# The American Practical Navigator/Chapter 19

# CHAPTER 19 - THE ALMANACS[edit]

## PURPOSE OF ALMANACS[edit]

### 1900. Introduction[edit]

Celestial navigation requires accurate predictions of the geographic positions of the celestial bodies observed. These predictions are available from three almanacs published annually by the United States Naval Observatory and H. M. Nautical Almanac Office, Royal Greenwich Observatory.

The *Astronomical Almanac* precisely tabulates celestial
data for the exacting requirements found in several scientific
fields. Its precision is far greater than that required by
celestial navigation. Even if the *Astronomical Almanac* is
used for celestial navigation, it will not necessarily result in
more accurate fixes due to the limitations of other aspects of
the celestial navigation process.

The *Nautical Almanac* contains the astronomical
information specifically needed by marine navigators.
Information is tabulated to the nearest 0.1' of arc and 1 second of
time. GHA and declination are available for the Sun, Moon,
planets, and 173 stars, as well as corrections necessary to reduce
the observed values to true.

The *Air Almanac* was originally intended for air
navigators, but is used today mostly by a segment of the
maritime community. In general, the information is similar to
the *Nautical Almanac*, but is given to a precision of 1' of arc
and 1 second of time, at intervals of 10 minutes (values for
the Sun and Aries are given to a precision of 0.1'). This
publication is suitable for ordinary navigation at sea, but
lacks the precision of the *Nautical Almanac*, and provides
GHA and declination for only the 57 commonly used
navigation stars.

The *Multi-Year Interactive Computer Almanac*
(MICA) is a computerized almanac produced by the U.S.
Naval Observatory. This and other web-based calculators are
available from: http://aa.usno.navy.mil. The Navy’s
STELLA program, found aboard all seagoing naval vessels,
contains an interactive almanac as well. A variety of
privately produced electronic almanacs are available as
computer programs or installed in pocket calculators. These
invariably are associated with sight reduction software which
replaces tabular and mathematical sight reduction methods.

## FORMAT OF THE NAUTICAL AND AIR ALMANACS[edit]

### 1901. *Nautical Almanac*[edit]

The major portion of the *Nautical Almanac* is devoted
to hourly tabulations of Greenwich Hour Angle (GHA)
and declination, to the nearest 0.1' of arc. On each set of
facing pages, information is listed for three consecutive
days. On the left-hand page, successive columns list GHA
of Aries (♈), and both GHA and declination of Venus,
Mars, Jupiter, and Saturn, followed by the Sidereal Hour
Angle (SHA) and declination of 57 stars. The GHA and
declination of the Sun and Moon, and the horizontal
parallax of the Moon, are listed on the right-hand page.
Where applicable, the quantities *v* and *d* are given to assist
in interpolation. The quantity *v* is the difference between
the actual change of GHA in 1 hour and a constant value
used in the interpolation tables, while *d* is the change in
declination in 1 hour. Both *v* and *d* are listed to the nearest
0.1'.

To the right of the Moon data is listed the Local Mean
Time (LMT) of sunrise, sunset, and beginning and ending
of nautical and civil twilight for latitudes from 72°N to
60°S. The LMT of moonrise and moonset at the same
latitudes is listed for each of the three days for which other
information is given, and for the following day. Magnitude
of each planet at UT 1200 of the middle day is listed at the
top of the column. The UT of transit across the celestial
meridian of Greenwich is listed as “Mer. Pass.”. The value
for the first point of Aries for the middle of the three days
is listed to the nearest 0.1' at the bottom of the Aries
column. The time of transit of the planets for the middle day
is given to the nearest whole minute, with SHA (at UT 0000
of the middle day) to the nearest 0.1', below the list of stars.
For the Sun and Moon, the time of transit to the nearest
whole minute is given for each day. For the Moon, both
upper and lower transits are given. This information is
tabulated below the rising, setting, and twilight
information. Also listed, are the equation of time for 0^{h} and
12^{h}, and the age and phase of the Moon. Equation of time
is listed, without sign, to the nearest whole second. Age is
given to the nearest whole day. Phase is given by symbol.

The main tabulation is preceded by a list of religious and civil holidays, phases of the Moon, a calendar, information on eclipses occurring during the year, and notes and a diagram giving information on the planets.

