The list shows possible double stars, with separations less than 2", predicted to be occulted by the Moon during February 2012 and visible from parts of Australia or New Zealand. The listing is a very abbreviated version of predictions produced by Occult plus an indication of the region of visibility. Observers need to generate their own precise predictions using Occult.
Observations of all pairs in the list are highly desirable. Those showing an OCc number have been reported as non-instantaneous at a lunar occultation. Confirmation or otherwise of any double nature is wanted.
The list below is generated by OCCULT for a 25cm telescope. Some of the events may be beyond the reach of smaller telescopes.
Please send reports of all observations of these stars to Brian Loader at palbrl@clear.net.nz, including any made in earlier months and not so far reported. And of course if you observe a stepped event for a star, which is not a known double, please report this. More details about reporting follow the predictions.
Lunar Occultations of Close Double Stars in February 2012 for Australia and NZ.
The list shows possible double stars with separations < 2" predicted to be occulted by the Moon during February and visible from parts of Australia or New Zealand. The listing is a very abbreviated version of predictions produced by Occult plus an indication of the region of visibility. Observers need to generate their own precise predictions using Occult.
The list below is generated by OCCULT for a 25cm telescope. Some of the events could be beyond the reach of smaller telescopes.
Observations of all pairs in the list are highly desirable. Those showing an OCc number have been reported as non-instantaneous at a lunar occultation. Confirmation or otherwise of any double nature is wanted.
d P Star Mag % Double details WDS or Area of
Feb No v ill magnitudes sepn PA? OCC # Visibility
2 d 630# 7.7 70+ : AB 8.26 8.45 0.59" 80.5 STF 520 ,AkW
2 d 76595 8.0 71+ : AB 8.71 8.87 0.07" 263.4 BU 1235 ABCHMRS
2 D 664 5.5 72+ : ** 6.2 6.2 0.05" 350.0 OCc 309 AHMP
3 d 77019 7.9 79+ : ** 8.6 8.6 0.05" 351.8 OCc 866 ,Ak
4 d 77981 9.1 86+ : ** 9.8 9.8 0.10" 121.0 OCc 655 ,AkW
4 D 946 3.5 87+ : AB 3.5 6.2 1.6" 253.3 BU 1008 AHMP
R 946: sec star is X 85102
4 d 78024 9.1 87+ : ** 10.0 10.0 0.05" 350.0 OCc1296 BR,AkChW
4 d 78103 9.4 87+ : AB 9.5 10.9 1.4" 135.4 COU 273 R
4 d 78156 9.3 87+ : AB 9.1 9.2 0.30" 39.7 COU 274 APR
4 d X 8800 8.5 88+ : AB 9.04 10.21 1.71" 50.1 AG 323 P
5 D 1077 4.0 93+ : ** 4.5 4.5 0.10" 90.0 OCc 293 B,AkChIW
5 d 96610# 8.1 94+ : AB 8.23 10.10 0.62" 65.1 COU 925 BCS
5 d 96739 8.4 94+ : ** 9.1 9.1 0.05" 350.0 OCc1351 P
6 d 97419 8.8 97+ : AB 8.90 11.14 0.50" 279.0 HDS1133 ,W
8 r 117991 9.4 99- : AB 9.4 9.5 1.6" 43.3 AG 170 ACMS
9 r 1564# 6.7 97- : AB 6.92 8.45 0.60" 247.5 A 2768 ABCHMR,AkChIW
10 r 138347 8.7 90- : AB 9.06 10.49 1.41" 297.8 A 1356 BCRS,AkChIW
10 r 138426 8.8 89- : AB 9.6 9.6 0.40" 272.0 TDS8048 P
11 R 1809! 7.0 82- : ** 7.5 8.1 0.01" 122.8 OCc1673 ABCHMRS,AkChI
11 r 138890 8.9 82- : ** 9.3 9.3 0.10" 313.0 OCc 428 P
11 R 1815 4.7 82- : ** 4.8 8.8 0.10" 214.0 OCc 760 P
12 R 1949# 5.9 72- : AB 6.30 7.29 0.42" 62.2 BU 932 ABCHMPRS
12 r 158101! 9.5 71- : ** 10.1 10.3 0.04" 106.1 OCc1659 P
13 r 158586 8.9 62- : ** 10.0 10.0 0.05" 350.0 OCc1462 ABCHMRS,AkChIW
13 r 158607 9.5 61- : ** 9.8 9.8 0.05" 350.0 OCc1463 ACHMS,ChIW
