>predicting where the moon will be at a given time, and vice versa
>Question:  is there an easy way to understand AND remember how the moon moves
>throughout the month?

The moon's motions have been predictable since at least the 1700s, when
'lunars' were used to navigate.  'Understanding & remembering' are not my
bailiwick.  You can remember that the moon follows the sun but is 51
minutes later each day (that is an average figure -- I  _think_  it is true
at any latitude.....)

Or, instead of remembering, you could just get a moondial.  There have been
some good posts on this subject over time; I've been off the sundial list
for a year but have the earlier posts   --Peter
-----------------
Date: Sun, 18 Jan 1998 21:21:36 +0100
From: "fer j. de vries" <[EMAIL PROTECTED]>
> I tried to design a sundial for the moonlight - moon dial. But I got more
 problems than solutions. Maybe somebody can help me? 
   http://www.hs-bremen.de/planetarium and AKTUELL
What accuracy do you want?
If you want to convert "moontime" into "watchtime" there are to many
parameters.
But if the main goal is just to find the time roughly there are many
solutions.

The main part is a table with average values for the hourangle between
the moon and the sun in realtion to the age of the moon.

Roughly there are 30 days in one period from new moon to new moon.
Each day the hourangle between the moon and the sun changes about 
24 * 60 / 30 = 48 minutes.

One solution is to use an equatorial sundial and rotate the dial's plate
with n * 48 minutes in which n is the age of the moon in days from new moon.
Or make on a normal sundial a number of scales for the age of the moon
and on each scale hourpoints with an offset of n * 48 minutes.
Connect all the hourpoints and you get a moondial as in the attached
figure.
In that figure the scales for the age of the moon are circles, but that
isn't necessary.
Also the pattern of the normal sundial can be removed.

In the bulletins of the Dutch (92.5), Spanish and British (92.1) Sundial
Societies some about moondials is written.
In the book Orologi Solari by Girolamo Fantoni, Italy, you find a
capital about moondials. 
The picture in this mail is scanned from that book.  moondial.jpg
Fer de Vries.
----
a photograph of a Chinese
moondial, probably a few centuries old, was included by Joseph Needham in
Volume III of _Science & Civilisation in China_ (Cambridge: Cambridge
University Press, 1959), in Plate XLII, opposite page 309. The briefest of
references to this instrument appears on page 311.
===============
Date:         Mon, 9 Nov 1998 18:57:45 -0500
Reply-To:     History of Astronomy Discussion Group <HASTRO-
From:         Fred Sawyer <[EMAIL PROTECTED]>
Subject:      Re: moondials
You can try the following web site:

www.quns.cam.ac.uk/Queens/misc/Dial.html

You might find the following article on Moon Dialing interesting - I wrote
it for The Compendium : Journal of the North American Sundial Society.  I
have not included the graphics or computer program here, but the discussion
and example may prove useful.

Moon Dialing
Fred Sawyer
Digital COMPENDIUM  1(2)  May 1994

One of the more interesting passages attempting to explain or shed light on
the fascination the dialist has with the sundial can be found in Frank
Cousins' introduction to his book Sundials:

"The sundial still remains, despite all advances in the art of time
measurement, the one philosophical tool which combines the two poles of the
human condition most faithfully: transience and arrogance - transience in
the ephemeral nature of the shadow cast and arrogance in the use of the
gyrations of the Earth about its stupendous luminary delicately to define
the successive quanta of human existence."

      - Frank W. Cousins   1969   Sundials

Transience and arrogance.  Indeed, the image of the fleeting shadow has
often been invoked to suggest the transience of our existence and of our
works; the image has a certain natural appeal.  However, the arrogance we
show by directly using the sun to clock our daily lives is alluded to far
less often.  Perhaps we should make an effort to raise our consciousness
and seek ways to curb our arrogance.  I submit that a first step in this
direction would be to consider stepping our arrogance down a notch by using
the moon rather than the sun as our source of light and shadow.