The main tabulation is followed by explanations and examples. Next are four pages of standard times (zone descriptions). Star charts are next, followed by a list of 173 stars in order of increasing SHA. This list includes the stars given on the daily pages. It gives the SHA and declination each month, and the magnitude. Stars are listed by Bayer’s name and also by popular name where applicable. Following the star list are the Polaris tables. These tables give the azimuth and the corrections to be applied to the observed altitude to find the latitude.

Following the Polaris table is a section that gives formulas and examples for the entry of almanac data, the calculations that reduce a sight, and a method of solution for position, all for use with a calculator or microcomputer. This is followed by concise sight reduction tables, with instructions and examples, for use when a calculator or traditional sight reduction tables are not available. Tabular precision of the concise tables is one minute of arc.

Next is a table for converting arc to time units. This is followed by a 30-page table called “Increments and Corrections,” used for interpolation of GHA and declination. This table is printed on tinted paper for quick location. Then come tables for interpolating for times of rise, set, and twilight; followed by two indices of the 57 stars listed on the daily pages, one index in alphabetical order, and the other in order of decreasing SHA.

Sextant altitude corrections are given at the front and back of the almanac. Tables for the Sun, stars, and planets, and a dip table, are given on the inside front cover and facing page, with an additional correction for nonstandard temperature and atmospheric pressure on the following page. Tables for the Moon, and an abbreviated dip table, are given on the inside back cover and facing page. Corrections for the Sun, stars, and planets for altitudes greater than 10°, and the dip table, are repeated on one side of a loose bookmark. The star indices are repeated on the other side.

### 1902. *Air Almanac*[edit]

As in the *Nautical Almanac*, the major portion of the *Air Almanac*
is devoted to a tabulation of GHA and declination.
However, in the *Air Almanac* values are listed at intervals of 10
minutes, to a precision of 0.1' for the Sun and Aries, and to a
precision of 1' for the Moon and the planets. Values are given for
the Sun, first point of Aries (GHA only), the three navigational
planets most favorably located for observation, and the Moon.
The magnitude of each planet listed is given at the top of its
column, and the percentage of the Moon’s disc illuminated,
waxing (+) or waning(−), is given at the bottom of each
page. Values for the first 12 hours of the day are given on
the right-hand page, and those for the second half of the day
on the back. In addition, each page has a table of the
Moon’s parallax in altitude, and below this the semidiameter
of the Sun, and both the semidiameter and age of the
Moon. Each daily page includes the LMT of moonrise and
moonset; and a difference column to find the time of
moonrise and moonset at any longitude.

Critical tables for interpolation for GHA are given on the inside front cover, which also has an alphabetical listing of the stars, with the number, magnitude, SHA, and declination of each. The same interpolation table and star list are printed on a flap which follows the daily pages. This flap also contains a star chart, a star index in order of decreasing SHA, and a table for interpolation of the LMT of moonrise and moonset for longitude.

Following the flap are instructions for the use of the almanac; a list of symbols and abbreviations in English, French, and Spanish; a list of time differences between Greenwich and other places; sky diagrams; a planet location diagram; star recognition diagrams for periscopic sextants; sunrise, sunset, and civil twilight tables; rising, setting, and depression graphs; semiduration graphs of Sunlight, twilight, and Moonlight in high latitudes; percentage of the Moon illuminated at 6 and 18 hours UT daily; a list of 173 stars by number and Bayer’s name (also popular name where there is one), giving the SHA and declination each month (to a precision of 0.1'), and the magnitude; tables for interpolation of GHA Sun and GHA ♈; a table for converting arc to time; a single Polaris correction table; an aircraft standard dome refraction table; a refraction correction table; a Coriolis correction table; and on the inside back cover, a correction table for dip of the horizon.

## USING THE ALMANACS[edit]

### 1903. Entering Arguments[edit]

The time used as an entering argument in the almanacs
is 12^{h} + GHA of the mean Sun and is denoted by UT, formerly
referred to as GMT and so referred to in this book to
avoid confusion. This scale may differ from the broadcast
time signals by an amount which, if ignored, will introduce
an error of up to 0.2' in longitude determined from astronomical
observations. The difference arises because the
time argument depends on the variable rate of rotation of
the Earth while the broadcast time signals are now based on
atomic time. Step adjustments of exactly one second are
made to the time signals as required (primarily at 24h on
December 31 and June 30) so that the difference between
the time signals and UT, as used in the almanacs, may not
exceed 0.9^{s}. If observations to a precision of better than 1^{s}
are required, corrections must be obtained from coding in
the signal, or from other sources. The correction may be applied
to each of the times of observation. Alternatively, the
longitude, when determined from observations, may be corrected
by the corresponding amount shown in Table 1903.

