Databases (NSDC) of the Natural Planetary Satellites.
Sources and references of the data
NSDC: Database of astrometric observations of Natural Planetary Satellites
S O U R C E S O F D A T A
The observational data are taken from various
- first from printed publications (scientific journals)
and electronic publications.
- second from internal publications or notes,
more difficult to obtain, for example in Scientific papers
deposited in ALL RUSSIAN INSTITUTE OF SCIENTIFIC AND TECHNICAL
INFORMATION. Data are regularly taken in electronic form from the
Minor Planet Electronic Circulars (MPEC). Some portions of
observations come as messages from the Minor Planet Center (MPC).
- third, directly from the observers who send their data to NSDC. In that case, they are asked to
provide all the necessary information on their observations, which will be put
in the file of description of the data.
Private published databases of observations.
Our database contains data from several databases of observations
of some groups of satellites, which were composed by researchers who
used the observations to improve satellite orbits using their own
theories. These data either did not have bibliographic references to the
sources where the observations had been published or these references
were incomplete. When we have found complete bibliographic references to
all published observations, we included them into the files of
description of observations (Content). Formats of such observational data
were taken as close as possible to the initial data formats.
used the following private databases of observations:
- The catalogue of observations of the Martian satellites published by
Morley T.A. A catalogue of ground-based astrometric
observations of the Martian satellites, 1877-1982, Astronomy and
Astrophysics Supplement Series. 1989. vol. 77. n. 2. p.
This database contains observations
made from 1877 to 1982 in 23 observatories located worldwide.
T.A. Morley's database has 2212 positions of Phobos and 2600
positions of Deimos relative to Mars as well as 100 mutual positions
of the satellites. We managed to find only 3 sets of observations
with a total number of satellite positions of 34, which were made from
1877 to 1982 and were not in the catalogue of T.A. Morley.
- A catalogue of observations of Phobos and Deimos provided to us by
V.A. Shor. This catalogue had been collected to improve the orbits of
the satellites. The results of this work were published in the
paper: Shor V.A. Refinement of the orbits of Phobos and Deimos
using ground- and space-based observations.
Pis'ma v Astronomicheskii Zhurnal. Vol. 14. S. 1123-1130.
Almost all observations from the catalogue of V.A. Shor made prior to
1983 were in the catalogue of T.A. Morley. We have compared other observations
from V.A. Shor's catalogue with the publications of these observations
and included them into our database as independent sets of data.
- A catalogue of observations of the Galilean satelites of Jupiter made up
by J.-E. Arlot. These observations have been pubished in his Ph. D.:
Arlot Jean-Eudes (1982) Amelioration des
ephemerides des satellites galileens de Jupiter par l'analyse des
These de Doctorat d'etat, Obs. de Paris.
This set of data
contains 3916 positions of the four satellites.
The observations have been carried out from 1891 to 1978 in 17 observatories
all over the world.
- A catalogue of observations of the eight outer Jovian satellites made up by
P. Rocher. Part of these observations was taken from the paper:
Bordovitsyna T. V. and Bykova L. E.
Teorii dvizheniia i efemeridy VI i VII sputnikov Iupitera na 1979-2000 gody.
Tomsk : Izd-vo Tom. un-ta.
- Observations of four out of eight satellites from the catalogue of
P. Rocher were used during the construction of numerical model of motion of the
satellites. This work is described in the following paper:Rocher P.,
Chapront J. Observations and ephemerides of the faint
satellites of Jupiter. Astronomy and Astrophysics. 1996. v.311.
The catalogue of P. Rocher has 1433 observations of the eight
satellites made from 1894 to 1993 at 24 observatories located all over the world.
We have found 84 bibliographic references of publications of these observations.
- A catalogue of observations of the major Saturnian satellites made up and
described in the following paper: Strugnell P. R., Taylor D. B. A
catalogue of ground-based observations of the eight major satellites
of Saturn, 1874-1989. Astronomy and Astrophysics Supplement
Series. 1990. v. 83. n. 2. p. 289-300.
This catalogue has
26393 observations of the eight major satellites of Saturn made from
1874 to 1989 at 28 observatories located all over the world.
