|
EAON - INFO N° 402002, SEPTEMBER to DECEMBER |
174 reports have been sent between September and December, about 156 observations (25 possibly positive) of 63 events (9 possibly positive) by 67 observers, from 15 countries. You will find in the following table the list of their abbreviations in alphabetical order, with the number of observations made by each of them.
AHO |
Mika AHO |
1 |
FI |
|
IBV |
Ivan BRYUHANOV |
1 |
BY |
AME |
Angel MASSALE |
1 |
ES |
|
IZF |
F. IZQUIERDO |
1 |
ES |
AND |
Sven ANDERSSON |
2 |
DE |
|
JHP |
Jon HARPER |
2 |
UK |
ASK |
Alan SNOOK |
1 |
UK |
|
JLX |
Jean LECACHEUX |
7 |
FR |
BAO |
Stefano BASSO |
1 |
IT |
|
JNK |
Tomas JANIK |
4 |
CZ |
BEI |
Wolfgang BEISKER |
1 |
DE |
|
JTC |
Jens Th. CARLSEN |
2 |
DK |
BOL |
Simone BOLZONI |
11 |
IT |
|
KZA |
Alain KLOTZ |
2 |
FR |
BZY |
Wojciech BURZYNSKI |
1 |
PL |
|
LAB |
Carlos LABORDENA |
3 |
ES |
CAS |
Ricard CASAS |
1 |
ES |
|
LTA |
Salvador LAHUERTA - ZAMORA |
1 |
ES |
CNS |
Oscar CANALES MORENO |
6 |
ES |
|
LTL |
Luis LAHUERTA - ZAMORA |
1 |
ES |
COF |
François COLAS |
1 |
FR |
|
LZJ |
Joan LOPEZ |
2 |
ES |
CRM |
Claudio CREMASCHINI |
1 |
IT |
|
MDT |
Ørnulf MIDTSKOGEN |
32 |
NO |
DDN |
Alberto DALLE DONNE |
1 |
IT |
|
MSS |
Stefan MESSER |
1 |
DE |
DEN |
Martin DENTEL |
3 |
DE |
|
NRL |
Remo NORELLI |
1 |
IT |
DGE |
Patrick DEGRELLE |
3 |
FR |
|
NVI |
Vitali NEVSKI |
1 |
BY |
DLC |
Carlo Di LUCCA |
1 |
IT |
|
OKE |
Oliver KLOES |
1 |
DE |
DLR |
Roberto Di LUCCA |
3 |
IT |
|
OSK |
Oddleiv SKILBREI |
1 |
NO |
EBA |
Eric BARBOTIN |
1 |
FR |
|
PAH |
Hilari PALLARES ALBALAT |
7 |
ES |
ENK |
Peter ENKSONATUS |
1 |
DE |
|
PHS |
Paal Henning SCHJØLBERG |
1 |
NO |
FIE |
Agnes FIENGA |
1 |
FR |
|
PTS |
Thormod Sten PALMESEN |
1 |
NO |
FIM |
Marcin FILIPEK |
2 |
PL |
|
RDI |
Sylvain RONDI |
1 |
FR |
FOC |
Mario FERNANDEZ OCANA |
2 |
ES |
|
REB |
Lars BØrge REBBESTAD |
1 |
NO |
FRP |
Eric FRAPPA |
2 |
FR |
|
RSD |
Runar SANDNES |
1 |
NO |
GBH |
BjØrn Haakon GRANSLO |
1 |
NO |
|
RTH |
Wolfgang ROTHE |
8 |
DE |
GCV |
Rui GONCALVES |
3 |
PT |
|
SCB |
Carles SCHNABEL |
9 |
ES |
GJJ |
Jaroslav GRNJA |
1 |
YU |
|
SKO |
Ivica SKOCIK |
1 |
HR |
GRM |
Juan GRADOS MORENO |
1 |
ES |
|
SPS |
Stefano SPOSETTI |
1 |
IT |
HCP |
Claus-Peter HEIDMANN |
1 |
DE |
|
TBU |
Toni BERNAUS |
1 |
ES |
HJP |
Philippe HENAREJOS |
1 |
FR |
|
THO |
Bertrand THOORIS |
3 |
BE |
HKR |
Chris HOOKER |
1 |
UK |
|
THU |
William THUILLOT |
3 |
FR |
HMG |
Hazel McGEE |
1 |
UK |
|
VGC |
Vicent GONZALES CEBRIA |
1 |
ES |
HPT |
Martina HAUPT |