Correction to time signals |
Correction to longitude |
---|---|

-0.7s to -0.9s | 0.2' to east |

-0.6s to -0.3s | 0.1' to east |

-0.2s to +0.2s | no correction |

+0.3s to +0.6s | 0.1' to west |

+0.7s to +0.9s | 0.2' to west |

*Table 1903. Corrections to time.*

The main contents of the almanacs consist of data from
which the GHA and the declination of all the bodies used
for navigation can be obtained for any instant of UT. The
LHA can then be obtained with the formula:

LHA = GHA + east longitude. |

LHA = GHA - west longitude. |

For the Sun, Moon, and the four navigational planets,
the GHA and declination are tabulated directly in the
*Nautical Almanac* for each hour of GMT throughout the
year; in the *Air Almanac*, the values are tabulated for each
whole 10 m of GMT. For the stars, the SHA is given, and
the GHA is obtained from:

GHA Star = GHA ♈ + SHA Star.

The SHA and declination of the stars change slowly
and may be regarded as constant over periods of several
days or even months if lesser accuracy is required. The
SHA and declination of stars tabulated in the *Air Almanac*
may be considered constant to a precision of 1.5' to 2' for
the period covered by each of the volumes providing the
data for a whole year, with most data being closer to the
smaller value. GHA ♈, or the GHA of the first point of
Aries (the vernal equinox), is tabulated for each hour in the
*Nautical Almanac* and for each whole 10m in the *Air Almanac*.
Permanent tables list the appropriate increments to the
tabulated values of GHA and declination for the minutes
and seconds of time.

In the *Nautical Almanac*, the permanent table for
increments also includes corrections for *v*, the difference
between the actual change of GHA in one hour and a
constant value used in the interpolation tables; and *d*, the
change in declination in one hour.

In the *Nautical Almanac*, *v* is always positive unless a
negative sign (−) is shown. This occurs only in the case of
Venus. For the Sun, the tabulated values of GHA have been
adjusted to reduce to a minimum the error caused by
treating *v* as negligible; there is no *v* tabulated for the Sun.

No sign is given for tabulated values of *d*, which is positive
if declination is increasing, and negative if decreasing. The
sign of a *v* or *d* value is also given to the related correction.

In the *Air Almanac*, the tabular values of the GHA of
the Moon are adjusted so that use of an interpolation table
based on a fixed rate of change gives rise to negligible
error; no such adjustment is necessary for the Sun and
planets. The tabulated declination values, except for the
Sun, are those for the middle of the interval between the
time indicated and the next following time for which a
value is given, making interpolation unnecessary. Thus, it
is always important to take out the GHA and declination for
the time immediately *before* the time of observation.

In the *Air Almanac*, GHA ♈ and the GHA and
declination of the Sun are tabulated to a precision of 0.1'. If
these values are extracted with the tabular precision, the
“Interpolation of GHA” table on the inside front cover (and
flap) should not be used; use the “Interpolation of GHA Sun”
and “Interpolation of GHA Aries" tables, as appropriate. These
tables are found immediately preceding the Polaris Table.

### 1904. Finding GHA and Declination of the Sun[edit]

*Nautical Almanac*: Enter the daily page table with the
whole hour before the given GMT, unless the exact time is
a whole hour, and take out the tabulated GHA and
declination. Also record the *d* value given at the bottom of
the declination column. Next, enter the increments and
corrections table for the number of minutes of GMT. If
there are seconds, use the next earlier whole minute. On the
line corresponding to the seconds of GMT, extract the value
from the Sun-Planets column. Add this to the value of GHA
from the daily page. This is GHA of the Sun. Next, enter the
correction table for the same minute with the *d* value and
take out the correction. Give this the sign of the *d* value and
apply it to the declination from the daily page. This is the
declination.

The correction table for GHA of the Sun is based upon
a rate of change of 15° per hour, the average rate during a
year. At most times the rate differs slightly. The slight error
is minimized by adjustment of the tabular values. The *d*
value is the amount that the declination changes between
1200 and 1300 on the middle day of the three shown.