Surely, the moon is a less stupendous luminary - if indeed it even
qualifies as a luminary, offering as it does only the reflection of
sunlight.  A moondial would clearly offer us all a lesson in humility and
at the same time provide an answer to the frequent refrain: "What do you do
to tell time when the sun goes down?"

Of course, this revelation is not new, and moondials, though rare, have
existed for at least the last three centuries.  A moondial is simply a
sundial together with some mechanism to correct for the difference between
solar and lunar hour angles.  This mechanism may take many forms:

1) A simple graph or correction table, such as may be seen here or, in a
slightly different form, on the famous Queen's College sundial in Cambridge
England.

2)  A mechanism for rotating the dial to give a direct reading, based on
the current phase of the moon, such as may be seen in Nicholas Bion's
well-known 18th century work, The Construction and Principal Uses of
Mathematical Instruments.

3)  A set of spiralling hour-lines designed to replace the usual lines and
to function correctly only in response to illumination by the moon, such as
the arrangement developed by Girolamo Fantoni (Bulletin of the British
Sundial Society 92(1):11-15, February 1992).

My goal in the present article is to provide a simple (but computer-aided)
foundation on which the insomniac dialist can begin to retrieve the
moondial from its relative obscurity and dismissal as an inaccurate
curiosity.  Even those few writers who have dealt with the moondial have
tended to give it short shrift.  Mayall suggests that one is lucky to come
within 30 minutes of the correct time; and he is correct for most earlier
treatments of the subject.  As we will see, the formulas produced here and
implemented on computer will virtually eliminate that error. 

Basic Theory

How, then, do we adapt a standard sundial for use as a moondial?  The basic
theory was outlined by Nicholas Bion in 1723 as follows:

"...the Moon by her proper Motion recedes Eastwards from the Sun every Day
about 48 Minutes of an Hour, that is, if the Moon is in Conjunction with
the Sun on any Day upon the Meridian, the next Day she will cross the
Meridian about three quarters of an Hour and some Minutes later than the
Sun: and this is the Reason that the Lunar Days are longer than the Solar
ones; a Lunar Day being that Space of Time elapsed between her Passage over
the Meridian, and her next Passage over the same; and these Days are very
unequal on account of the irregularities of the Moon's Motion."

"Now when the Moon is come to be in Opposition to the Sun, she will again
be found in the same Hour-Circle as the Sun is; so that if, for example,
the Sun should be then in the Meridian of our Antipodes, the Moon would be
in our Meridian, and consequently would shew the same Hour on our Sun-Dials
as the Sun would, if it was above the Horizon.  But this Conformity would
be of small duration, because of the Moon's retardation of about two
Minutes every Hour.  If moreover the Sun, at the Time of the Opposition, be
just setting above our Horizon, the Moon being diametrically opposite to it
will be just rising, &c...."

"[To make] the Table...used for finding the Hour of the Night by the Shadow
of the Moon upon an ordinary Dial..., draw 4 Parallel right Lines or Curves
of any length, and divide the [Center] Space...into twelve equal Parts for
12 Hours, and the two other Spaces into 15, for the 30 Lunar Days."

"First observe what Hour the Shadow of the Moon shews upon a Sun-Dial; then
find the Moon's Age, and seek the Hour correspondent thereto in the Table,
and add the Hour shewn by the Sun-Dial thereto; then their Sum, if it be
less than 12, or else it's excess above 12, will be the true Hour of the
Night.  For example; Suppose the Hour shewn upon the Sun-Dial by the Moon,
be the 6th, and her Age be 5 or 20 Days, against either of these Numbers in
the Table you will find 4, which added to 6 makes 10, and so the Hour of
the Night will be 10.  Again, Suppose the Moon shews the Hour of 9 upon the
Sun-Dial, when she is 10 or 25 Days old, against 10 and 25 in the Table you
will find 8, which added to 9, makes 17, from which 12 being taken, the
Remainder 5 will be the true Hour sought.  And so of the others."

