175
march 14. 1677 -
Entred
m
r. Henshaw
the Vice presid
t. tooke the chair
vpon Reading the minutes of the la
st Day wherein it was suppo
sd that the ouall
figure of

might be cau
sed by the velocity of its Dinatic
. . .turbinated or Diurnall motion
of it vpon its own Axis m
r. Henshaw obiected
that if it were soe why did it not always appear of that ouall figure when
it was seen at its greate
st Elongation as well as when it was in coniunction
w
th. the Sun. to w
ch. S
r. Ionas more
answered /added/ that m
r. Flam
stead was of opinion
that it was cau
sd by the refraction or badne
sse of the gla
sse and proceeded from
mi
stake and not from any reall appearance since he could ea
sily make it ap
pear soe w
th. any gla
sse, and that there were many other mi
stakes in the
said ob
seruation and soe could not be Relyed vpon.
But m
r. Hooke to both the
se obiections answerd fir
st that the figure of

might be really allways soe ouall as mo
r. Gallet had affirmd to haue ob
seruedit and yet through the inaduertency of others it might not be taken
notice of, and po
ssibly for want of as good gla
sses as tho
se was it might
not haue been vi
sible hereto fore. and to confirme this
. . . /he said/ mo
r Gallet had
noted that euen in this obseruation through
the 3 foot gla
sse it appeard Round
secondly the rea
sons why it may not appear Ouall in its greate
st Elongation may be
3. first that it is very small and farr Di
stant & very bright all w
ch. doe make it
very difficult vnle
sse w
th very good gla
sses to see any figure at all of its body
but only a radiating point. Secondly that being seen
. . . only part inlight
ned and neuer in opposition
&c to the Sun the whole superficies of it seen
by vs is neuer all inlightned but only some parts of it which is a sufficient
rea
son to make it appear Round though the body of it be really ouall as is
supposed ^ /a part of this ouall being really not seen whereby the ouall is toournd into a circle/ for it mu
st be a very good gla
sse by w
ch. one is able to Di
scouer the
true figure of

when half inlightne
ss by reason of its smallne
sse & radiation
and it ought to be a very much better one to Di
scouer the figure of

.
3
ly. the figure of a dark body in a light medium is much better Di
scouerd than the
figure of a light body in a dark medium by reason of
the Radiation -
next as to m
r. Flam
steads suppo
sition. m
r. Hooke said that it was noe ways pro-
bable that a man that had made the whole obseruation w
th soe much
care and w
th. soe many witne
sses, and be
sides had soe Ingeniously and knowingly
contriued the apparatus for obseruing it could either be Deceiued himself or Indea=
uour to Deceiue others. and therefore till there were better arguments than coniectures
or hypothe
ses again
st the
se circum
stances of
the obseruation we ought not to reiect or
condemn them.
vpon the mention of v
sing long tele
scopes w
th.out tubes seuerall obiections were
made as the bending of the lines the Difficulty rai
sing it and fixed it and the
like but m
r. Hooke affirmed he had actually done it that he had tryd Heuelius
his 90 foot gla
sse w
th.out a tube. though it were afterwards tryed also w
thouta tube
. . by m
r Cox at m
r Oldenburghs de
sire.
Ref: CELL/RS/HF_177 © Centre for Editing Lives and Letters