*Air Almanac*: Enter the daily page with the whole 10^{m}
preceding the given GMT, unless the time is itself a whole
10^{m}, and extract the GHA. The declination is extracted
without interpolation from the same line as the tabulated
GHA or, in the case of planets, the top line of the block of
six. If the values extracted are rounded to the nearest
minute, next enter the “Interpolation of GHA” table on the
inside front cover (and flap), using the “Sun, etc.” entry
column, and take out the value for the remaining minutes
and seconds of GMT. If the entry time is an exact tabulated
value, use the correction listed half a line above the entry
time. Add this correction to the GHA taken from the daily
page. This is GHA. No adjustment of declination is needed.
If the values are extracted with a precision of 0.1', the table
for interpolating the GHA of the Sun to a precision of 0.1'
must be used. Again no adjustment of declination is needed.

### 1905. Finding GHA and Declination of the Moon[edit]

*Nautical Almanac*: Enter the daily page table with the
whole hour before the given GMT, unless this time is itself
a whole hour, and extract the tabulated GHA and
declination. Record the corresponding *v* and *d* values
tabulated on the same line, and determine the sign of the *d*
value. The *v* value of the Moon is always positive (+) and
is not marked in the almanac. Next, enter the increments
and corrections table for the minutes of GMT, and on the
line for the seconds of GMT, take the GHA correction from
the Moon column. Then, enter the correction table for the
same minute with the *v* value, and extract the correction.
Add both of these corrections to the GHA from the daily
page. This is GHA of the Moon. Then, enter the same
correction table with the *d* value and extract the correction.
Give this correction the sign of the *d* value and apply it to
the declination from the daily page. This is declination.

The correction table for GHA of the Moon is based
upon the minimum rate at which the Moon’s GHA
increases, 14°19.0' per hour. The *v* correction adjusts for
the actual rate. The *v* value is the difference between the
minimum rate and the actual rate during the hour
following the tabulated time. The *d* value is the amount
that the declination changes during the hour following the
tabulated time.

*Air Almanac*: Enter the daily page with the whole 10^{m}
next preceding the given GMT, unless this time is a whole
10^{m}, and extract the tabulated GHA and the declination
without interpolation. Next, enter the “Interpolation of
GHA” table on the inside front cover, using the “Moon”
entry column, and extract the value for the remaining
minutes and seconds of GMT. If the entry time is an exact
tabulated value, use the correction given half a line above
the entry time. Add this correction to the GHA taken from
the daily page to find the GHA at the given time. No
adjustment of declination is needed.

The declination given in the table is correct for the time 5 minutes later than tabulated, so that it can be used for the 10-minute interval without interpolation, to an accuracy to meet most requirements. Declination changes much more slowly than GHA. If greater accuracy is needed, it can be obtained by interpolation, remembering to allow for the 5 minutes.

### 1906. Finding GHA and Declination of a Planet[edit]

*Nautical Almanac*: Enter the daily page table with the
whole hour before the given GMT, unless the time is a
whole hour, and extract the tabulated GHA and declination.
Record the *v* value given at the bottom of each of these
columns. Next, enter the increments and corrections table
for the minutes of GMT, and on the line for the seconds of
GMT, take the GHA correction from the Sun-planets
column. Next, enter the correction table with the *v* value
and extract the correction, giving it the sign of the *v* value.
Add the first correction to the GHA from the daily page,
and apply the second correction in accordance with its sign.
This is GHA. Then enter the correction table for the same
minute with the *d* value, and extract the correction. Give
this correction the sign of the *d* value, and apply it to the
declination from the daily page to find the declination at the
given time.

The correction table for GHA of planets is based upon
the mean rate of the Sun, 15° per hour. The *v* value is the
difference between 15° and the change of GHA of the
planet between 1200 and 1300 on the middle day of the
three shown. The *d* value is the amount the declination
changes between 1200 and 1300 on the middle day. Venus
is the only body listed which ever has a negative *v* value.

*Air Almanac*: Enter the daily page with the whole 10^{m}
before the given GMT, unless this time is a whole 10^{m}, and
extract the tabulated GHA and declination, without interpolation.
The tabulated declination is correct for the time 30^{m}
later than tabulated, so interpolation during the hour
following tabulation is not needed for most purposes. Next,
enter the “Interpolation of GHA” table on the inside front
cover, using the “Sun, etc.” column, and take out the value
for the remaining minutes and seconds of GMT. If the entry
time is an exact tabulated value, use the correction half a
line above the entry time. Add this correction to the GHA
from the daily page to find the GHA at the given time. No
adjustment of declination is needed.