 - From Edmund Stone's 1758 translation of Nicholas Bion's The Construction
and Principal Uses of Mathematical Instruments, Book VIII, Chapter 6.

Note that this passage is abbreviated because the actual instrument Bion
described to implement this design breaks the cardinal rule requiring that
the gnomon always be parallel to the celestial axis.  His use of the
instrument rotates the gnomon out of the north-south plane.

A Different Approach

Given the traditional reliance on knowing the current lunar age (phase) to
use a moondial, it would be natural to think that the key to a more
accurate reading is a more precise determination of the moon's phases. 
However, more precision here actually would be of little utility.  The
traditional calculation only uses the phase to determine the point of entry
in what is itself a very approximate table of data, assuming an average 48
minutes/day additional elongation from the sun's position.  For more
precision, we need to return to the fundamentals. 

Begin by selecting an hour of day to use as a reference time.  For
convenience, we use midnight Standard Time - the time when the (fictional)
mean sun crosses the longitude line half-way around the world from the
longitude line at the center of our own time zone.  Thus, the reference
time for May 1 in the Eastern Time zone is 2400 EST May 1 (or equivalently,
0500 GMT May 2). 

Next, determine the lunar and solar apparent right ascensions for the
reference times.  These values can be found from an ephemeris or from the
astronomical software available on many electronic bulletin boards. 
Although the solar right ascension does not change significantly from hour
to hour, there is a fairly large variation in the lunar value - whence the
need for selecting a reference time.

Now note that at any moment, the difference between the sun's and moon's
hour-angles equals the difference between the moon's and sun's apparent
right ascensions:

HA sun - HA moon  =  RA moon - RA sun

Thus, by calculating this difference between the apparent right ascensions,
we obtain a preliminary value for the lunar equation of time.  When this
value is added to the moon's hour-angle, which is obtained by reading the
shadow on the moondial, we have the solar hour-angle, i.e. local apparent
time.

Now modify this initial value for the equation to account for the usual
solar equation of time with which all dialists are familiar, and for the
difference in longitude between the dial's location and the central
meridian of the time zone.  These are both normal adjustments which convert
any traditional sundial reading from local apparent time first to local
mean time and then to standard time.

Finally, for convenience, add (or subtract) 12 hours to (from) the equation
as it now stands.  This modification allows us, for example, to interpret
what is normally the 10am line on the sundial as 10pm, and the noon line
thus becomes the hour-line for midnight.

We now have a lunar equation of time calculated for the moment of midnight
standard time in the dial's time zone.  This value should work very well
close to midnight; however, the never very well-behaved moon rapidly
introduces errors.  To improve accuracy at other times of night, make an
additional adjustment, after the lunar equation has been applied to the
reading, by subtracting 2 minutes for each hour that the result falls
before midnight and adding 2 minutes for each hour after midnight.  This
adjustment, which works well enough over short periods, is based on the
traditional rule of thumb which forms the basis for older moondial
treatments: the moon's elongation from the sun increases on average by 48
minutes in each 24 hour period.

All of these adjustments are incorporated into the executable program
included with this issue of the Digital COMPENDIUM.  A listing of the
QuickBASIC source code for the program is also included.  The program
produces a monthly table for the lunar equation of time and displays a
worked example of its use. 

With this equation and final adjustment, the dialist should be able to get
much improved accuracy from a moondial on any bright moon-lit night.  Of
course, for about half the nights in any given month, before and after the
new moon, there will not be enough light from the moon even to take a
reading (these nights are
roughly those shown in red on the digital moondial chart).  But for those
nights when a near full moon shining brightly through the window wakes you
from a sound sleep, you can now use your favorite dial to tell you how many
hours you have before the alarm goes off and the 20th century intrudes
again on your dialing
reverie. 

