[find_orb] Various updates
Bill Gray
pluto at projectpluto.com
Thu Oct 28 11:31:25 EDT 2021
Hello all,
Several minor updates since my last posting in March... actually,
quite a few; my apologies for the length of this post. I should just
make smaller updates more frequently. On the bright side, there's a
lot of good stuff here; I encourage upgrading :
-- The program is now somewhat better about puzzling out an initial
orbit on its own. That mostly involved improvements in outlier
rejection. I've been focussing on this problem in recent months;
ideally, Find_Orb could be used in a fully automatic mode in which it
would read in files of astrometric data and spit out orbits unattended.
It's actually rather close to that, with the occasional "gotcha" that
I'm still working on.
-- You can specify data about your MPC code, such as primary and
secondary mirror size, sky brightness at zenith, and pointing limits
(such as an irregular horizon and/or declination limits). These will be
used in ephemeris generation to compute somewhat accurate expected SNRs
and exposure durations, and so that the ephemerides will tell you when
an object is below your "real" horizon, rather than just below altitude
0 degrees. See the file 'site_310.txt' for an example and discussion of
how to set this up.
-- User interface improvements, mostly involving the mouse. See
https://www.projectpluto.com/findhist.htm#user_interf for details.
-- In ephemeris generation, if you click on the ephemeris type (by
default, "Observables"), you get a menu of possible ephemeris types.
The "State vectors" and "Cartesian coord positions" options now also
provide options for specifying distance and time units and selecting
equatorial vs. ecliptic coordinate systems.
-- Also in ephemeris generation : if you toggle 'Show Advanced
Options' on, you'll see that one of them is 'Show explanations at end
of ephems'. These explanations will be shown for the ephemeris
quantities you've turned on, and will appear after the ephems and in
any pseudo-MPECs you generate.
-- Added a four-parameter comet non-grav model, with a parameter
reflecting a time lag between perihelion and maximum activity. See
https://www.projectpluto.com/findhist.htm#comet_dt for details. Usual
warning : don't apply non-gravs unless you really have reason to think
the object is cometary or small enough for SRP to matter.
-- You can now specify ephemerides to be from the "MPC codes" SE1
through SE5, corresponding to the Sun-Earth Lagrange 1 through 5 points.
Similarly, EM1 through EM5 are the Lagrange points for the Earth-Moon
system, and SJ1-5 for the Sun-Jupiter pair. There are further comments
on all this at https://www.projectpluto.com/findhist.htm#lagrange.
-- Magnitude band offsets now use the MPC-blessed table, so H
values should be a little closer to MPC's values.
-- Lots of minor bug fixes, and updates to MPC codes and such.
-- Bill
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