herschel outlines of astronomy

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OF ASTRONOMY
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ASTRONOMY 481
approach
of
this
comet
to
the
earth
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tf 8
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of
the
line
of
nodes.
Then
(as
in
art.
620)
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very
great
number
of
revolutions
of
both
bodies,
P
will
678 OUTLINES
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planets
whose
times
of
revo-
lution
that
the
differences
in
both
respects
are
only
what
remain
outstanding
after
the
com-
pensation
of
by
626 OUTLINES
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and
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turbed
place
may
be
assimilated,
during
its
increase,
to
the
space
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munication
of
its
predicted
place
to
Dr,
Gralle
and
of
the
new
planet
ber of times
Walker's formulas
where
the
plumb-line
would
point,
or
the
level
alone,
and
which,
when
investigated
rigorously,
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ele-
vations,
which
cannot
be
unaffected
by
difference
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than
82*
asunder.
M.
Struve,
prosecuting
the
inquiry
with
instru-
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in
the
heav-
ens,
in
this
interval
of
time,
through
orbit,
88
or
154,185,000
miles
per
annum,
or
422,000
miles
(that
is
to
say,
nearly
its
own
semidiameter)
per
diem:
in
other
words,
with
a
velocity
a
very
little
greater
than
one-
magnitude,
and
beside
it;
or
choose
two,
equally
bright,
and
784: OUTLINES
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disk,
and
sometimes
on
the
other,
the
effect
being
the
same
as
if,
the
moon
remaining
fixed,
the
eye
were
shifted
from
right
to
left
through
an
angle
equal
to
the
total
libration.
Now
this
is
the
condition
on
which
stere-
oscopic
vision
depends
Solar
apex
in
E.
A.
261
14';
N.P.D.
Solar
a
P
ex
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Benzenburg
and
Brandes;
and
Sdly,
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Qftiw.Mbar$ surface^

herschel outlines of astronomy

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