### 1907. Finding GHA and Declination of a Star[edit]

If the GHA and declination of each navigational star
were tabulated separately, the almanacs would be several
times their present size. But since the sidereal hour angle and
the declination are nearly constant over several days (to the
nearest 0.1') or months (to the nearest 1'), separate tabulations
are not needed. Instead, the GHA of the first point of Aries,
from which SHA is measured, is tabulated on the daily pages,
and a single listing of SHA and declination is given for each
double page of the *Nautical Almanac*, and for an entire volume
of the *Air Almanac*. Finding the GHA is similar to
finding the GHA of the Sun, Moon, and planets.

*Nautical Almanac*: Enter the daily page table with the
whole hour before the given GMT, unless this time is a
whole hour, and extract the tabulated GHA of Aries. Also
record the tabulated SHA and declination of the star from
the listing on the left-hand daily page. Next, enter the
increments and corrections table for the minutes of GMT,
and, on the line for the seconds of GMT, extract the GHA
correction from the Aries column. Add this correction and
the SHA of the star to the GHA on the daily page to
find the GHA of the star at the given time. No adjustment
of declination is needed.

The SHA and declination of 173 stars, including Polaris and the 57 listed on the daily pages, are given for the middle of each month. For a star not listed on the daily pages, this is the only almanac source of this information. Interpolation in this table is not necessary for ordinary purposes of navigation, but is sometimes needed for precise results.

*Air Almanac*: Enter the daily page with the whole 10^{m}
before the given GMT, unless this is a whole 10^{m}, and
extract the tabulated GHA . Next, enter the “Interpolation
of GHA” table on the inside front cover, using the
“Sun, etc.” entry column, and extract the value for the
remaining minutes and seconds of GMT. If the entry time
is an exact tabulated value, use the correction given half a
line above the entry time. From the tabulation at the left side
of the same page, extract the SHA and declination of the
star. Add the GHA from the daily page and the two values
taken from the inside front cover to find the GHA at the
given time. No adjustment of declination is needed.

## RISING, SETTING, AND TWILIGHT[edit]

### 1908. Rising, Setting, and Twilight[edit]

In both *Air* and *Nautical Almanacs*, the times of sunrise,
sunset, moonrise, moonset, and twilight information, at
various latitudes between 72°N and 60°S, is listed to the
nearest whole minute. By definition, rising or setting occurs
when the upper limb of the body is on the visible horizon,
assuming standard refraction for zero height of eye. Because
of variations in refraction and height of eye, computation to
a greater precision than 1 minute of time is not justified.

In high latitudes, some of the phenomena do not occur during certain periods. Symbols are used in the almanacs to indicate:

1. Sun or Moon does not set, but remains continuously above the horizon, indicated by an open rectangle.

2. Sun or Moon does not rise, but remains continuously below the horizon, indicated by a solid rectangle.

3. Twilight lasts all night, indicated by 4 slashes (////).

The *Nautical Almanac* makes no provision for finding
the times of rising, setting, or twilight in polar regions. The
*Air Almanac* has graphs for this purpose.

In the *Nautical Almanac*, sunrise, sunset, and twilight
tables are given only once for the middle of the three days
on each page opening. For navigational purposes this
information can be used for all three days. Both almanacs
have moonrise and moonset tables for each day.

The tabulations are in LMT. On the zone meridian, this
is the zone time (ZT). For every 15' of longitude the
observer’s position differs from the zone meridian, the zone
time of the phenomena differs by 1^{m}, being later if the
observer is west of the zone meridian, and earlier if east of
the zone meridian. The LMT of the phenomena varies with
latitude of the observer, declination of the body, and hour
angle of the body relative to the mean Sun.

The UT of the phenomenon is found from LMT by the formula:

UT = LMT + W Longitude |

UT = LMT - E Longitude. |

To use this formula, convert the longitude to time using the table on page i or by computation, and add or subtract as indicated. Apply the zone description (ZD) to find the zone time of the phenomena.

Sunrise and sunset are also tabulated in the tide tables (from 76°N to 60°S).