14 r 183552 10.1 49- : AB 10.7 11.1 0.23" 223.2 B 2358 ABCHMRS
16 r X 42308 8.7 29- : AB 8.8 9.3 0.69" 170.0 HDL 133 ,AkChIW
X 42308: sec star is X141848
16 r 185355 9.0 29- : AB 9.15 11.21 0.10" 205.0 HDS2456 ,AkChIW
16 r X 42464 8.9 28- : AB 9.2 11.0 0.44" 219.6 RST3107 ACHM,ChI
16 R 2535* 6.3 27- : AB 6.60 8.04 0.10" 18.0 HDS2492 P
17 R 2666 4.9 19- : AB 5.03 7.43 1.47" 272.8 JC 6 ,AkChIW
R2666: sec star is X156529
17 R 187040 7.5 18- : AB 7.52 10.56 1.32" 166.1 HO 567 AP
S187040: sec star is X158664
18 r 2828 5.8 12- : ** 3.7 6.7 0.02" 106.0 OCc 994 ,ChW
18 r X 45992 9.8 11- : AB 9.9 10.3 1.8" 200.8 HDL 35 ,AkChIW
X 45992: sec star is X176589
19 R 163460 8.5 5- : ** 9.4 10.3 0.06" 125.0 OCc 440 ,ChIW
19 R 2968 6.1 5- : Ba,Bb 6.16 9.14 0.49" 62.6 BAR 12 ,AkChIW
19 R 2969 3.1 5- : Aa,Ab 3.1 4.9 0.10" 209.4 BLA 7 ,AkChIW
R2969: B star is R 2968 (206" 266.9)
19 r 163551 8.4 5- : ** 9.8 9.8 0.10" 89.0 OCc 920 ABCHMRS
19 R 163569 9.2 5- : AB 10.0 10.0 0.31" 56.3 RST4065 BR
19 R 163563 8.6 5- : ** 9.6 10.2 0.09" 190.5 OCc 402 ABCRS
25 d 102 8.8 11+ : ** 9.6 9.6 0.10" 82.0 OCc 833 BRS
28 d 75809 9.2 35+ : ** 9.6 9.6 0.10" 214.0 OCc 898 AM
29 d X 68409 10.1 43+ : AB 10.7 11.0 0.50" 128.0 TDS2715 R
29 D 601 5.9 44+ : Aa,Ab 6.0 0.52" 281.9 CHR 158 ABCHMRS
======================================================================
Visibility codes:
Australia: A Adelaide, B Brisbane, C Canberra, H Hobart, M Melbourne, P Perth, R Rockhampton, S Sydney
NZ (following a ,) Ak Auckland, W Wellington, Ch Christchurch, I Invercargill.
----------------------------------------------------------------------
Stars with previous occultation observations:
!: Recent video discoveries, confirmation needed. (DD disappearance, RD reappearance)
R1809, 2009 May 6 NZ, DD. S158101, 2006 Jul 5 USA, DD.
#: observations indicating double (DD disappearance, RD reappearance)
R630, 2011 Mar 11 Greece, DD; 2011 Apr 8 USA, DD. R 946, 2011 Nov 14 NZ, RD
R1564, 2009 Aug 31 USAx4 DD 2+ve, 1-ve, 1 doubtful, DD; 2010 Jul 15 Ausx2, 1+ve, 1-ve, DD; 20111 Nov 19 Aus -ve RD
R1949, 2004 Mar 7 NZ, RD.
*: Observations not showing double
R2535, 2011 Oct 30 Aus, DD.
Further observations of all the above are needed
==================================================================
The most convenient way of reporting is to use Dave Herald's new version of OCCULT which has a Double Star report option in the Observations editor. Before using it, generate a light curve with Limovie and copy to the clip board. Your graph will then be attached to the email which you can then send to palbrl@clear.net.nz.
Otherwise in reporting please include your name and positional data as for other occultations reports, also your telescope type and method of observing and timekeeping.
For each event give the star name and the times of each step of the event with the corresponding accuracy. The limb PA, Rv and Cct of the event would also be useful.
In addition to measures of the PA and separation of binary stars, there is also a need for an estimate of the magnitude difference. An estimate of this can be made from the step sizes shown by Limovie data. So if possible a determination should be made of the size of each step together with an estimate of accuracy.
Please also report cases where a double event is predicted but none detected. These are especially likely with stars shown with an OCc designation
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