|
EAON - INFO N° 522005, November and December |
123 observations have been performed during 2005, November and December ( 18 positive or possibly positive) about 62 events ( 9 positive or possibly positive) by 69 observers, from the 12 following countries (and numbers of observers) :
BE = Belgium ( 5 ), CH = Switzerland ( 3 ), CZ = Czech Republic ( 3 ), DE = Germany (10 ), ES = Spain ( 6 ), FR = France ( 23 ), IT = Italy (2 ), NL = The Netherlands ( 3 ), PL = Poland (1), PT = Portugal (1), SK = Slovakia ( 2 ), UK = United Kingdom ( 8 ).
You will find in the table hereafter the list of the observers abbreviations in alphabetical order, with the number of observations made by each of them.
ACH |
Apostolos CHRISTOU with A. MORAGHAN |
1 |
UK |
|
JNK |
Tomas JANIK |
1 |
CZ |
|
JPR |
Jean Paul ROUSSELLE |
1 |
FR |
||||
BCL |
Philippe BERNASCOLLE |
3 |
FR |
|
JVA |
Jean VILAR |
1 |
FR |
BOL |
Simone BOLZONI |
2 |
IT |
|
KID |
Marc KIDGER |
1 |
ES |
BLM |
Lex BLOMMERS |
1 |
NL |
|
KWK |
Silvia KOWOLLIK with Helmut C. BAUER |
1 |
DE |
BRD |
Emmanuel BROCHARD |
1 |
FR |
|
||||
BTG |
Rene BOURTEMBOURG |
1 |
BE |
|
LAQ |
Pierre LAQUES |
1 |
FR |
CHR |
Bernard CHRISTOPHE with Thierry MIDAVAINE (MID) |
1 |
FR |
|
LCP |
Laurent CORP |
1 |
FR |
|
MAA |
Andrea MANNA |
1 |
CH |
||||
CNS |
Oscar CANALES MORENO |
2 |
ES |
|
MBU |
Michel BOUTET with Jacques SANCHEZ (JSZ) |
1 |
FR |
COF |
Francois COLAS with Jean LECACHEUX (JLX) |
1 |
FR |
|
1 |
|||
1 |
|
MJL |
Jose Luis MARCO LARRIBA |
2 |
ES |
|||
CQU |
Jean CAQUEL |
1 |
FR |
|
MUM |
Michel MEUNIER |
1 |
FR |
DMK |
Roger DYMOCK |
2 |
UK |
|
PAW |
Thierry PAUWELS with Peter de Cat |
1 |
BE |
DNZ |
Helmut DENZAU |
6 |
DE |
|
||||
DPY |
Michel DUPOUY with Vincent WISNIEWSKI |
1 |
FR |
|
PCI |
Paolo CORELLI |
2 |
IT |
|
PSY |
Raymond PONCY |
2 |
FR |
||||
EBA |
Eric BARBOTIN |
2 |
FR |
|
RTH |
Wolfgang ROTHE |
2 |
DE |
EEA |
Andreas EBERLE with Larry POORMAN |
1 |
DE |
|
RWD |
Chris ROWLAND |
1 |
UK |
|
RYF |
Francisco REYES |
1 |
ES |
||||
ELL |
Andrew ELLIOTT |
2 |
UK |
|
SAU |
Christof SAUTER |
1 |
CH |
FAR |
Otto FARAGO with Gunter WOYSCH |
1 |
DE |
|
SMD |
Libor SMID |
1 |
CZ |
|
SMI |
Michael SCHMIDT |
1 |
DE |
||||
FAU |
Gerard FAURE |
1 |
FR |
|
SPS |
Stefano SPOSETTI |
3 |
CH |
FBG |
Juan FABREGAT |
1 |
ES |
|
SPU |
Klaus SPRUCK |
1 |
DE |
FIM |
Marcin FILIPEK |
1 |
PL |
|
STP |
Roger STAPLETON |
1 |
UK |
FLJ |
John Mac FARLAND |
1 |
UK |
|
SUB |
Robert SOUBIE |
1 |
FR |
FRP |
Eric FRAPPA |
1 |
FR |
|
TCH |
Pascale TORTECH |
1 |
FR |
GCV |
Rui GONCALVES |
1 |
PT |
|
THO |
Bertrand THOORIS |
2 |
BE |
GRS |
Christian GROS |
3 |
FR |
|
trt |
TAROT (see below) |
|
FR |
HAL |
Karel HALIR |
1 |
CZ |
|
VIJ |
Josef VILAGI with Stefan GADJOS (GJD) |
1 |
SK |
HRU |
Harrie G. J. RUTTEN |
3 |
NL |
|
||||
JDO |
Jose Luis DORESTE |
1 |
