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Current NEOCP and PCCP orbit data

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Residuals

Complete current Find_Orb observation residuals, rebuilt only for objects whose observation set changed in a regular calculation. Each object name opens its Project Pluto pseudo-MPEC. Hover a point for its UTC observation time, observatory, measured R.A. and Dec, and residuals. The normal scale keeps the central 95 percent readable; a red-ringed point at an edge means the true residual lies beyond that scale. Hover or select the accompanying edge button to show every residual at its full position.

A11F5VI

47 observations; 47 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

A11FeGk

4 observations; 4 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

A11FgaP

7 observations; 7 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

A11FgaQ

5 observations; 5 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

LA0CemH

7 observations; 7 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

LA0CeOu

10 observations; 10 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oAio

19 observations; 19 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oAS5

10 observations; 10 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oAYQ

7 observations; 7 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oAYR

8 observations; 8 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oAZ6

6 observations; 6 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oDgH

7 observations; 7 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oDgI

6 observations; 6 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oEGq

3 observations; 3 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oEGv

10 observations; 10 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oG7V

5 observations; 5 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12oImJ

32 observations; 32 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P12onNw

55 observations; 55 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P22nJzF

43 observations; 43 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P22oDk3

8 observations; 8 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P22oDk4

5 observations; 5 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P22oG6r

8 observations; 8 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P22oG6W

8 observations; 8 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P22oG6X

5 observations; 5 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

P22osbK

36 observations; 36 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

RMM2026

80 observations; 80 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

ST26G90

20 observations; 20 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

ST26G95

36 observations; 36 displayed astrometric residual pairs. Find_Orb supplies the horizontal value as the sky-plane component ΔR.A. × cos(Dec), so both axes are directly comparable in arcseconds.

Observatory colours

The same observatory code keeps the same colour in every residual chart and table preview. Select a colour or code to highlight that observatory in all charts; select it again to clear the highlight.

Website generated by the get-cp monitor. Date: 08-02-2026