2 |
DE |
|
WHS |
Wolfgang HASSE |
2 |
DE |
HSC |
Chris HILLS |
1 |
UK |
|
WUE |
Nikolai WUENSCHE |
1 |
DE |
HZM |
Michel HERNANDEZ |
1 |
FR |
|
|
|
|
|
Those countries (and numbers of observers) are :
BE = Belgium (1), BY =
Belarus (2), CZ = Czech Republic (1), DE = Germany (11), DK = Denmark (1),
ES = Spain (14), FI = Finland (1), FR = France (11), HR = Croatia (1), IT =
Italy (8), NO = Norway (7),
PL = Poland (2), PT = Portugal (1), UK = United Kingdom (5), YU =
Yugoslavia (1).
The Tercidina event has been treated in a special INFO n°39.
2002 (September to December) Observations
Usually negative, excepted when otherwise specified. ‘mp’ stands for the minor planet, ‘*’ for the star. All times are in UTC.
2002.09.14 : (143) Adria / HIP 31913 JLX JNK MDT
2002.09.14 : (25) Phocaea / TYC 0444-02306-1 SCB
2002.09.17 : (493) Griseldis /TYC 2895-02760-1 BEI (with HCP) DLR (with DLC) MDT OKE (with MSS) SKO
and one perhaps positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
JTC |
N 56 44 48 |
E 08 57 54 |
? m |
22:04:45 ± ? |
? |
JTC observed for less than 1 s , a magnitude drop to ~ 10, whereas (493) magnitude was ~ 15.3
2002.09.19 : (240) Vanadis / TYC 1275-00004-1 THO
2002.09.25 : (342) Endymion / TYC 6266-00766-1 EBA KZA PAH
and one perhaps positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
SCB |
N 41 29 41.5 |
E 01 52 25.7 |
+ 180 m |
18:58:27.7 ± 0.5 s |
18:58:31.1 ± 0.5 s |
|
|
|
|
18:58:37.2 ± 0.5 s |
18:58:48.2 ± 0.5 s |
SCB comments : “ both of them could be caused by air turbulence or by some failure on my eye”. That is probable since the second occultation would require a 150km body, whereas (342) is estimated ~65km only.
2002.09.28 : (302) Clarissa / PPM 144222 JLX
According to D. Dunham, a positive observation was recorded in USA.
2002.09.28 : (713) Luscinia / TYC1316 1900 JLX
2002.10.02 : (241) Germania / TYC1865-01967-1 BOL THU (with FIE)
and one positive:
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
DLR, DDN, NRL |
N 44 21 28 |
E 11 09 13 |
+651 m |
00:17:34.92 ± ? |
00:17:55.12 ± ? |
20.2 s |
2002.10.03 : (25) Phocaea / TYC 0457-00098-1 BOL GCV
and one positive:
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
CNS |
N 41 19 15.2 |
W 01 20 22.4 |
+1050 m |
19:43:06.1 ± 0.2 s |
(19:43:09.4 ± 1 s) |
About 2 s |
CNS comment : “The Reappearance time is not accurate... The given time is that from the stopwatch with no Personal Equation subtracted because it is totally subjective... My estimated duration of the occultation is 2 seconds”.