ES |
|
VNB |
Fernand VANDENBULCKE |
1 |
BE |
JGS |
Malcolm JENNINGS |
2 |
UK |
|
WKL |
Jan Martin WINKEL |
2 |
NL |
JLX |
Jean LECACHEUX with Francois COLAS (COF) |
2 |
FR |
|
|
|
|
|
1 |
|
|
|
|
|
TAROT (Acronym for “Télescope à Action Rapide pour les Objets Transitoires”) is an automatic telescope, located at Calern Observatory, dedicated to g-rays bursts optical study; when available, it can be used for various survey programs.
2005 (November and December) Observations
Observations are usually visual and negative, excepted when otherwise specified. All times are in UTC.
2005.11.01 : (67) Asia / 2UCAC 36051757 FIM GRS HRU SPU
and one possibly positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
WKL |
N 51 54 16 |
E 06 15 41 |
+20 m |
22:01:57.8 ±0.4 s |
? |
GRS was in the S. Preston’ updated predicted path.
WKL : possible blink at the predicted time; if related with (67) Asia, this observation should imply either a wide shift of the asteroid (at least 5 path widths) or the presence of a secondary body.
2005.11.02 : (1755) Lorbach / HIP 92370 PCI
PCI : CCD drift-scan
2005.11.05 : (3) Juno / TYC 0114-01163-1 CHR with MID
CHR : CCD drift-scan. It is a peculiar event as Juno (mag 7.9) is brighter than the star (mag 11.7). CHR was situated at the eastern predicted path border. The recording shows only strong fluctuation during about 6 sec at the predicted event time. Therefore no definite conclusion can be drawn.
2005.11.08 : (5485) Kaula / TYC 0027-00395-1 RTH
RTH : videorecording
2005.11.08 : (1032) Pafuri / HIP 48303 HRU PAW with P. De CAT
PAW: CCD drift-scan
2005.11.10 : (71) Niobe / TYC 0836-01199-1 THO
and one positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
DNZ |
N 54 20 34 |
E 10 33 06 |
+40 m |
05:42: 30.5 ±0.12 s |
05:42:33.7 ±0.12 s |
3.2 ±0.4 s |
THO : three events (1) 05:39:58:44 to 05:40:07.15, (2) 05:41:43.38 to 05:41:53.2, (3) 05:42:09.3 to 05:42:35.4, probably due to clouds, the third including the predicted appulse time.
DNZ : videorecording; DNZ was nearly on the centreline, since he observed an event with a duration close to the max predicted value (3.7 s.); the path has been shifted by 1.5 time its width, toward N-E.
2005.11.11 : (5749) 1991FV / 2UCAC 36467374 PCI
PCI : CCD drift scan; very short light drop (0.8-0.9 s approx) has been recorded between 02:22:01.00 – 02:22:01.09 whose nature still remains unclear (noise or true secondary occultation?)
2005.11.18 : (128) Nemesis / TYC 1412-00199-1
Two positive observations, one of them from Canada :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
JLX |
N 48 48 17.9 |
E 02 13 48.3 |
+168 m |
06:14:55.22 ±0.15 s |
06:15:05.8 ±0.15 s |
11.6 ±0.4 s |
E. BRIGGS |
N 43 46 22 |
W 79 23 19 |
+180 m |
06:09:50.4 ± ? s |
06:10:01.6 ± ? s |
11.2 ± ? s |
JLX : Blink at 06:14:36.2 ±0.3 s.