### 1909. Finding Times of Sunrise and Sunset[edit]

To find the time of sunrise or sunset in the
*Nautical Almanac*, enter the table on the daily
page, and extract the LMT for the latitude next smaller
than your own (unless it is exactly the same).
Apply a correction from Table I on
almanac page xxxii to interpolate for latitude, determining
the sign by inspection. Then convert LMT to ZT using the
difference of longitude between the local and zone
meridians.

For the *Air Almanac*, the procedure is the same as for
the *Nautical Almanac*, except that the LMT is taken from
the tables of sunrise and sunset instead of from the daily
page, and the latitude correction is by linear interpolation.
The tabulated times are for the Greenwich meridian.
Except in high latitudes near the time of the equinoxes, the
time of sunrise and sunset varies so little from day to day
that no interpolation is needed for longitude. In high
latitudes interpolation is not always possible. Between two
tabulated entries, the Sun may in fact cease to set. In this
case, the time of rising and setting is greatly influenced by
small variations in refraction and changes in height of eye.

### 1910. Twilight[edit]

Morning twilight ends at sunrise, and evening twilight
begins at sunset. The time of the darker limit can be found
from the almanacs. The time of the darker limits of both
civil and nautical twilights (center of the Sun 6° and 12°,
respectively, below the celestial horizon) is given in the
*Nautical Almanac*. The *Air Almanac* provides tabulations
of civil twilight from 60°S to 72°N. The brightness of the
sky at any given depression of the Sun below the horizon
may vary considerably from day to day, depending upon
the amount of cloudiness, haze, and other atmospheric
conditions. In general, the most effective period for
observing stars and planets occurs when the center of the
Sun is between about 3° and 9° below the celestial horizon.
Hence, the darker limit of civil twilight occurs at about the
mid-point of this period. At the darker limit of nautical
twilight, the horizon is generally too dark for good
observations.

At the darker limit of astronomical twilight (center of
the Sun 18° below the celestial horizon), full night has set
in. The time of this twilight is given in the
*Astronomical Almanac*. Its approximate value can be determined by
extrapolation in the *Nautical Almanac*, noting that the
duration of the different kinds of twilight is proportional to
the number of degrees of depression for the center of the
Sun. More precise determination of the time at which the
center of the Sun is any given number of degrees below the
celestial horizon can be determined by a large-scale
diagram on the plane of the celestial meridian, or by
computation. Duration of twilight in latitudes higher than
65°N is given in a graph in the Air Almanac.

In both *Nautical* and *Air Almanacs*, the method of
finding the darker limit of twilight is the same as that for
sunrise and sunset.

Sometimes in high latitudes the Sun does not rise but
twilight occurs. This is indicated in the *Air Almanac* by a
solid black rectangle symbol in the sunrise and sunset
column. To find the time of beginning of morning twilight,
subtract half the duration of twilight as obtained from the
duration of twilight graph from the time of meridian transit
of the Sun; and for the time of ending of evening twilight,
add it to the time of meridian transit. The LMT of meridian
transit never differs by more than 16.4^{m} (approximately)
from 1200. The actual time on any date can be determined
from the almanac.

### 1911. Moonrise and Moonset[edit]

Finding the time of moonrise and moonset is similar to finding the time of sunrise and sunset, with one important difference. Because of the Moon’s rapid change of declination, and its fast eastward motion relative to the Sun, the time of moonrise and moonset varies considerably from day to day. These changes of position on the celestial sphere are continuous, as moonrise and moonset occur successively at various longitudes around the Earth. Therefore, the change in time is distributed over all longitudes. For precise results, it would be necessary to compute the time of the phenomena at any given place by lengthy complex calculation. For ordinary purposes of navigation, however, it is sufficiently accurate to interpolate between consecutive moonrises or moonsets at the Greenwich meridian. Since apparent motion of the Moon is westward, relative to an observer on the Earth, interpolation in west longitude is between the phenomenon on the given date and the following one. In east longitude it is between the phenomenon on the given date and the preceding one.

To find the time of moonrise or moonset in the *Nautical Almanac*,
enter the daily-page table with latitude, and extract
the LMT for the tabulated latitude next smaller than the
observer’s latitude (unless this is an exact tabulated value).
Apply a correction from table I of almanac page xxxii to
interpolate for latitude, determining the sign of the correction
by inspection. Repeat this procedure for the day following
the given date, if in west longitude; or for the day preceding,
if in east longitude. Using the difference between these two
times, and the longitude, enter table II of the almanac on the
same page and take out the correction. Apply this correction
to the LMT of moonrise or moonset at the Greenwich
meridian on the given date to find the LMT at the position of
the observer. The sign to be given the correction is such as to
make the corrected time fall between the times for the two
dates between which interpolation is being made. This is
nearly always positive (+) in west longitude and negative (−)
in east longitude. Convert the corrected LMT to ZT.