Contemporary sources of data for
planetary satellites observations are:
Each portion of data published in electronic circulars
contains, as a rule, three kinds of information:
- International Astronomical Union Circular (IAUC)
- Minor Planet Electronic Circulars (MPEC)
- Electronic data at CDS associated to papers published in scientific journals
Such ephemerides are suitable only at short time intervals.
- Results of observations.
- Osculating Keplerian elements of satellite orbits.
- Satellite ephemerides calculated using formulae of Keplerian
motion on the basis of determined orbital parameters.
Observational data available on-line at the Web sites of observers.
In some cases observers publish description of their observations in
scientific journals and put their data in their Internet Web site, for example there is
a Web site ftp://ftp.nofs.navy.mil/pub/outgoing/plansats.
The corresponding paper is: Stone R.C., Harris F.H. (2000) CCD
Positions Determined in the International Celestial Reference Frame
for the Outer Planets and Many of Their Satellites in
1995-1999. The Astronomical Journal. 2000. v. 119. p.
Observational data from scientific journals.
Some scientific journals (e.g., Astronomy and
Astrophysics) publish papers whose text is in the journal itself while
large tables are placed at the journal's Web site. The article has corresponding
Web links. In this way results of observations of planetary satellites are
also published. An example: Fienga
A., Arlot J.-E., Baron N., Bec-Borsenberger A., Crochot A.,
Emelyanov N., Thuillot W. CCD observations of Phoebe, 9th
satellite of Saturn. Astronomy and Astrophysics. 2002. v. 391. p.
The table with coresponding observations (plain text file)
is available on-line at http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/391/767.
Observational data entered manually from publications.
A significant number of sets of observations were added to the database
manually. From recently, we made scanning and automatic text recognition to
convert printed data into digital form. The numerical data are carefully verified
after the conversion.
Observational data from observers.
Some observational data are obtained
directly from observers as plain text files. A file describing the data
is then necessary for use.
sent electronically by the Minor Planet
The MPC receives data some containing positions of
natural satellites observed together with asteroids. These data are sent directly to
NSDC and are added to the data base.
NSDC: Bibliographic database.
S O U R C E S O F T H E
D A T A
Electronic bibliographic sources.
The first source of bibliographic references was the manual search
in all available publications. Since a few years, the main source of the bibliographic database is the
ADS Abstract Service.
This bibliographic database contains everything that is printed
in the world on astronomy. Completeness of the bibliography and user-friendly
interface have made this Web tool very popular among astronomers worldwide.
However, just this excessiveness of the database makes the search of needed
publications difficult. So, we changed the key-words in order to make easier the search for a specific
publication on the natural satellites.
Manual entries of references.
A lot of references were added to the scientific papers published in
less accessible journals such as Manuscripts deposited in ALL
RUSSIAN INSTITUTE OF SCIENTIFIC AND TECHNICAL INFORMATION and others.
Some bibliographic references were added that are not available in the
ADS Abstract Service, most of them issued from the libraries of
Paris observatory and Bureau des longitudes.
NSDC: Parameters - Data on planetary satellites and their motion.
Sources of information and references
The orbital parameters provided in our data base are mainly extracted
from the theoretical studies on Natural Satellites (cf. references in this page).
Most of the physical data come from space probes. Rotational and poles coordinates
are extracted from the publications of the Working group on Cartographic coordinates
and rotational elements of solar system objects:
Seidelmann P.K., Archinal B.A., A'Hearn M.F., Cruikshank D.P., Hilton J.L.,
Keller H.U., Oberst J., Simon J.L., Stooke P., Tholen D.J., Thomas P.C. 2005,
Cel. Mech. & Dyn. Astronomy, vol. 91, p.203.
Seidelmann P.K., Abalakin V.K., Bursa M., Davies M.E., De Bergh C., Lieske J.H.,
Oberst J., Simon J.L., Standish E.M., Stooke P., Thomas P.C. 2002,
Cel. Mech. & Dyn. Astronomy, vol. 82, p.110.
Davies M.E., Abalakin V.K., Bursa M., Lieske J.H., Morando B., Morrison D.,
Seidelmann P.K., Sinclair A.T., Yallop B., Tjuflin Y.S.1998, Report of the
IAU/IAG/COSPAR Working Group on Cartographic Coordinates and Rotational
Elements of the Planets and Satellites: 1994, Cel. Mech. & Dyn. Astronomy, vol. 63, p.127.