Both observers were predicted to be close to the centreline, what effectively occurred, since they observed an event with a duration close to the max predicted value (11.8 s, corresponding to the assumed 188 km diameter for (128) Nemesis )
2005.11.19 : (1994) Shane / TYC 1218-00868-1 CQU DPY with V. WISNIEWSKI FRP GRS HAL LCP MAA MBU SAU SMD SPS TCH
DPY, SPS : CCD drift-scan; FRP, SMD : videorecording
CQU : blink at 23:11:13.3; TCH : possible short blink at 23:12:08.3 (No PE taken into account). Both events occurred several minutes before the expected appulse time, so they are probably not related to the (1994) Shane event.
FRP and GRS were both in the S. Preston updated predicted path. There must have been a significant shift of the shadow path, but the lack of positive observation lets its position remaining unknown.
2005.11.28 : (210) Isabella / HIP 22711 RYF
2005.11.29 : (1999) Hirayama / HIP 50501 CNS
CNS : videorecording
2005.12.01 : (1247) Memoria / 2UCAC 36230768 HRU JLX RTH trt
and one positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
DNZ |
N 54 20 34 |
E 10 33 06 |
+40 m |
17:24:03.7 ±0.16 s |
17:24:05.6 ±0.16 s |
1.9 ±0.3 s |
DNZ : videorecording; his positive observation shows a path shifted by three times its width, toward NW
2005.12.02 : (405) Thia / HIP 37521 (NZ Gem) JNK
JNK : videorecording
2005.12.07 : (2222) Lermontov / 2UCAC 39657553 SPS trt
SPS : CCD drift-scan
2005.12.09 : (1113) Katja / TYC 5233-01086-1 DNZ
DNZ : videorecording
2005.12.09 : (723) Hammonia / HIP 39809 BTG trt
2005.12.10 : (4054) Turnov / TYC 1945-00865-1 JGS trt
JGS : videorecording
2005.12.11 : (1833) Shmakova / TYC 0257-00720-1 DMK
2005.12.11 : (524) Fidelio / TYC 2380-00914-1 BCL PSY
and three positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
CNS |
N 4150 15.23 |
W 00 44 43.81 |
+330 m |
23:23:06.03 ± 0.03 s |
23:23:11.47 ±0.03 s |
5.44 ±0.3 s |
MJL |
N 41 50 15.2 |
W 00 44 43.7 |
+332 m |
23:23:06.54 ± ? s |
23:23:11.63 ± ? s |
5.09 ± ? s |
GCV |
N 39 31 22.6 |
W 08 23 01.5 |
+90 m |
23:24:16.60 ±0.16 |
23:24:23.26 ±0.16 |
6.66 ±0.22s |
CNS : videorecording; GCV, PSY : CCD drift scan; MJL : no PE taken into account
The positive observations and the negative BCL one (who was in the predicted path, close to its northern border) show the real path has been slightly shifted toward South, and/or the shape of (524) Fidelio is irregular.
2005.12.12 : (121) Hermione / TYC 4974-01069-1 COF EBA GRS LAQ MUM STP SUB
and seven positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
ACH |
N 54 21 11 |
W 06 38 59 |
+70 m |
06:05:59.69 ±0.5 s |
06:06:06.37 ±0.1 s |
±0.3 s |
EEA |
N 48 49 09.88 |
E 09 00 19.42 |
+420 m |
06:06:20.005 ±0.02 s |
06:06:25.765 ±0.02 s |
5.76 ±0.02 s |
ELL |
N 53 44 25.6 |
W 02 54 25.4 |
+14 m |
06:06:04.75 ±0.02 s |
06:06:10.35 ±0.02 s |
5.60 ± ?s |
FAR |
N 48 46 56.64 |
E 09 11 47.12 |
403 m |
06:06:20.4 ±0.2 s |
06:06:26.4 ±0.2 s |
6.0 ±0.2 s |
KWK |
N 48 46 56.73 |
E 09 11 47.35 |
+401 m |
06:06:20.32 ±0.01 s |
06:06:26.12 ±0.01 s |
2.85 ±0.22 s |
FLJ |
N 54 21 11.0 |
W 06 38 59.5 |
+70 m |
06:06:01.0 ±0.4 s |
- |
|
JVA |
N 48 38 50 |
E 07 42 50 |
+135 m |
06:06:15.45 |
06:06:20.33 |
4.88 |
ACH : with A. Moraghan, in double station with FLJ; EEA was with L. Poorman
EBA: CCD drift-scan; ELL, STP, SUB : drift scan; FAR (with G. Woysch), KWK (with H. Bauer) : videorecording, both in double station; JVA : possible 0.15 s flash, 4.35 s after D
Despite scattering, positive observations can be fitted with an elliptical profile with main axis about 200 X 220 km.