GCV at Linhaceira N 39 31 22.6 W 08 23 01.5 +90 m
[mp 0.304" ± 0.012" NNE of * at UT 19:42:45.5 ± 1.5 s from 22 CCD images]
2002.10.08 : (2916) Voronveliyia / HIP 17583 BOL DGE JLX KZA
RTH
2002.10.23 : (1112) Polonia / TYC 1183-00030-1 BAO BOL CRM GCV
JLX JNK LAB RTH
SPS THO
and one positive:
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
FRP |
N 45 19 51.6 |
E 04 03 08.2 |
+872 m |
22:48:37.67 ± 0.21 s |
22:48:40.52 ± 0.11 s |
2.85 ± 0.22 s |
Mid-event : 22:48:39.1
GCV at Linhaceira N 39 31 22.6 W 08 23 01.5 +90 m
[mp 0.048" ± 0.050" NNW of * at UT 22:50:35.0 ± 6.5 s from 25 CCD images]
GCV data are in close agreement with J.Manek’s update and FRP positive observation.
2002.10.25 : (407) Arachné / TYC 1926-00284-1 FIM
and three positive:
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
DEN |
N 52 27 31.7 |
E 13 21 11.2 |
+ 78 m |
03:32:38.1 ± 0.4 s |
03:32:40.8 ± 0.3 s |
2.7 ± 0.4 s |
JNK |
N 50 41 32 |
E 14 02 02 |
+ 378 m |
03:32:34.0 ± 0.2 s |
About 1 s |
|
RTH |
N 52 27 44.7 |
E 13 25 23.9 |
+ 66 m |
03:32:37.7 ± 0.7 s |
03:32:41.5 ± 0.7 s |
3.8 ± 1.0 |
DEN and RTH positive observations confirm each other and the initial prediction. JNK blink cannot be due to the main body : it is either spurious, either due to a possible satellite.
2002.10.26 : (407) Arachné / TYC 1926-01282-1 HSC JLX (with THU)
2002.10.26 : (886) Washingtonia / TYC 2471-00409-1 BOL JLX (with THU)
2002.10.27 : (1200) Imperatrix / TYC 1349-00324-1 BOL MDT PAH
2002.10.28 : (209) Dido / TYC 1220-01179-1 BOL
2002.10.29 : (233) Asterope / TYC 1319-00673-1 BOL
2002.11.03 : (431) Nephele / HIP 18735 AHO AND (with HPT) DEN
GBH JTC MDT OSK
PHS PTS RTH WHS
WUE
REB recorded an occultation from Oerstad (N 62 13 E 06 05). Several others positive observations have been done in USA, according to D. Dunham.
2002.11.03 : (680) Genoveva / HIP 49947 - GSC 1974 1031 CNS DEN JNK
MDT RTH
2002.11.04 : (309) Fraternitas / HIP 35494 AND (with HPT) DGE DLR
ENK MDT RTH WHS
2002.11.05 : (962) Aslog / HIP 57757 DGE MDT RTH
This event has been predicted first by Jerome BERTHIER from IMCCE.
2002.11.12 : (612) Veronika / TYC 4814-03182-1 BOL
2002.11.13 : (1049) Gotho / TYC 3359-0341 RSD
2002.11.18 : (844) Leontina / TYC 2361-01655-1 SCB
and one positive:
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
CNS |
N 42 36 14.2 |
W 00 50 35.7 |
+640m |
03 00 08.5 ± 0.3 s |
03 00 10.4 ± 0.2 s |
1.9 s |
Another disappearance has been reported from 02:56:01.5 to 02:59:36.1 but this event is obviously spurious.
