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Planetary and
Lunar Coordinates 2001-2020
by Her Majesty's Nautical Almanac Office, 494 pages, 6 by 9 inches, hardbound,
includes CD-ROM with ASCII tables, 2Lbs 5 Ozs. ship wt. $29.95. (Book and CD)
Special Offer: Purchase the Astronomical Almanac 2008 plus Planetary and Lunar Coordiantes 20012020 and pay only $59.95 Save $10.00 
This book provides essential information for those people who require
low-precision astronomical positions of the Sun, Moon and planets for
tasks such as the planning of observations and the computation of cometary
orbits well into the future. It is prepared jointly by HM Nautical Almanac
Office at Rutherford Appleton Laboratory and the Nautical Almanac Office
of the United States Naval Observatory.
Phenomena for the Sun, Moon and planets are provided starting with solar
and lunar eclipses for a twenty-year period, listed in
chronological order and by type, followed by visibility maps (Lunar
and Solar)
and timing information. Principal phases of the Moon in UT to the nearest
minute are tabulated as well the instants when the Moon is nearest to
(perigee) and furthest from (apogee) the Earth. The astronomical seasons
and the instants when the Earth is closest to (perihelion) and furthest
from (aphelion) the Sun are given to a similar precision. Dates for the
passage of the Earth through the ring plane of Saturn providing optimum
views of the Saturnian satellites as well as the dates for the rare transits
of Mercury and Venus across the Sun are listed.
Greatest elongations for Mercury and Venus are provided to the nearest
hour. Oppositions, conjunctions and stationary points for the superior
planets are given to the same precision. The section on Observability
Data provides the transit time, the elongation of the planet from
the Sun and the visual magnitude for Mercury, Venus, Mars, Jupiter and
Saturn at ten-day intervals and for Uranus, Neptune and Pluto at forty-day
intervals.
The coordinates of the planets Mercury, Venus, Mars, Jupiter, Saturn,
Uranus, Neptune and Pluto are tabulated for four coordinate systems:
- geocentric equatorial spherical coordinates, i.e. right
ascension, declination, and light-time
- heliocentric equatorial rectangular coordinates
- geocentric ecliptic spherical coordinates, i.e. longitude,
latitude, and distance
- heliocentric ecliptic spherical coordinates, i.e. longitude,
latitude, and distance
If geocentric coordinates are tabulated, the position of the
Sun is also provided. Likewise, if heliocentric coordinates are tabulated, the
position of the Earth/Moon barycentre is also provided.
Geocentric and
heliocentric positions of Mercury are given at five-day intervals to a
precision of 0h.001 in right ascension, 0°.01 in declination,
longitude and latitude and 0.001astronomical units (au) in rectangular
coordinates and distances. For the Sun and the remaining planets right
ascension is given to 0h.0001 and declination, longitude and
latitude to 0°.001
and 0.0001au in rectangular coordinates and distances. Light times are given in
micro-days (approximately 0s.1) which can be used directly in the
calculation of the corrections for aberration. The tabulation interval is ten
days or forty days for Uranus, Neptune and Pluto.
Geocentric positions
of the Moon are given daily to a 0h.001 in right ascension and
0°.01in declination,
longitude and latitude. The tabulation also includes the elongation of the Moon
from the Sun at 0h and the transit time as well as rectangular
coordinates given in units of 10-7 au. Formulae and constants for
the computation of horizontal parallax and semi-diameter are given with other
data for the Moon.
Rectangular coordinates of the barycentre and the
indirect attractions of the planets on the Sun, which may be used in the
numerical integration of cometary orbits, are tabulated at ten-day intervals.
The tabulated coordinates of the Sun, Moon and planets were derived
from fundamental ephemerides computed at the Jet Propulsion Laboratory,
Pasadena, California and are given relative to the equinox and equator or
ecliptic of J2000.0.
The companion CD-ROM to this book contains
computer readable ASCII files of the planetary and lunar coordinates. The ASCII
files are similar to the tabulated data but without column headings, gaps or
pagination and Julian dates are given in full. A read.me file giving the
structure of these files is provided. |