- What is NEODyS?
- How NEODyS works
- Future expansion of NEODyS
- Credits
What is NEODyS?
Fundamentally, NEODyS provides information on Near Earth Objects
with a convenient Web-based interface. It is based on a continually
and (almost) automatically maintained database of near earth
asteroid orbits. (Comet orbits are planned for a future expansion.)
This site provides a number of services to the NEO community.
- For each NEO in our database, the results of our orbit
determination are available for inspection and comparison with
other sources. Everything needed by the user to verify our
computations is available online, including our
software.
- Our observation prediction service provides ephemeris
predictions and finder charts with information on the linear or
semi-linear
confidence region as appropriate.
- Each object is linked to a database of known physical properties.
How NEODyS works
NEODyS is based on a
Postgresql
database running on a
Linux system.
The database of orbits is continually and automatically maintained
with the most recent
Minor Planet Center
observations. The orbits are computed with the
OrbFit
software package provided by the
OrbFit Consortium.
All of the computational services provided by this site can
also be done with this software package.
Future expansion of NEODyS
NEODyS is continually expanding and improving. Here are a few of the things
on our "To Do" list.
- Uncertainties of all the quantities provided with the orbit, e.g., MOID
and absolute magnitude
- Variable time span for impact monitoring, based upon orbit uncertainty
- Inclusion of non-gravitational perturbations in the dynamic model
Credits
-
NEODyS is currently operated by a consortium with the following
participing institutions:
-
Department
of Mathematics
, University of
Pisa, Italy (in particular the Celestial Mechanics
Group):
- Andrea
Milani Comparetti is one of the founders of
NEODyS, Giovanni
F. Gronchi, and
Giacomo
Tommei are active members.
-
IASF-INAF
Rome, Italy:
- Giovanni B. Valsecchi is one of the founders
of NEODyS.
-
SpaceDyS
srl, Cascina,
Italy:
- Fabrizio
Bernardi, Andrea
Chessa, and
Alessio
Del Vigna after having worked to the system for several years
in their previous jobs at University of Pisa.
-
There are other institutions with which either we have a collaboration
which is important for the quality of the NEODyS service, or have
greatly contributed in the past to the development and operations of
the system:
- Jet Propulsion Laboratory, Pasadena (CA), USA
- Steve
Chesley is one of the founders of NEODyS. The NEODyS
automatic information system was developed by Steve while at
the University of Pisa on a NATO-sponsored postdoctoral
fellowship, under the supervision of Andrea. He wrote most of
the Perl code that transfers the output of the Fortran
programs into the database. Steve left the University of Pisa
at the end of 1999 to work at the Jet Propulsion
Laboratory. In his present position of responsible for the
NASA Sentry system he is still an essential collaborator,
because of the requirement for technical verification of the
most serious risk cases.
- Department of Applied Mathematics,
University of Valladolid, Spain:
-
María Eugenia Sansaturio and Oscar Arratia have contributed important software
segments and have also operated the system for a long time.
-
We would like also to acknowledge the following contributions:
- Hyperborea
srl, Cascina, Italy:
- Nicola Ronci and Raffaele
Guerriero have been major contributors in the development of
the original database and web interface for NEODyS. The
interface has now been replaced with one based upon the free
software PHP, but the basic ideas are the same.
-
OrbFit Consortium
- The members of this group of researchers have developed the
OrbFit
software system. OrbFit does many things, the most important ones
being orbit propagation, orbit determination, observation prediction,
close approach analysis, and orbit identification. All of the orbital
computations done by NEODyS, including the ones for impact monitoring,
are based on library routines from this package.