Sezione di Ricerca Asteroidi

MPCL: Critical List Astrometric Program
2016, Foglia S., Galli G.

Date of positions:      2018/12/13
Magnitude limit:        21.0
Elongation from Sun  >= 90.0

Date of MPCOrb:         2018/12/13

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          Minor Planet            R.A.  Decl. Elong. Magn.      Arc  Rms   LastObs     Code  U   NOss NOpp   Type
                                  hh.h    dd           V              "    yyymmdd
---------------------------------------------------------------------------------------------------------------------------
   2340  Hathor                07.84  -02  135.2W  19.1 1976-2014  0.62     00000    C802  2    321    7   NEA
  85938  1999 DJ4              06.84  +39  154.7W  21.0 1999-2017  0.53     00000    C803  0    600    9   NEA
 163683  2002 YP2              10.30  +45  116.8W  21.0 2002-2018  0.39     00000    C803  2    145   10   NEA
 164207  2004 GU9              11.95  +47  101.1W  21.0 2001-2018  0.49     00000    C803  2    227   13   NEA
 267221  2001 AD2              10.89  +00   96.0W  19.1 2001-2018  0.52     00000    C803  2    323   12   NEA
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Options:

By default, ephemerides are referred to MPC 203

Start date for ephemerides: Number of dates to output

Ephemeris interval: Ephemeris units: days hours minutes seconds

Observatory code:

Display positions in: truncated sexagesimal or full sexagesimal or decimal units

Display motions as: "/sec "/min "/hr °/day

Total motion and direction Separate R.A. and Decl. sky motions Separate R.A. and Decl. coordinate motions

Suppress output if sun above local horizon

Suppress output if object below local horizon

Generate perturbed ephemerides for unperturbed orbits

Also display elements for epoch

Format for elements output:

none MPC 1-line MPC 8-line
SkyMap (SkyMap Software) Guide (Project Pluto) MegaStar V4.x (E.L.B. Software)
TheSky (Software Bisque)

If you select 8-line MPC format, you may display the residual block for the objects selected:

Show residuals blocks.Show only residual lines containing observations from code .