A11GKat

L01 · TIČAN STATION

Status

too scattered no window

Discovery

digest2 score	100
V magnitude	29.2
H magnitude	27.9
Observations	4
Arc	0.010 d
Not seen	2.65 d
NEOCP note	Updated Sept. 13.22 UT
MPC markers	none

Who observed it

Discovered by	T05 ATLAS-HKO, Haleakala
Telescope	0.5-m f/2.0 Schmidt + CCD
Usual observers	L. Denneau, R. Siverd, J. Tonry, H. Weiland
Usual measurers	L. Denneau, N. Erasmus, A. Fitzsimmons, J. Robinson, R. Siverd J. Tonry, H. Weiland

Names are the people who usually observe at that site, from Project Pluto's tables. MPC's astrometry records only the observatory code, never the individual, so these are not the observer of this particular object. Automated surveys list a telescope and no people.

Orbit

Perihelion q	0.5041 AU
Eccentricity e	0.7420
Inclination	21.5°
NEO-like	yes
Scatteredness	3849″ × 25122″ wide
Observed from L01	no

Tonight

Best altitude	no window
Exposure	—
Window	0 min
Alt / Az now	—
Sky motion	—
Moon separation	—
Sun altitude	—
Ephemeris rows	0 of 24 usable nearSun×24

Sky-plane uncertainty

Variant orbits	99
Distinct positions	97
Cloud extent	±621280″ RA · ±140897″ Dec
Scatteredness	3849″ × 25122″
L01 field	2600″ × 2600″
One pointing covers	0.0% more than one pointing needed

Drawn from MPC's own variant-orbit offsets, at the same epoch as their plot. Each orbit is one solution consistent with the observations so far; the ring marks the nominal position, and the field box appears only when it is comparable in size to the cloud.

Dot size shows how many variants share a position. MPC publishes these offsets rounded to whole arcseconds, so a tightly constrained object has thousands of orbits landing on a handful of grid points — their own picture is drawn from unrounded values and looks smoother. Sizing by count puts that density back rather than stacking invisible dots. Hover any dot for its share.