Hermione has a satellite called S/2002 (121) 1 La Fayette. Its predicted track run mainly over south of France. No occultation has been observed in relation with this small body (30 km).
2005.12.12 : (3274) Maillen / TYC 1852-01760-1 VIJ with GJD
2005.12.12 : (2372) Proskurin / 2UCAC 39828784 DNZ
DNZ : videorecording
2005.12.17 : (294) Felicia / TYC 4962-00486-1 PSY trt
PSY : CCD drift scan
The TAROT observatory was in the predicted path. This negative observation shows the real path has been shifted but the lack of positive observation lets its real position remaining unknown.
2005.12.18 : (3311) Podobed / 2UCAC 39642472
Only one positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
DNZ |
N 54 20 34 |
E 10 33 06 |
+40 m |
05:15:28.74 ±0.16 s |
05:15:28.90 ±0.16 s |
0.16 ±0.04 s |
DNZ : videorecording
2005.12.19 : (397) Vienna / TYC 0634-00772-1 BLM BOL DMK JGS JPR
RWD SMI SPS THO VNB WKL
BOL : partial, due to clouds; SPS : CDD drift scan
Unfortunately, there was no station in the predicted path.
2005.12.22 : (684) Hildburg / TYC 2438-01021-1 BOL
2005.12.23 : (389) Industria / TYC 5228-00818-1 BCL FAU MJL
and one positive :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
MBU |
N 43 16 28.3 |
E 01 13 40.0 |
+310 m |
19:10:55.72 ±0.06 s |
19:10:57.54 ±0.06 s |
1.82 ±0.05 s |
MBU and JSZ observed an event with duration in agreement with their position in the predicted path and the max predicted duration ( 2.6 s). MJL was close to the southern border of the predicted path.
2005.12.26 : (4298) 1941WA / TYC 1879-00055-1 DNZ
DNZ : videorecording
2005.12.26 : (1101) Clematis / HIP 32338 BCL BRD
2005.12.27 : (661) Cloelia / TYC 0610-01401-1 EBA
EBA was in the predicted path; his negative observation shows the real one has been shifted but the lack of positive observation lets it remaining unknown.
2005.12.27 : (134) Sophrosyne / TYC 2949-00549-1
Only one positive observation :
Abbr |
Latitude |
Longitude |
Height |
Disappearance UT |
Reappearance UT |
Duration |
ELL |
N 53 44 25.6 |
W 02 54 25.4 |
+14 m |
22:27:31.18 ±0.02 s |
22:27:36.38 ±0.02 s |
5.20 ±0.02 s |
ELL : videorecording
ELL was close to the northern border of the predicted path but observed an event with long duration (nearly half of the max predicted one : 12.6 s). Due to the lack of any other
observation, no conclusion can be drawn. Note that the shape of (134) Sophrosyne is not circular (what is shown by the reduction of the 1980/11/24 event registered in the
Winoccult[1] database ). Besides, the event occurred nearly 15 s sooner than the predicted appulse time.
2005.12.31 : (20000) Varuna / 2UCAC 40675770 JDO JLX with COF FBG KID
20000 Varuna is a Trans Neptunian Object. Assuming a 900 km diameter, the probability of positive occultation deduced from the last update by Steve Preston, varies in Europe, from 13.5 % for Gibraltar (on the centre line) to 11.0 % for Bergen (Norway); in America, probability is lower (Chicago : 10.4 %, Los Angeles : 7.1% ). With a 1200 km diameter, the probabilities are enhanced by a factor close to 4/3.
