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SLALIB_Version_2.3-0 Expiry 30 September 1999
The latest releases of SLALIB include the following changes:
* The 1999 January 1 UTC leap second has been added to the DAT routine.
* Four new routines have been introduced which transform between the
FK5 system and the ICRS (Hipparcos) system. FK52H and H2FK5 transform
star positions and proper motions from FK5 coordinates to Hipparcos
coordinates and vice versa. FK5HZ and HFK5Z do the same but for the
case where the Hipparcos proper motions are zero.
* Six new routines have been introduced for dealing with orbital elements.
Four of them (sla_EL2UE, sla_PV2UE, sla_UE2EL and sla_UE2PV) provide
applications with direct access to the "universal variables" method
that was already being used internally. Compared with using conventional
(angular) elements and solving Kepler's equation, the universal variables
approach has a number of advantages, including better handling of near-
parabolic orbits and greater efficiency. The remaining two routines
(sla_PERTEL and sla_PERTUE) generate updated elements by applying
major-planet perturbations. The new elements can then be used to
predict positions that are much more accurate. For minor planets,
sub-arcsecond accuracy over a decade is achievable.
* Several observatory sites have been added to the OBS routine: CFHT,
Keck 2, Gemini North, FCRAO, IRTF and CSO. The coordinates for all
the Mauna Kea sites have been updated in accordance with recent aerial
photography results made available by the Institute for Astronomy,
University of Hawaii.
P.T.Wallace
21 April 1999
ptw@star.rl.ac.uk
+44-1235-44-5372
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