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Occultation of TYC 1310-2435-1 by Tethys, 15 December 2002











Map of the shadow over Europe



Map of the shadow over Japan



Chords: the raw data





Chords: best circular fit

(allowing for offsets in times)

In order to obtain the graph above, I have allowed for offsets in time (Dt) at each station, choosing the Vitebsk timing as a reference. This is arbitratry , in the absence of criterium (at the present moment) to decide which station has the best absolute timing. Thus the Dt's listed in the table below could be changed by a constant arbitrary additive quantity, with the same conclusion as to the satellite shape.

With these offsets in time, I obtain a best circular fit to the chords with a radius of 537.2 km, and a rms radial dispersion of 6.0 km. The timing of chords 5-9 should be re-examined carefully to detect possible systematic trends in the corresponding timings, or even some interesting effects like the oblateness of Tethys.

The radius obtained here (537.2 km) is close to the equatorial radius of Tethys, as determined by Voyager :535 km.



Site

Ingress (UT)

Egress (UT)

Dt (sec)

Vitebsk

19 01 25.41

19 02 05.82

+0.00

Ooe

18 56 54.745

18 57 34.82

+0.28

Czarna

19 01 41.0

19 02 20.35

-0.01

Kooriyama

18 56 52.

18 57 31

+0.66

Hitachi

18 56 51.8

18 57 28.1

-0.54

Kashiwa

18 56 50.6

18 57 23.61

+1.34

Musashino

18 56 51.605

18 57 24.63

+0.52

Mitaka

18 56 52.

18 57 25.

+0.12



About the background image: the Atacama desert, near the border between Chile and Bolivia. The volcanoes in the skyline culminate at 5000-5500 m above sea level. This photo was taken after the Pluto occultation of 20 July 2002 (B. Sicardy).


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