"ROTATIONAL PERIODS AND PEAK TO VALLEY AMPLITUDES OF THE ROTATIONAL LIGHT CURVES OF COMETS" --------------------------------------------------------- Ignacio Ferrín, Center for Fundamental Physics, University of the Andes, Mérida, Venezuela, ferrin@ula.ve Introduction. ============= In this document you will find what we believe is the most complete compilation of rotational periods and peak to valley amplitudes (APTV) of the rotational light curves of comets. You are welcome to use this data set which has been written in ASCII format for your convenience, so that it can be transported easily. However we request, in accord with scientific principles, to give proper credit to this work: Ferrín, I., "Secular Light Curve of Comets, II: 133P/Elst-Pizzarro, an Asteroidal Belt Comet", 2006, ICARUS, in press. Updated regularly at the web site: http://www.webdelprofesor.ula.ve/ciencias/ferrin A preliminary analysis of this data has already been carried out (above reference) with the following result: there is a correlation of rotational periods and diameters that may be evidence of rotational evolution. An histogram of number vs rotational period, allows the determination of a rotational error for snapshot observations, of ±0.63 magnitudes. The histogram is available elsewhere in this web page. Please contribute to this effort by making corrections and additions, or by sending new data. Updates ============ 051126 Schleicher et al. 1998. 051205 Snodgrass et al. 2005. 060304 Toth and Lisse, 2006. 060812 Weissman et al., 1999. 061103 Manzini et al., 2006. 061103 Snodgrass et al. 2006 in press 061105 Jorda & Lecacheux (IAUC 5664) 070117 Boehnhardt et al. (2002) 070214 Lowry and Weissman (2007) 070408 Wasserman et al. (1995) 070408 Larson&Hergenrother (1995) 070409 Schleicher and Osip (2002) Table 1 ======= ROTATIONAL PERIODS AND PEAK TO VALLEY AMPLITUDES OF THE ROTATIONAL LIGHT CURVES OF COMETS. ====================================================================== COMET PROT[hr] APTV[mag] REFERENCES ====================================================================== 001P/Halley* 53.96 1.1 Belton et al. (1986) 177.6 ---- Millis and Schleicher (1986) 52.8 ---- Sagdeev et al. (1989) 177.6 ---- Sagdeev et al. (1989) ----- 0.81 Meech et al. (1986) 002P/Encke* 15.08 0.62 Luu and Jewitt (1990) 14.95 0.88 Jewitt and Meech (1987) 15.21 >0.7 Fernandez et al. (2000) 11.01 0.27 Lowry et al. (2003) 11.083 0.25 Lowry and Weissman (2007) 004P/Faye ----- 0.51 Lamy and Toth, (1995) 006P/D'Arrest 7.20 0.18 Lowry and Weissman (2003) ----- 1.1 Wasserman et al. (1995) 007P/Pons-Winnecke 8.2 ---- Sekanina, (1989) 008P/Tuttle ----- >0.2 Licandro et al. (2000) 009P/Tempel 1 40.7 0.3 Meech et al. (2000) 41.85 0.7 Belton et al. (2005) ----- 0.34 Lamy et al. (2001) 14-39 ---- Weissman et al. (1999) 010P/Temple 2 8.9 ---- Jewitt and Meech, (1988) 8.93 0.67 Sekanina (1991) 8.95 0.75 Jewitt and