2002.11.18 : (1049) Gotho / TYC 3358-00173-1 HKR JHP MDT
2002.11.22 : (1208) Troilus / TYC 3358-02307-1 BOL HJP PAH
2002.11.30 : (301) Bavaria / TYC 4669-00528-1 BOL
2002.12.01 : (845) Naema / TYC 2413-00783 THO
2002.12.02 : (392) Wilhelmina / TYC 0097-00489-1 JHP
2002.12.12 : (845) Naema / TYC 2411-00909-1 FIM MDT
2002.12.15 : (42) Isis / TYC 1861-01129-1 IBV
2002.12.16 : (509) Iolanda / TYC 0111-01109-1 SCB
2002.12.28 : (509) Iolanda / TYC 0110-00178-1 CNS SCB
2002.12.29 : (445) Edna / TYC 2414-00419-1 GJJ LAB
and one perhaps positive:
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
SCB |
N 41 29 41.5 |
E 01 52 25.7 |
+180 m |
23:21:05.9 ± 0.5 s |
23:21:09.9 ± 0.5 s |
4.0 s |
SCB thinks it could be spurious. PE subtracted : 0.3 s
Other observations (not in E.A.O.N. program) :
2002.09.11 : (5458) Aizman / TYC 0575-00860 MDT
2002.09.22 : (5215) Tsurui / HIP 13491 MDT
2002.09.31 : (345) Tercidina / HIP 19499 MDT
2002.10.16 : (3171) Wangshouguan / HIP 15110 AME FOC LAB
LTA (with LTL) LZJ RDI (with HZM) SCB VGC
AME and SCB, LZJ and FOC were in double station.
We received 12 observations by courtesy from Steve Preston : 3 negative ones by Gerry Smerchanski, Dale Ireland and Arthur Lee, 2 uncertain and 7 positive reports :
Observer |
Latitude (N) |
Longitude (W) |
Disapp. UT |
Reapp. UT |
Dur. |
Comments |
John Ritter |
47 43 55.92 |
122 37 52.74 |
|
|
|
Minimal fade - possible single component occultation. |
Harry Colvin |
47 39 44.1 |
122 32 49.80 |
04:35:29 |
|
2.1 s |
UT is probably off - 35:36 instead |
David Warman |
47 41 32.50 |
122 30 30.49 |
04:35:35.6 |
04:35:37.4 |
1.8 s |
|
Dave Runyan |
47 36 39.85 |
122 30 25.57 |
04:35:36.3 |
04:35:39.65 |
3.35 s |
adjust lag on start to 35.5 |
Dale Gombert |
47 34 33 |
122 22 47.00 |
04:35.34.32 |
04:35:39.43 |
5.1 s |
|
Steve Preston |
47 38 20.70 |
122 14 13.2 |
04:35:33.68 |
04:35:38.57 |
4.9 s |
|
John Robbins |
47 28 38.00 |
122 08 46 |
04:35:35 |
|
1 s |
|
Steve Preston |
48 02 57.54 |
122 06 29.22 |
|
|
|
Automatic telescope |
Jon Seamans |
47 43 48 |
122 06 00 |
04:35:40 |
04:35:42 |
2 ? |
start time and/or duration approx |
2002.10.26 : (15874) 1999TL66 / HIP 13530 ASK CNS HMG LZJ
PAH RTH SCB TBU
TBU and SCB were in double station. 1999 TL 66 is a Trans Neptunian Object (TNO).