To find the time of moonrise or moonset by the
*Air Almanac* for the given date, determine LMT for the
observer’s latitude at the Greenwich meridian in the same
manner as with the *Nautical Almanac*, except that linear
interpolation is made directly from the main tables, since no
interpolation table is provided. Extract, also, the value from
the “Diff.” column to the right of the moonrise and moonset
column, interpolating if necessary. This “Diff.” is the halfdaily
difference. The error introduced by this approximation
is generally not more than a few minutes, although
it increases with latitude. Using this difference, and the
longitude, enter the “Interpolation of moonrise, moonset”
table on flap F4 of the *Air Almanac* and extract the
correction. The *Air Almanac* recommends taking the
correction from this table without interpolation. The results
thus obtained are sufficiently accurate for ordinary
purposes of navigation. If greater accuracy is desired, the
correction can be taken by interpolation. However, since
the “Diff.” itself is an approximation, the *Nautical Almanac*
or computation should be used if accuracy is a consideration.
Apply the correction to the LMT of moonrise or
moonset at the Greenwich meridian on the given date to
find the LMT at the position of the observer. The correction
is positive (+) for west longitude, and negative (−) for east
longitude, unless the “Diff.” on the daily page is preceded
by the negative sign (−), when the correction is negative (−)
for west longitude, and positive (+) for east longitude. If the
time is near midnight, record the date at each step, as in the
*Nautical Almanac* solution.

As with the Sun, there are times in high latitudes when
interpolation is inaccurate or impossible. At such periods, the
times of the phenomena themselves are uncertain, but an
approximate answer can be obtained by the Moonlight graph
in the *Air Almanac*, or by computation. With the Moon, this
condition occurs when the Moon rises or sets at one latitude,
but not at the next higher tabulated latitude, as with the Sun. It
also occurs when the Moon rises or sets on one day, but not on
the preceding or following day. This latter condition is
indicated in the *Air Almanac* by the symbol * in the “Diff.”
column.

Because of the eastward revolution of the Moon around the Earth, there is one day each synodical month (29½ days) when the Moon does not rise, and one day when it does not set. These occur near last quarter and first quarter, respectively. Since this day is not the same at all latitudes or at all longitudes, the time of moonrise or moonset found from the almanac may occasionally be the preceding or succeeding one to that desired. When interpolating near midnight, caution will prevent an error.

The effect of the revolution of the Moon around the
Earth is to cause the Moon to rise or set later from day to
day. The daily retardation due to this effect does not differ
greatly from 50^{m}. However, the change in declination of the
Moon may increase or decrease this effect. This effect
increases with latitude, and in extreme conditions it may be
greater than the effect due to revolution of the Moon.
Hence, the interval between successive moonrises or
moonsets is more erratic in high latitudes than in low
latitudes. When the two effects act in the same direction,
daily differences can be quite large. When they act in
opposite directions, they are small, and when the effect due
to change in declination is larger than that due to revolution,
the Moon sets earlier on succeeding days.

This condition is reflected in the *Air Almanac* by a negative
“Diff.” If this happens near the last quarter or first
quarter, two moonrises or moonsets might occur on the
same day, one a few minutes after the day begins, and the
other a few minutes before it ends, as on June 8, 2002,
where two moonrises occur at latitude 72°. Interpolation for
longitude is always made between consecutive moonrises
or moonsets, regardless of the days on which they fall.
Beyond the northern limits of the almanacs the values
can be obtained from a series of graphs given near the back
of the *Air Almanac*. For high latitudes, graphs are used instead
of tables because graphs give a clearer picture of
conditions, which may change radically with relatively little
change in position or date. Under these conditions
interpolation to practical precision is simpler by graph than
by table. In those parts of the graph which are difficult to
read, the times of the phenomena’s occurrence are uncertain,
being altered considerably by a relatively small change
in refraction or height of eye.

On all of these graphs, any given latitude is represented by a horizontal line and any given date by a vertical line. At the intersection of these two lines the duration is read from the curves, interpolating by eye between curves.

