CMO/OAA Cahier #07
Great Comet in 1680 and Flamsteed vs
This is
a translation of the Japanese articles published in the Heavens (Journal of the OAA) in 1985
(I
in August 1985 issue, II in the September 1985 issue and III in the November 1985
issue respectively).
I.
Before the
advent of Halleyfs Comet in 1985/1986, several books on Halleyfs Comet were
published also in
Any modest
description of the story says as follows: In December 1680 a great comet
appeared in the evening sky, and as pointed out by Flamsteed, this was regarded
as the same comet as the one that appeared one month before. So Isaac Newton,
considering that it obeyed his theory of universal gravitation, tried to obtain
the possible orbit of the comet to the effect that the observation values were
quite identical with the calculation values from his proposed parabolic orbit,
and so Newton said that the two comets were nothing but one and identical and
thus the orbit was correctly determined. Edmund Halley then followed
Do you
think this description is simply right? The present writer however is not quite
satisfied with this interpretation. This is because the Great Comet in 1680
should be called Flamsteedfs Comet.
@Any
reliable book describes that almost all astronomers at that time regarded the
two comets in November and December in 1680 as different comets. Here we should recall that
Recall
first that the images of the planets and comets were quite different at that
time. As to the motions of the planets, Keplerfs
three laws of planetary motion was known as necessary and sufficient laws and a
touchstone of any following theory, whereas as to the motions of comets, Keplerfs idea was widely believed that any comet must move
on a straight line whose theory was issued by him based on his observations in
1607. On this point Newton, since his second law of motion inevitably depended
on Keplerfs three laws, he was urged to believe in Keplerfs idea of straight motion of comets, and furthermore
he must have been energetic in deriving the Keplerfs
motion from his theory. At least he must have never believed that the comets
could belong to the kind of planets. As will be elucidated later he did not
believe so for quite a long time (really for several years).
On the
other hand, Flamsteed looked to have been instinctively confident from the
outset that the December 1680 Comet was the recurrence of the November 1680
Comet. The comet passed the perihelion on around 9 December, while Flamsteed
wrote as early as on 15 December to James Crompton (1648-1694) his idea clearly.
Furthermore he looked to have predicted the recurrence and wrote gI concluded that having past ye Sun it would
appear after his setting in December.h In fact he detected a part of the
tail above the evening horizon on 10 and 11 December, and on the following 12
December he found the head of the Comet. Flamsteed himself, however, did not
watch the Comet in November, but it was observed by Cuthbert, a member of the
Observatory. Flamsteed wrote also gby
what I learnt from Othersh (p315 in Ref 1), and so
it must have been possible he also had other data. Contrarily speaking,
Flamsteed was not only the first class observer, but also a first class person
who could read the astronomical data. In a sense he could be quite
revolutionary because he was not polluted by the mechanics. If it was a
revolution of Kepler in that he replaced a complete
circular orbit of the planets to an elliptic orbit, we can equally say that
Flamsteed was revolutionary in the sense he replaced the straight line orbit of
the comets into a U-turn orbit which have never been conceived by the
forerunners. Unfortunately he first considered, as was severely scolded by
We should
recall here that
But what ever there be
in these difficulties, this sways most with me that to make ye Comets of
November & December but one is to make that one paradoxical. Did it go in a
bent line other comets would do ye like & yet no such thing was ever
observed in them but rather contrary. The comets of 1665, 1677 & others
which moved towards ye Sun, or some of them at least, had they twisted about ye
Sun & not proceeding on forward gone away behind him they would have been
seen again coming from him. c.. (16 April 1681,
Newton
further suspected Flamsteedfs observation on 12
December (gI fear not altogether righth)
and persuaded Flamsteed to re-examine the data recorded on 13 January before
the publications as follows gThe greatest
difference being in Jan 13, it may perhaps be worth your while to examine your
own observation of that day before you publish it.h (p365
in Ref. 1)
It should
be recalled that this malicious situation did not change even if the following
famous comet in 1682 came and went away.
