T3: finding comet in the asteroid population
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1 Vienn, 2006 My T3: finding comet in the steroid popultion Luc Buzzi 1, Cludio Cremschini 2, Sergio Fogli 3, Ginni Glli 3,4, Ginluc Msi 5, Mur Tombelli 6 1 Schiprelli Observtory 2 Bssno Brescino 3 Suno 4 Gig Observtory 5 Università di Rom Tor Vergt 6 Montelupo Motivtion Severl objects discovered s steroids hd cometry fetures: 2002 EX P (NEAT) 2004 TU P (Siding Spring) 2004 YJ 35 C/2004 YJ 35 (LINEAR) 2005 JQ 5 P/2005 JQ 5 (Ctlin) 2005 YQ 127 P/2005 YQ 127 (LINEAR) 2006 CK 10 C/2006 CK 10 (Ctlin) 1
2 2004 TU 12 Ner Erth Asteroid 2004 Nov 12 (Msi et l., MPC I05) P/2002 EX 12 = 169P (NEAT) Ner Erth Asteroid 2005 Aug 3 (Fogli, Glli, MPC 147) 2
3 2005 JQ 5 Ner Erth Asteroid 2005 My 14 (Fogli, Glli, MPC 147) P/2005 JQ 5 (Ctlin) 2005 My 27 (Fogli, Glli, MPC 147) 6C3D486 = 2006 CK Feb 4 (Buzzi, MPC 204) C/2006 CK10 (Ctlin) 2006 Apr 7 (Fogli, Glli, MPC 147) 3
4 Trget Selection Levison s comet txonomy is bsed on the Tissernd prmeter respect to Jupiter (T) T = Tissernd prmeter respect to Jupiter J T = + 2 J 2 ( 1 e ) cos(i) J e i semi-mjor xis Jupiter s semi-mjor xis eccentricity inclintion 4
5 dot = steroid circle = comet 5
6 Minor bodies with T < 3 re under the Jupiter s grvittionl influence nd probbly they should be cometry nuclei of the Jupiter Fmily Comet clss. T should be the discriminnt prmeter for trget selections to find comets in the steroid popultion. Observing Progrm To find comets in the steroid popultion we suggest n observing progrm clled T3 (Tissernd 3) to observe ll steroids with T < 3. Most of the surveys do not check their imges to find the possible cometry feture of detected minor bodies tht re usully clssified s steroids. Further observtions would be useful to confirm physiclly the dynmicl behviour of the minor body. 6
7 Frequently n e-mil messge is sent to interested observers nd it contins the observtions oppurtunities with the following conditions: mgnitude limit 20.0 elongtion from Sun >= Minor Plnet Design code Tper Tj Opp e i R.A. Decl. Delt r Mg Elong. no nme yyyy mm hh mm.mm dd pp.p A.U. A.U. V dd Hidlgo E 2000 DQ110 K00DB0Q E A computer progrm written by S. Fogli extrct dt from the MPCORB.DAT file of the Minor Plnet Center. L. Buzzi is the coordintor of the messge lert nd obtined results re distributed to observers. Observtionl s Technique Whenever the cometry behviour is not obvious, i.e. no til nd no com re visible in the imges, FWHM prmeter of the trget is compred to those of severl strs with similr mgnitude. In order to hve secure SNR we usully obtin severl imges of the trget tht re dded using the well known Trck & Stck method of Astrometric computer progrm. To mesure FWHM of the trget stcked imge is obtined with the motion vector of the minor body, while to obtin FWHM of strs the sme imge is restcked using 0.0 motion vector. If cometry behviour is found, other observers will be dvised s soon s possible in ny wy (phone or emil), n indipendent confirmtion is well cknoledged by Minor Plnet Center. It is good to obtin further confirmtion by professionls nd we ve strted outstnding collbortions with severl stronomers. 7
8 Obtined Results Negtive Observtions: (52872) Okyrhoe Positive Observtions: 2005 SB 216 If you re interested in the T3 observing progrm plese contct Luc Buzzi Web service will be vilble s soon s possible t the following URL: 8
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