The star is very faint : R ~ 15.1, so large telescopes or long integrations were required. A 40 ±5 sec duration was expected.
M. Vasseur observing from Canada registered a one minute long event between 06:18 and 06:19 UTC from his location (N 45 28 50.2 W 75 42 09). Due to the lack of any other observation, no conclusion can be drawn.
FBG : CCD imaging, no occultation longer than 10 s; JLX, videorecording : no occultation longer than 4 s
The 30 following events have been observed by TAROT only – all with negative results :
2005/11/08 : ( 9601 ) 1991 UE3 : ( TYC 1877-00600-1 2005/11/15 : ( 9306 ) Pittosporum / 2UCAC 39311854
2005/11/17 : ( 3961 ) Arthurcox / TYC 1750-00204-1 2005/11/18 : ( 12662 ) 1978 CK / TYC 2466-01419-1
2005/11/20 : ( 605 ) Juvisia / TYC 3398-02431-1 2005/11/21 : ( 12561 ) Howard / TYC 1880-00073-1
2005/11/23 : ( 1368 ) Numidia / 2UCAC 46280551 2005/11/23 : ( 11 ) Parthenope / TYC 1300-00570-1
2005/11/23 : ( 1490 ) Limpopo / HIP 113977 2005/11/26 : ( 565 ) Marbachia / TYC 5203-01230-1
2005/11/28 : ( 4119 ) Miles / TYC 6404-00623-1 2005/11/28 : ( 1401 ) Lavonne / TYC 1860-00090-1
2005/11/30 : ( 3980 ) Hviezdoslav / TYC 1279-01228-1 2005/11/30 : ( 1407 ) Lindelof / 2UCAC 40813639
2005/12/01 : ( 5883 ) 1993 VM5 / TYC 2936-00839-1 2005/12/03 : ( 4452 ) Ullacharles / TYC 1168-01570-1
2005/12/03 : ( 1235 ) Schorria / TYC 4032-00950-1 2005/12/03 : ( 2163 ) Korczak / 2UCAC 39453323
2005/12/04 : ( 35347 ) 1997 JN12 / 2UCAC 42919904 2005/12/04 : ( 5021 ) Krylania / HIP 36307
2005/12/06 : ( 552 ) Sigelinde / TYC 1863-00525-1 2005/12/07 : ( 1420 ) Radcliffe / TYC 1383-00535-1
2005/12/07 : ( 3193 ) Elliot / TYC 2408-01654-1 2005/12/08 : ( 7494 ) Xiwanggongchen / 2UCAC 41330288
2005/12/10 : ( 2436 ) Hatshepsut / TYC 0585-00735-1 2005/12/16 : ( 10837 ) 1994 EJ1 / TYC 5308-01320-1
2005/12/18 : ( 913 ) Otila / TYC 1896-00312-1 2005/12/21 : ( 4402 ) Tsunemori / 2UCAC 35560592
2005/12/21 : ( 1368 ) Numidia / TYC 3392-00950-1 2005/12/21 : (1889) Pakhmutova / TYC 2488-01116-1
It is necessary to send a report even if there has been no occultation from your place (negative observation). These negative observations can sometimes be of as great interest as positive ones : they can be decisive to determine the exact position of the shadow path (see for instance in this info, the case of BCL and (524) Fidelio, during the 2005/12/11 event).
Please DON’T FORGET to use the IAU format YYYYMMDD for the date of your reports. When one finds a report with date 04/01/06 , must he have to compute a prediction for the six possible dates before finding the correct one ? Thanks for him.
Clear skies for all.
G. REGHEERE gillesregheere@yahoo.fr
96 rue de Mercantour
78310 Maurepas - FRANCE
[1] WINOCCULT is a software developed by D. HERALD, dedicated amongst others, to prediction of asteroidal occultation and reduction of observations.