Note
however that both were not necessarily on bad terms each other at first, and Flamsteed
himself, though he was very confident in his observations and his intuition,
was like a man who wrote gI love peace
& I know very well what trouble such a publication of things besides my
province might create meeh on 7 March 1981
(Flamsteed to Crompton for Newton, p348 in Ref. 1). Such a dreadful discord
occurred later in the 1690s, and around 1681
Finally
however
With this,
Flamsteed might have been well satisfied, but it is not fair if we diminish the
problem to the problem whether the Comets of November and December were
identical or not. The true problem was concerned with the U-turn orbit of any
comet, and on this
Here we
need a bit of mention of Edmond Halley. It was after 1684 that Halley became a
minion of
At any rate
Halley must have learned much from Flamsteed, but almost kept silent during the
controversy between Flamsteed and
There
remains a question why, though the facts were as abovementioned, such an
illusionary story of the tag team of
Ref
1.
The Correspondence of
Isaac Newton, volume II 1676-1687 (Ed. by H. W.
Turnbull, Cambridge at the University Press, 1960.)
II
Isaac
Newtonfs Philosphopiæ naturalis
Principia Mathematica (abbreviated as Principia here) is a big and important
book which contains the distinguished law i.e. the second law of motion and
first published in 1687. It should be remembered that it was in 1686, the next
year of
It is natural that the
last edition was regarded as a refined and fixed edition and really the
translations of Principia which are
available to us are all those translated from the Third Edition. One of the
well-known English edition is the one by Florian Cajori (Ref. 2)
(California Univ Press, the first edition in 1934)
which based on Andrew Mottefs translation in 1729.
(They say there is another translation by R. Thorp in 1776). The first American
edition was based on A. Mottefs translation and first
published in 1846 (By Daniel Adee, NY): Ref. 3.
Japanese
translations are twofold, one published in 1971 and the other 1977. These are
also translations of the Third Edition.
As a matter
of fact, with respect to Flamsteedfs Comet, the First
Edition of the Principia must have
been most important, as easily suspected. But unfortunately as far as the
present writer knows, we cannot read the First Edition in translation.
Fortunately however, we have a very precious and important work in which all of
the foregoing variants of the Latin sentences have been investigated and cited
in the foot notes; namely the work by A. Koyré and I.
B. Cohen in 1972 (Ref. 4) by which we can narrowly know the form of the First
Edition. According to Koyré and Cohen, there seem to
exist a lots of versions including the manuscript called M1, M, E1,
E1i, E1ii,
E1a, E2,
E2i, E2ii,
E2a, and E3
where
M implies the manuscript, Ek
is
the kth
Edition, Eki is the corrections by tags or lebels,
and Eka implies an addition of comments. Especially
concerning the 1680 Comet, their variants are extraordinarily complex.
Of course,
a naïve reading will easily reveal the Third Edition contains a large number of
alterations which were made since it also contained the comet in 1723. The
following famous statements were also added after E2: gThe observations of this comet from the
beginning to the end agree as perfectly with the motion of the comet in the
orbit just now described as the motions of the planets do with the theories
from whence they are calculated; and by this agreement plainly evince that it
was one and the same comet that appeared all that time, and also that the orbit
of that comet is here rightly defined.h (Ref. 3, p.480.)
The newly cited Table just above the sentences contains the data from 3
November to 9 March and the first one was made by Gottfried Kirch
about which
First of
all, we pick out the first sentence from Exemplum; gLet the comet of the year 1680 be proposed. The following table shews the motion thereof, as observed by Flamsted, [and calculated afterwards by him from his observations,
and corrected by Dr. Halley from the same observations]h (Ref. 3, p.473)
where the parenthesis [c] is inserted
by the present writer because the part was not found in M~ E2, but occurred in E3, and this is the part inserted after
the death of Flamsteed. It is apparent that with or without [c] the very nuances of the sentences
are different. What did Halley added?
Secondly it is interesting to note that Motte
wrote Dr. Halley though the original Latin in E3 does not
imply. Motte called Flamsted without Mr (though Cajori on the other
hand replaced it by Mr. Flamsteed).
