T 0 D A Y
Template by Round the Bend Wizards
Observatory Residuals
Minor Planet Discoveries
2004 HJ48
2004 JY6
2005 UL1
Generate Ephemeris
Astrometric observations of any of the following objects should be sent directly to mpc@cfa.harvard.edu. Updated orbits will be available automatically through this page.
mpc@cfa.harvard.edu
2004 HJ48 2004 JY6 2005 UL1
By default, ephemerides are geocentric, begin now and are for 20 days at 1 day intervals.
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
Generate perturbed ephemerides for unperturbed orbits
Also display elements for epoch
Format for elements output:
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 . If you select 8-line MPC format the elements will be displayed with the ephemerides. If you select any format other than 8-line MPC format, only the elements are returned. In such cases your browser should download the elements file and save it to your local disk.
Ephemerides can be supplied for objects with only Väisälä elements, but the elements themselves are not supplied.
The time-scale of the supplied ephemerides is UTC.
If you desire a topocentric ephemeris, enter your observatory code in the appropriate box. When local circumstances are displayed, the azimuths are reckoned westwards from the south meridian.
As an aide-mémoire, the packed form of the object's designation (as used on the astrometric observation record) is displayed immediately above the ephemeris.
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