral eclipses in Solar Saros 121.

Images


Animated path

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.[3]

February 28, 2044 Solar Eclipse Times! Event! Time (UTC)
First Penumbral External Contact2044 February 28 at 18:10:40.7 UTC
Equatorial Conjunction2044 February 28 at 19:25:50.0 UTC
First Umbral External Contact2044 February 28 at 20:06:18.0 UTC
Ecliptic Conjunction2044 February 28 at 20:13:36.1 UTC
First Central Line2044 February 28 at 20:17:45.9 UTC
Greatest Duration2044 February 28 at 20:17:45.9 UTC
Greatest Eclipse2044 February 28 at 20:24:39.5 UTC
Last Central Line2044 February 28 at 20:32:09.6 UTC
Last Umbral External Contact2044 February 28 at 20:43:34.0 UTC
Last Penumbral External Contact2044 February 28 at 22:38:55.6 UTC
February 28, 2044 Solar Eclipse Parameters! Parameter! Value
Eclipse Magnitude0.96001
Eclipse Obscuration0.92161
Gamma−0.99537
Sun Right Ascension22h45m44.1s
Sun Declination-07°51'30.6"
Sun Semi-Diameter16'08.8"
Sun Equatorial Horizontal Parallax08.9"
Moon Right Ascension22h47m30.6s
Moon Declination-08°41'25.7"
Moon Semi-Diameter15'29.6"
Moon Equatorial Horizontal Parallax0°56'51.8"
ΔT80.8 s

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.

Related eclipses

Eclipses in 2044

Metonic

Tzolkinex

Half-Saros

Tritos

Solar Saros 121

Inex

Triad

Inex series

External links

Notes and References

  1. Web site: February 28, 2044 Annular Solar Eclipse. timeanddate. 14 August 2024.
  2. Web site: Moon Distances for London, United Kingdom, England. timeanddate. 14 August 2024.
  3. Web site: Annular Solar Eclipse of 2044 Feb 28. EclipseWise.com. 14 August 2024.