This is not trivial. This clearly proves that as was brought out the
What did
Dr. Halley correct? Halley learnt
the recurrence of comets from Flamsteed and others (J. Cassini was also a
curious teacher to Halley: In 1681, Cassini told to him that the 1680 Comet was
an incarnation or something like that of the 1577 Comet observed by Tycho as well as the 1665 April Comet). Halley was
successful in the 76 year recurrence of the 1682 Comet based on the data, but
it is well known that he also overplayed his hand by stating that the 1680
comet was the coming-back of the comets in BC44, 531, 1106
with the period of 575 years.
However,
Halley lacked and abused the accuracy about the data which are necessary for
the prediction of the 575 year period. In this respect we should point out that
to do so he made bad use of Flamsteedfs data to the
effect that by the gcorrection by Halleyh in the Third Edition the readers of
it cannot know the original correct data made by Flamsteed. Fortunately
nowadays because of the Koyré and Cohen Edition, we
can recover the original data in comparison with Halleyfs arbitrary
alterations: Apparently Dr. Halley altered the Flamsteed original observational
data in order for them to agree with the calculations which are needful for the
575 year period. Occasionally he moved the original Flamsteed data by about 2
minutes of arc notwithstanding that Flamsteedfs
accuracy at that time was said within 10 arc seconds.
Halleyfs
action, especially the framing Flamsteed up, was along with the intention of
Isaac Newton, whereas because of the meddling of Halley,
It is well
known that
From the
present point of view, the appearance of the Principia looks unnecessarily bulky and misshaped including the
notion of fluxion: Especially as far as the Book III Exemplum is concerned, we
donft understand why one needed such a complicated and intricate structure. We
donft understand how further news of observations and re-calculation did add
something more than the case of the first intuition of Flamsteed. Since in M1
(though
erased after M) already the November
Comet was stated as following the parabolic orbit for the succeeding three
months and we wonder how any further new information was given in the following
editions. Considering the ability of the calculations and observations, the
input and output were sufficiently balanced just in M1.
Study about
To be
concluded in the next by stating a bit about John Flamsteed.
Ref.
2. The
Mathematical Principles of Natural Philosophy by Sir Isaac Newton;
translated by Florian Cajori,
(California Univ Press, the first edition in 1934)
Ref.
3.
http://rack1.ul.cs.cmu.edu/is/newton/
Ref.
4.
Isaac Newtonfs Philosophiae
Naturalis Principia Mathematica,
The third Edition (1726) with Variant Readings, Assembled and edited by Alexandar Koyré and I. Bernard
Cohen with the Assistance of Anne Whitman (Harvard University Press 1972)
III
John
Flamsteed is familiar with us, the amateur astronomers, from the outset through
the Atlas Celeste de Flamsteed. However it
may not be so to those scientists and journalists who are not particularly
acquainted with the star skies, even they could write about Halleyfs
comet. N. Calder did not touch on Flamsteed when he wrote about the era
of the 1680s concerning the Principia
and pointed out the clumsiness of the latter book. The present writer was also
disappointed with the description of Collin Wilson who clearly brought a false
illusion of Galileo into light, but was very lenient towards
Some
persons criticise that Flamsteed might have been accurate and cautious in
observations but a very obstinate person, perhaps deducing something from the
fact that Flamsteed was unwilling to give some possibly inaccurate data to
Newton who needed obstinately the data for his theory of the motion of the
Moon. However to establish the Grand Theory of Motion, it was needless to
especially adhere to the strange motion of the Moon. At that time it was
premature to try to establish the theory of delicate libration
of the Moon, and it was naturally impossible for Flamsteed to well cope with it
because it was beyond the application limit. If Flamsteed responds or not, we
should say the Theory of Newton could not become better or worse.
