Dear Observers, For the upcoming lunation, we have as many as five return binaries and a few other interesting targets for the BinAstPhotSurvey and the NEOSource project. Of very high importance is the NEA binary 1996 FG3 for which just one event detection (possibly just one night) in this apparition could give a unique model for detecting BYORP; it would be the first such case. Then there are many other interesting targets for all of us :-) Enjoy! This list of targets is also available at http://www.asu.cas.cz/~asteroid/binastphotsurvey_neosource_targets20111225.txt Clear Skies, Petr Pravec Object V Dec Elo Mot Bga H q a Arc Hrev P Ampl U 0. Worked objects: (1573) Vaisala 15.5 -8 108v 0.2 -67 12.2 1.82 2.37 22opp Slow rotator, worked from Modra. (2195) Tengstrom 14.8 21 155^ 0.2 24 12.1 1.99 2.22 22opp Return prime suspect, worked by Don Pray. (2870) Haupt 16.2 6 111v 0.3 -56 12.7 1.89 2.39 16opp Slow rotator, worked by Julian Oey. (3665) Fitzgerald 16.7 4 143v 0.2 -35 13.4 2.20 2.42 17opp Return prime suspect, worked by Jim Brinsfield and Don P. (4826) Wilhelms 16.0 8 151v 0.3 -27 12.3 1.92 2.38 15opp Worked by David Higgins. (24475) 2000 VN2 14.4 30^ 133v 1.4 -27 16.1 1.10 1.97 6opp Long period or low amplitude; suitable as a supplementary target. 1. Returning binaries (2121) Sevastopol 16.7 12 130^ 0.1 42 12.4 1.79 2.18 22opp D_2/D_1 = 0.41, P_orb = 37.12 h, 2nd apparition (3749) Balam 16.0 19 145^ 0.1 33 13.4 1.99 2.24 18opp "Quadruple" system. NEOSource project. (4607) Seilandfarm 15.4 22 178^ 0.3 3 13.0 2.22 2.26 14opp D_2/D_1 = 0.30, P_orb = 31.65 h, 2nd apparition (6265) 1985 TW3 16.7 28 161^ 0.3 21 13.4 1.75 2.17 16opp D_2/D_1 = 0.32, P_orb = 15.86 h, 3rd apparition (175706) 1996 FG3 15.6f 29 171v 0.9 -1r 18.2 0.69 1.05 8opp BYORP target - NEOSource project. 2. Paired asteroids (errors <=0.03 mag needed): (17430) 1989 KF 16.8 31 150^ 0.2 32 12.2 2.58 2.85 12opp Suitable as a supplementary target - only a semi-dense coverage needed. 3. YORP objects (errors <=0.05 mag needed) - NEOSource project: (1620) Geographos 16.8 53 150 0.5 13a 15.6 0.83 1.25 27opp P = 5.22 h, one lightcurve per lunation sufficient. 4. Mini-family members (errors <=0.05 mag needed) - NEOSource project: (6825) Irvine 16.8 27 144^ 0.1 37 13.6 2.13 2.17 16opp P = 3.75 h, one lightcurve per lunation sufficient. (14627) Emilkowalski 16.7 42 133^ 0.2 49 13.1 2.21 2.60 9opp P ~ 11.13 h, one lightcurve per lunation sufficient. Suitable as a supplementary target, for its longish period. 5. Returning "prime suspects", to be followed up on their 2nd (3rd, ...) apparitions (1344) Caubeta 15.6 29 162^ 0.2 20 12.8 1.98 2.25 21opp 12.8 3.1220 0.21 3 (16233) 2000 FA12 16.2 20 142^ 0.1 36 12.2 2.30 2.61 10opp 12.2 3.1811 0.17 3 (138524) 2000 OJ8 16.2 -4 128^ 0.2 28 16.6 1.02 2.36 6opp 16.6 2.6835 0.06 2 6. New targets (6529) Rhoads 15.9 9 151^ 0.2 18 13.3 2.04 2.35 15opp (16432) 1988 VL2 16.3 6 147^ 0.2 19 13.2 2.19 2.42 15opp Note: The ephemerides were computed for 2011-12-25 ^/v means that the value increases/decreases by more than 0.05 mag/day (for V) or by more than 0.5 deg/day for Dec and Elong. The rate of apparent motion (Mot) is in deg/day. Bga is the galactic latitude. Compact listing: (1573) (2195) (2870) (3665) (4826) (24475) (2121) (3749) (4607) (6265) (175706) (17430) (1620) (6825) (14627) (1344) (16233) (138524) (6529) (16432)