2002.11.02 : (3330) Gantrisch / TYC 1220-00198 MDT
2002.11.03 : (2578) Saint-Exupery / TYC 1954-01097 MDT
2002.11.04 : (4471) Graculus/ CMC 818096 MDT
2002.11.05 : (3940) Larion/ TYC 4666-00224 MDT
2002.11.18 : (3774) Megumi / TAC +30°919 MDT
2002.11.22 : (269) Justitia / TYC 0681-01015-1 PAH
2002.12.26 : (4100) Sumiko / TAC +9°751 MDT
2002.12.27 : (1466) Mundleria / TYC 175-945 MDT
2002.12.04 : (2378) Pannekoek / TYC 4725-01108-1 FOC
2002.12.08 : (4162) SAF / TYC 1767-00618-1 MDT
2002.12.08 : (23973) 1999CA4 / TYC 2375-00337-1 MDT
2002.12.08 : (5483) Cherkashin / HIP 41875 MDT
2002.12.09 : (148) Gallia / HIP 72096 MDT
2002.12.09 : (2718) Handley / TYC 1884-01174-1 MDT
2002.12.10 : (31819) 1999RS150 / HIP 23556 MDT
2002.12.11 : (1881) Shao / TAC +3°16749 MDT
2002.12.11 : (29555) 1998DP / TAC +16°2005 MDT
2002.12.12 : (2893) Peiroos / TAC +3°1162 MDT
2002.12.18 : (4368) Pillmore/ TYC 6077-01518 MDT
2002.12.21 : (3418) Izvekov / TAC +23°1314 MDT
2002.12.22 : (1765) Wrubel / TYC 2428-00928 MDT
2002.12.31 : (3708) 1974FV1 / TYC 2389-01674-1 PAH
2002.12.31 : (5571) 1978LG / TYC 1367-0161-1 MDT
Special Event:
Following a warning from Bruno Sicardy (Observatory of Paris-Meudon), EAON called to observe Tethys - one of the large Saturn satellites - occulting a Mv 9 star, as it has been done for Titania on 2001. Unfortunately, north-western Europe has been covered by clouds.
2002.12.15 : TETHYS / TYC 1310-02435-1 CAS CNS COF FRP GCV
GRM IZF PAH SCB
We received two positive
reports from Europe (BZY and NVI) and seven positive reports from the
Japanese Occultation Information Network. BZY
recorded the event with a camcorder and observed visually a TV screen. The
visual timing of reappearance was poor, and was eventually deduced from duration
39.95s ± 0.1s , obtained by Janusz Wiland from monitoring the magnetic tape.
Here are the corresponding chords in decreasing longitude order :
Name |
Latitude (N) |
Longitude (E) |
Height |
Disappearance UT |
Reappearance UT |
||
|
|
|
|
begin |
end |
begin |
end |
Akira Yaeza |
36 32 19.22 |
140 37 48.50 |
+20 m |
18:56:51.8 |
18:57:28.1 |
||
Hiromi and Hiroko Hamanowa |
37 27 26.76 |
140 26 00.51 |
+260 m |
18:56:52 |
18:57:31 |
||
Mitsuru Kashiwagura |
38 22 36.9 |
140 08 52.4 |
+182 m |
18:56:54.71 |
18:56:54.78 |
18:57:34.79 |
18:57:34.85 |
Hideo Takashima |
35 50 48.3 |
139 57 10.9 |
+39 m |
18:56:50.65 |
18:57:23.61 |
||
Katsuhiko Kitazaki |
35 42 24.2 |
139 33 51.5 |
+66 m |
18:56:51.59 ± 0.02 s |
18:56:51.62 ± 0.02 s |
18:57:24.63 ± 0.02 s |
|
Eisaku Katayama |
35 41 53 |
139 33 22 |
+62 m |
? |
18:56:52 |
18:57:25 |
? |
Akie Hashimoto |
35 57 53 |
139 02 11 |
+355 m |
? |
18:57:27.79 |
||
Vitali Nevski |
55 03 40 |
30 19 39 |
+180 m |
19:01:25.41 ± 0.1 s |
19:02:05:82 ± 0.1 s |
||
Wojciech Burzynski |
53 17 53.8 |
23 35 42.8 |
+158 m |
19:01:41.0 ± 0.2 s |
19:02:20.95 ± 0.2 s |
A first reduction was made by Tsutomu Hayamizu, then Bruno Sicardy (Observatory of Paris-Meudon) made a more elaborate one. The mean diameter obtained here (1074.4 km) is in agreement with the official size (from IAU) of Tethys as determined by Voyager spacecraft : 1072 X 1056 X 1052 km.
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G. REGHEERE gillesregheere@voila.fr
13 bis rue de l’église
78890 GARANCIERES - France