The
conflicts between Flamsteed and
Flamsteed
was never stubborn when he communicated with
Unfortunately
the present writer has not had any opportunity to read Francis Bai1yfs account of John Flamsteed, the first royal astronomer (published in
1835) which is said to have shocked the science world, and hence the present
writer is unfit to write more, but even if we come back to the problem of the
1680 Great Comet, we can be allowed to say his maiden ideas about the comets
give free play to our imagination about Flamsteedfs
gmissed opportunitiesh in his future. We shall close so this article by picking
out a few pieces of his words.
We first
note that in the letter to Halley which was dated 17 February 1681 (as once
cited in I when we wrote how Flamsteed predicted the return of the November
Comet)*2, Flamsteed expresses that he conceives that the Sun attracts all the planets as well as all like bodys
that come within our Solar system vortex more
or lesse according to the different substance of theire bodyes and nearenesse or remotenesse from
him. As to the body of the Comet, he suggests it might have been a planet belonging formerely
to another Vortex now ruined. The reason may be that Worlds may die as well as men. *3 He also gives a
picture that the planet might have broken when the Vortex ruined and the
remainder might have carry the ghumid
partsh and further that the humid
part of ye body ye comet being outmost might cause it to have a large
atmosphere: & from both when it was neare ye Sun
the violent action of his raies upon it might carry
forth plentifull Streames
of matter to a vast distance which caused ye tayle to
appeare double the lenghth
when neare the Sun it did to the length on its
perigee where it lay most convenient to be seene
& should on yt account have appeared longest.
(p339 in Ref. 1 in I). This kind of opinion was not
common at that time, and for example, John Wallis (1616-1703), a famous English
mathematician, was one of the rebutters (on 13 August 1681, Wallis to
Flamsteed*4). Wallis considered that the comets were not permanent bodies making excursions in
certain periods into our System or Solar World. He thought rather that they
were made by ye collection of Exhalation
or Effluvia from the Æther or Ætherial
Bodies. As well, the tail was thought as a tinging of the sunbeams passing through the Head.
An
interesting fact was that Newton was partially assented*5 to
Flamsteed concerning these ideas of Flamsteed (in the letter on 28 February
1681, Newton to Crompton for Flamsteed, p340 in Ref.1): For example Newton
wrote gBesides these things wch seem obnoxious to some objections, there are some other
parts of his Theory wch I easily approve & think
will be hard to object against, as yt ye tayle of ye Comet is a thin vapour, that it rises from ye
atmosphere about the head, that ye action of ye Sunfs light conduces to raise
it, that it shines not by its own light but only by reflexion of ye Sunfs
light, & that ye atmosphere about ye head shines also by the suns light,
though perhaps not altogether by it.h It is so unfair to say such opinions
belongs to
Finally we
should like to close by citing a sentence of Flamsteed, which is the kind that
may not be written by such a digital person like
The tayle of ye
Comet was nearly but not exactly
in a streight line
being a littele curved backward,
towards ye west.
(Note)
*1. This
was a set of the words given by William Whiston (1667-1752) who succeeded Newton as Lucasian Professor of Mathematics: It conveys the
superlative as gthe most fearful,
cautious and suspicious" among the persons he met in his life.
*2. This,
also cited in I, was at the hand of Flamsteed, and so it is not the same that
Halley received. If Halley might have had, it might have been vanished. However
the similar letter looks to have been sent to
*3.
Furthermore a similar letter must have been sent to J. Wallis: In the letter of
Wallis to Flamsteed on 13 August 1681 (see *4 below), Wallis cited the set of
Flamsteed words hWorlds dying as well as menh.
*4. See p339 in Ref. 1 in I
*5. Said somewhere, the original letter
written by Flamsteed as to which
*6. This is from an extract by
On ye 10th
after sunset or indeed ye end of daylight I first saw ye tayle
ascending up from ye horizon not exactly perpendicular but enclined
a little to the right hand, it passed in the Middle betwixt ye tayle of the Serpent of Ophiuchus
& ye South wing of Aquila (ƒÂ in Bayerus) &
reared up to 3 small stars marked Awb in his said Mapps.
Masatsugu MINAMI
(uploaded in June 2009)
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