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SHORTER CONTRIBUTION A tidal period of 1800 years By W. DE ROP, Royal Observatory, Belgium (Manuscript Received October 5, 1970; revised version January 14, 1971) E : Eal"th P : T'n·igtJ. of th. Moo" iiPf. ot ---- .... Zine of 110J•• 0---- 5UN Fig. 2. The projection of the line of apeides on the ecliptic coincides with the line Sun-Ea.rth. If at the same time this moment of maximum influence coincides with the moment at which' the Earth is in the perihelion of its orbit, the tides will reach an absolute maximum. We will nOW consider how often such a situa- tion of maximum tides will occur. The perigee moves 0.164 358 002 0 a day relative to the node, corresponding to 360 0 in a period p 2 190.340565 days. So, when the perigee of the Moon's orbit coincides with the ascend- ing node, then this situation repeats after 2190.340565 days. This period p corresponds to 5.996 667 350 anomalistic years, thus nearly an entire number of anomalistic years. A period of 300 p corresponds to 17.990002050 anoma- listie years, hence, to exactly an entire number of anomalistic years. Thus it can be said that after exactly 17.99 centuries the coincidence of the perigee and the the Moon to the East, describes an angle of 0.111 404080 0 a day or 40.69 0 a year, thus one revolution is made in 8.84 years. If both the line of apsides is in the direction of Earth and Sun and the perigee is situated between Sun and Earth the influences of Sun and Moon on the Earth will reach a relative maximum once a month by New Moon (viz., when the Moon is in its perigee). The Swedish oceanographer O. Pettersson has presented evidence indicating that the last maximum of oceanic tides occurred about 1433. He pointed out that there is a coincidence between a tidal period of 1800 years and cli- matic changes of the same period. We think we can explain this period as follows. The time the Earth needs to move in its elliptical orbit around the Sun from the peri. helion back to this point is 365.259 641 340 days. This period is the well known anomalistic year. The line of nodes, the intersecting-line of the plane of the Earth's orbit and the plane of the Moon's orbit moves in a direction (westwards) that is opposite to the lunar movement. The angle described in the plane of the Earth's orbit by the line of nodes is 0.052 953 922 0 a day, or 19.3414 0 a year, thus one revolution is made in 18.61 years. When the line of nodes stands in the direction Sun-Earth, Sun, Earth and Moon will be situated on one line twice a month. During this particular period the gravi- tational forces of Sun and Moon on the Earth will be more intensive than in other times. 0---- - ------------f SUN \ ,,/ ", -' ; A """ orbit Fig. 1. The line of nodes of the lunar orbit coincides with the line Sun-Earth. The line of apsides, the major axis of the Moon's orbit, moving in the same direction as Tellus XXIII (1971), 3

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Page 1: A tidal period of 1800 years

SHORTER CONTRIBUTION

A tidal period of 1800 years

By W. DE ROP, Royal Observatory, Belgium

(Manuscript Received October 5, 1970; revised version January 14, 1971)

E : Eal"th

P : T'n·igtJ. of th. Moo"

iiPf. otafJ.il1~11

----.... Zine of 110J••

0----5UN

Fig. 2. The projection of the line of apeides on theecliptic coincides with the line Sun-Ea.rth.

If at the same time this moment of maximuminfluence coincides with the moment at which'the Earth is in the perihelion of its orbit, thetides will reach an absolute maximum.

We will nOW consider how often such a situa­tion of maximum tides will occur. The perigeemoves 0.164 358 002 0 a day relative to thenode, corresponding to 3600 in a period p ~

2 190.340565 days. So, when the perigee ofthe Moon's orbit coincides with the ascend­ing node, then this situation repeats after2190.340565 days. This period p correspondsto 5.996 667 350 anomalistic years, thus nearlyan entire number of anomalistic years. A periodof 300 p corresponds to 17.990002050 anoma­listie years, hence, to exactly an entire numberof anomalistic years.

Thus it can be said that after exactly 17.99centuries the coincidence of the perigee and the

the Moon to the East, describes an angle of0.111 404080 0 a day or 40.69 0 a year, thus onerevolution is made in 8.84 years. If both theline of apsides is in the direction of Earth andSun and the perigee is situated between Sunand Earth the influences of Sun and Moon onthe Earth will reach a relative maximum oncea month by New Moon (viz., when the Moon isin its perigee).

The Swedish oceanographer O. Petterssonhas presented evidence indicating that the lastmaximum of oceanic tides occurred about 1433.He pointed out that there is a coincidencebetween a tidal period of 1800 years and cli­matic changes of the same period. We think wecan explain this period as follows.

The time the Earth needs to move in itselliptical orbit around the Sun from the peri.helion back to this point is 365.259 641 340days. This period is the well known anomalisticyear.

The line of nodes, the intersecting-line of theplane of the Earth's orbit and the plane of theMoon's orbit moves in a direction (westwards)that is opposite to the lunar movement. Theangle described in the plane of the Earth'sorbit by the line of nodes is 0.052 953 922 0

a day, or 19.34140 a year, thus one revolutionis made in 18.61 years. When the line of nodesstands in the direction Sun-Earth, Sun, Earthand Moon will be situated on one line twice amonth. During this particular period the gravi­tational forces of Sun and Moon on the Earthwill be more intensive than in other times.

0---- - ------------fSUN \ ,,/ ",-' ;

A """ orbit

Fig. 1. The line of nodes of the lunar orbit coincideswith the line Sun-Earth.

The line of apsides, the major axis of theMoon's orbit, moving in the same direction as

Tellus XXIII (1971), 3

Page 2: A tidal period of 1800 years

262 W. DEl BOP

Fig. 3. After three years the line of nodes has turnedover an angle IX = 3 x 19~ 3414 = 58~0242, whilst theline of apsides described an angle {3 = 3 x 40~ 69 =122~07. Hence we have IX+{3'" 180°.

ascending node occurs on the same day of theanomalistic year.

So, if this coincidence also coincides with themoment of perihelion passage of the Earth inits orbit, this situation of double coincidencewill repeat after exactly 1799 years. Hence,

."/'

/'/

//

IIII

only once in about 1 800 years the line of nodesand the line of apsides (the Moon in its perigee)coincides with the major axis of the Earth'sorbit and the position of the Earth in theperihelion. In case of this double coincidence,the tidal forces exerted by Sun and Moon willreach an absolute maximum. Every nine yearsafterwards, the coincidence of the line of nodesand the line of apsides deviates more and morefrom the direction perihelion-Sun and finallyafter 900 years a situation will occur when lineof nodes and line of apsides coincide with themoment at which the Earth is at its aphelion.In this case a minimum of gravitational forcesfrom Sun and Moon will occur.

Other less intensive maxima are superposedon the period of 1800 years. They are causedby a coincidence of the line of nodes and theline perihelion-Sun as well as a coincidence ofthe line of apsides and the line perihelion-Sun.

In view of the present explanation we mayexpect the next maximum of tidal action aboutthe year 3233 and the minimum about 2333.

d i re a t i ont.cne of nodesafter .1 ~H~arB

""Zin. of apsidu " ............ /"after ,'r !,ears - -

REFERENCES

Pettersson, O. 1912. Klimatforandringar i historiskoch forhistoriak tid. Kungl. Svenska Vetenskaps­akademiens Handlingar, Ed. 51, no. 2.

Tellus XXIII (1971), 3