Middle of eclipse season December 30
The annular solar eclipse on December 26, 2019, happened some four days before the middle of the eclipse season, which came to pass onDecember 30, 2019. An eclipse season lasts for approximately 35 days, and any new moon or full moon occurring within this time period will undergo an eclipse. Given that the lunar month (period of time between successive new moons or successive full moons) is about 29.5 days long, a minimum of two eclipses (one solar and one lunar, in either order), or a maximum of three eclipses (either lunar/solar/lunar, or solar/lunar/solar) can take place in one eclipse season.
Most often, there are only two eclipses in one eclipse season. For three eclipses to occur, the first one has to come quite early in the eclipse season to allow for a third eclipse near the end.
This time around, there are two eclipses in one eclipse season. The solar eclipse on December 26, 2019, took place about four days before the middle of the eclipse season, whereas the lunar eclipse on January 10, 2020, occurs a solid 11 days after the midpoint of the eclipse season. Because this lunar eclipse happens rather late in the eclipse season, the upcoming new moon on January 10, 2020, won’t even meet up with the Earth’s dark umbral shadow. Rather, it’ll be a penumbral eclipse of the moon, whereby the moon sweeps through the faint penumbral shadow but misses the dark umbra, as depicted on the diagram below.
However, if an eclipse happens fairly close to the mid-point of the eclipse season, as the annular solar eclipse on December 26, 2019, did, then you have a central eclipse. If it’s a solar eclipse, the central eclipse presents either a total or annular eclipse of the sun; or if it’s a lunar eclipse, the central eclipse features a total eclipse of the moon. If the eclipse falls near the beginning or the end of the eclipse season, it’s either a penumbral eclipse of the moon or small partial eclipse of the sun.
Eclipses of the new moon and full moon don’t occur every month. That’s because the moon’s orbital plane is inclined by about 5 degrees to the plane of the ecliptic (Earth’s orbital plane). But the moon’s orbital path does intersect the Earth’s orbital plane at two points called nodes. Whenever these lunar nodes point directly at the sun, it marks the midpoint of the eclipse season. The lunar nodes line up with the sun in periods of about 173.3 days, or nearly 10 days shy of six calendar months. Therefore, the middle of the eclipse season will next recur around the June 2020 solstice, when the line of nodes once again points directly at the sun.
Because the lunar eclipses will happen so early and so late in the June/July 2020 eclipse season, the lunar eclipses on June 5, 2020, and July 5, 2020, will be extremely faint and hard-to-see penumbral lunar eclipses. See the illustration of these eclipses below.
On the other hand, the solar eclipse on June 21, 2020, which takes place almost dead center in the eclipse season, will present a central eclipse, exhibiting an annular eclipse of the sun. See diagram above.
Thirty-eight eclipse seasons (19 eclipse years) are almost exactly commensurate to 223 lunar months, a period of 18 years and 11 1/3 days (four intervening leap years) or 18 years and 10 1/3 days (5 intervening leap years). Therefore, the eclipses coming up in June/July 2038 display similar geometries to those in June/July 2020. This 223-lunar-month period of time is known as the Saros.
The year 2020:
The year 2038:
Interestingly, the Sar or Half Saros, representing a period of 111.5 lunar months (9 years and 5 2/3 days), gives us alternating eclipses (solar/lunar/solar) of similar character. Contrast the years 2020 and 2038 above with the years 2029 and 2047 below.
The year 2029:
The year 2047:
The eclipse master Fred Espenak tells us a Saros series can last anywhere from 1,226 to 1,550 years and is made up of 69 to 87 eclipses. A Saros series, whether it be solar or lunar, always starts off with skimpy eclipses and ends with skimpy eclipses. The middle of a Saros series brings about the closest alignment of the three celestial bodies – Earth, sun and moon – whereby they line up almost perfectly in space.
In any eclipse season where there are three eclipses, the first and third eclipses are meager productions whereas the middle eclipse is a highly visible central eclipse. And in any Saros series, the early and late eclipses are also paltry at best, whereas the middle part of a Saros series presents central eclipses.
Here’s something that may surprise you: Any eclipse happening early in an eclipse season always occurs late in a Saros series – and vice versa. For example, let’s look at the upcoming three-eclipse season in June/July 2020:
The year 2020:
The first eclipse of the eclipse season on June 5, 2020, belongs to Lunar Saros 111 and presents the 67th of 71 eclipses in this Saros series. Yet, the third and final eclipse of the eclipse season on July 5, 2020, belongs to Lunar Saros 149, and features the third of 71 eclipses in this particular Saros series.
Unsurprisingly, perhaps, the second (or middle) eclipse of the eclipse season on June 21, 2020, is the 36th of 70 eclipses in Solar Saros 137.
Bottom line: The middle of the eclipse season fell on December 30, 2019, and this eclipse season hosts two eclipses: an annular solar eclipse that occurred on December 26, 2019, and an upcoming penumbral lunar eclipse on January 10, 2020. The following eclipse season coming less than six calendar months thereafter will produce three eclipses (lunar/solar/lunar), though only the second of these three eclipses – the annular “ring of fire” eclipse on June 21, 2020 – will produce any real theatrics on the great stage of the sky.