The “Semiduration of Sunlight” graph gives the number of hours between sunrise and meridian transit or between meridian transit and sunset. The dot scale near the top of the graph indicates the LMT of meridian transit, the time represented by the minute dot nearest the vertical dateline being used. If the intersection occurs in the area marked “Sun above horizon,” the Sun does not set; and if in the area marked “Sun below horizon,” the Sun does not rise. The “Duration of Twilight” graph gives the number of hours between the beginning of morning civil twilight (center of Sun 6° below the horizon) and sunrise, or between sunset and the end of evening civil twilight. If the Sun does not rise, but twilight occurs, the time taken from the graph is half the total length of the single twilight period, or the number of hours from beginning of morning twilight to LAN, or from LAN to end of evening twilight. If the intersection occurs in the area marked “continuous twilight or Sunlight,” the center of the Sun does not move more than 6° below the horizon, and if in the area marked “no twilight nor Sunlight,” the Sun remains more than 6° below the horizon throughout the entire day.

The “Semiduration of Moonlight” graph gives the number of hours between moonrise and meridian transit or between meridian transit and moonset. The dot scale near the top of the graph indicates the LMT of meridian transit, each dot representing one hour. The phase symbols indicate the date on which the principal Moon phases occur, the open circle indicating full Moon and the dark circle indicating new Moon. If the intersection of the vertical dateline and the horizontal latitude line falls in the “Moon above horizon” or “Moon below horizon” area, the Moon remains above or below the horizon, respectively, for the entire 24 hours of the day.

If approximations of the times of moonrise and moonset are sufficient, the semiduration of Moonlight is taken for the time of meridian passage and can be used without adjustment. When an estimated time of rise falls on the preceding day, that phenomenon may be recalculated using the meridian passage and semiduration for the day following. When an estimated time of set falls on the following day, that phenomenon may be recalculated using meridian passage and semiduration for the preceding day. For more accurate results (seldom justified), the times on the required date and the adjacent date (the following date in W longitude and the preceding date in E longitude) should be determined, and an interpolation made for longitude, as in any latitude, since the intervals given are for the Greenwich meridian.

Sunlight, twilight, and Moonlight graphs are not given for south latitudes. Beyond latitude 65°S, the northern hemisphere graphs can be used for determining the semiduration or duration, by using the vertical dateline for a day when the declination has the same numerical value but opposite sign. The time of meridian transit and the phase of the Moon are determined as explained above, using the correct date. Between latitudes 60°S and 65°S, the solution is made by interpolation between the tables and the graphs.

Other methods of solution of these phenomena are
available. The Tide Tables tabulate sunrise and sunset from
latitude 76°N to 60°S. Semiduration or duration can be
determined graphically using a diagram on the plane of the
celestial meridian, or by computation. When computation is
used, solution is made for the meridian angle at which the
required negative altitude occurs. The meridian angle
expressed in time units is the semiduration in the case of
sunrise, sunset, moonrise, and moonset; and the semiduration
of the combined Sunlight and twilight, or the time
from meridian transit at which morning twilight begins or
evening twilight ends. For sunrise and sunset the altitude
used is (−)50'. Allowance for height of eye can be made by
algebraically subtracting (numerically adding) the dip
correction from this altitude. The altitude used for twilight
is (−)6°, (−)12°, or (−)18° for civil, nautical, or astronomical
twilight, respectively. The altitude used for moonrise and
moonset is −34' − SD + HP, where SD is semidiameter and
HP is horizontal parallax, from the daily pages of the
*Nautical Almanac*.

### 1912. Rising, Setting, and Twilight on a Moving Craft[edit]

Instructions to this point relate to a fixed position on the Earth. Aboard a moving craft the problem is complicated somewhat by the fact that time of occurrence depends upon the position of the craft, which itself depends on the time. At ship speeds, it is generally sufficiently accurate to make an approximate mental solution and use the position of the vessel at this time to make a more accurate solution. If greater accuracy is required, the position at the time indicated in the second solution can be used for a third solution. If desired, this process can be repeated until the same answer is obtained from two consecutive solutions. However, it is generally sufficient to alter the first solution by 1m for each 15' of longitude that the position of the craft differs from that used in the solution, adding if west of the estimated position, and subtracting if east of it. In applying this rule, use both longitudes to the nearest 15'. The first solution is the first estimate; the second solution is the second estimate.