Closing Reflection

Having now finished presenting the intended material for this article, I
feel compelled to make a confession to the reader: 

Midway through the preparation it occurred to me that a good case could be
made for the charge that contriving a celestial billiard game, banking rays
of light off the moon and down to a dial - all in order to keep track of
our night hours, may yet be a step up in arrogance.  Perhaps there is no
escaping our baser nature!

----------------------------------

As an example, suppose on the night of June 21, 1994 we have a moondial
reading of 11:35 a.m. at longitude 72 degrees in the Eastern time zone.

Recall that what would be an a.m. reading on a sundial becomes p.m. on the
moondial.  The digital moon chart lists an equation for this date and
location of -1:24, thus correcting the original reading to 10:11 p.m.  This
adjustment includes allowance for the solar equation and for the 3 degree
(i.e. 12 minute) difference between the dial's longitude and the central
meridian (75 degrees) of the time zone.

Making a final adjustment of -4 minutes (since the first result is
approximately 2 hours before midnight) yields a time of 10:07 p.m. Eastern
Standard Time.

        Reading   11:35   (a.m. converted to p.m.)
        Equation    -1:24
                   ________
        First Result  10:11 p.m.
        Adjustment  -0:04
                 ________
                             10:07 p.m. Eastern Standard Time

Thus, a total correction of -1:28 is applied to the 11:35 reading to obtain
the time 10:07 p.m.  In order to see how close this result is to a
precisely calculated value, we can refer to an ephemeris, first, to find
that at 10:07
p.m. on that date the apparent right ascensions are as follows:

        Moon  16:42:57
        Sun  06:02:08
            ________
        Diff.  10:40:49 =====>> -1:19:11  (by subtracting 12 hours)

Also, at this date, time and longitude, the local apparent time
(corresponding to the sun's hour angle) is found by subtracting from
Eastern Standard Time 1 minute 50 seconds for the solar equation of time
and adding 12 minutes for the longitude difference, to obtain the result
10:17:10 p.m.  Now subtracting the difference between the right ascensions
yields an hour angle for the moon corresponding to 11:36:21, very close to
the 11:35 reading with which this example began.  Thus, in this case, the
procedure produces a value with an error of less than 1.5 minutes.
======
Date: Thu, 14 Jan 1999 18:28:42 -0500
From: Patrick Powers <[EMAIL PROTECTED]>
...there are a few examples of moon dials - the most famous in the UK
is the one at Queens College Cambridge (though I believe the Nuremburg
Diptych dials carry them too).

On the Queens College dial there is a table of 'hours correction' versus
'age of the moon, in days'.  This is simply applied to the observed reading
to convert moon time to apparent solar time.  One then applies the EoT to
get clock time.

This process is not at all accurate and, except perhaps at the moment of
full moon, is not likely to be something on which you would like to depend
for an appointment!

An interesting point is that the Queens College table is designed so that
the correction is always added whereas I believe that on other moon dials
may have to be added or subtracted.

There is an interesting article in the BSS Bulletin (No.97.1 January 1997,
p37) by Ing JTRC Schepman of the Netherlands entitled "How to determine
time by Moonlight".

In this article the author discusses these correction tables but also
describes a simple analogue instrument to convert lunar indication to
apparent solar time - it consists of concentric disks - and you may wish to
refer to that article.

Also, if you are able to get to Cambridge or can write to the Head Porter
to buy a copy, you might wish to read the blurb in the Queens College
leaflet on the dial - that too describes the way in which the simple table
works.  This dial was also discussed (albeit rather derogatorily I
thought!) by the late Charles Aked in the BSS Bulletin 94.3 October 1994.
There was another article in a BSS Bulletin (I think - though it may have
been in the NASS Compendium, my memory is not clear! - about the ease (or
otherwise!) by which a 'moon EoT' might be derived but I cannot find that
at the moment.
I suspect that these ideas only work on dials that use hour angle or
azimuth.      Patrick






_______________________________________
Peter Abrahams   [EMAIL PROTECTED]   The history of the telescope & 
   the binocular:   http://www.europa.com/~telscope/binotele.htm

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