Luu (1989) 8.9 0.6 A'Hearn et al. (1989) 8.94 0.62 Mueller and Ferrin (1996) 014P/Pons-Winnecke 7.53 0.29 Snodgrass et al. (2005) 017P/Holmes 7.2 0.28 Snodgrass et al. (2006) 8.6 0.28 Snodgrass et al. (2006) 10.3 0.28 Snodgrass et al. (2006) 12.8 0.33 Snodgrass et al. (2006) 019P/Borelly 25.0 0.95 Lamy et al., (1998) 26.0 1.0 Mueller, Samarasinha(2002) 021P/Giacobini- ----- 0.4 Mueller (1991) Zinner 9.5 ---- Leibowitz and Brosch, (1986) 022P/Kopff 12.30 0.55 Lowry and Weissman (2003) 023P/Brorsen-Metcalf 13.5-15.0 ---- Watanabe and Nakamura,(1990) 30-40 ---- Watanabe and Nakamura,(1990) 026P/Grigg-Skjellerup ----- >0.3 Licandro et al. (2000) 028P/Neujmin 1 12.67 0.5 Jewitt and Meech (1988) ----- 0.71 Campins et al. (1987) 12.6 0.42 Wisniewski et al. (1986) 12.7 0.56 Mueller and Heinrichs (2002) 12.75 0.45 Delahodde et al. (2001) 029P/SW 1 14/32 ---- Meech et al. (1993) 5.0 ---- Whipple (1980) >1440. ---- Stansberry et al. (2004) 6. ---- Jewitt (1990) 10. 0.50 Luu and Jewitt, (1993) 030P/Reinmuth 1 ----- 0.7 Scotti(IAUC6072) 031P/SW2 5.58 0.53 Luu and Jewitt, 1992 ======================================================================== Table 1. (Continued) ROTATIONAL PERIODS AND PEAK TO VALLEY AMPLITUDES OF THE ROTATIONAL LIGHT CURVES OF COMETS. ====================================================================== Comet PROT [hr] AROT[mag] REFERENCES ====================================================================== 036P/Whipple 3.5 ---- Snodgrass et al. (2005) 037P/Forbes ----- >0.5 Licandro et al. (2000) 041P/Tuttle-Giacobini- ----- 0.7 Larson&Hergenrother (1995) Kresak 044P/Reinmuth 2 ----- 1.3 Scotti (1993) 046P/Wirtanen 7.6 >0.09 Meech et al. (1997) 6.0 0.22 Lamy et al., (1998) 6-7.5 0.15 Boehnhardt et al. (2002) 047P/Ashbrook-Jackson 11.2 0.26 Snodgrass et al. (2006) 15.5 0.25 Snodgrass et al. (2006) 21.6 0.38 Snodgrass et al. (2006) 44.0 1.35 Snodgrass et al. (2006) 048P/Johnson 29.00 0.32 Jewitt and Sheppard (2004) 049P/Arend-Rigaux 6.78 0.38 Jewitt and Meech (1985) ----- 0.55 Vedeer et al, (1987) 13.47 0.72 Millis et al. (1988) 13.6 0.53 Wisniewski et al. (1986) 055P/Tempel-Tuttle 15.31 0.76 Hainaut et al. (1998) 14.79 ---- Jorda et al. (1998) 065P/Gunn ----- >0.3 Licandro et al. (2000) 067P/Churyumov- 12.3 ---- Lamy et al. (2003a) Gerasimenko ----- >0.61 Mueller (1991) 073P/S-W 3 ----- 0.57 Boehnhardt et al. (1999) 074P/Smirnova-Chernykh ----- >0.3 Licandro et al. (2000) 081P/Wild 2 ----- 0.55 Ferrin (2005) 082P/Gehrels 3 ----- >0.6 Licandro et al. (2000) 092P/Sanguin 6.22 0.40 Snodgrass et al. (2005) 095P/2060 Chiron 5.92 0.05 Campins et al. (1994) 096P/Machholz 1 6.38 0.3 Lamy et al. (2003b) 097P/Metcalf-Brewington ----- >0.7 Licandro et al. (2000) 098P/Takamizawa ----- >0.6 Licandro et al. (2000) 103P/Hartley 2 ----- >0.1 Licandro et al. (2000) 107P/Wilson-Harrington 6.1 0.21 Osip et al. (1995) 109P/Swift-Tuttle 69.36 ---- Yoshida et al, (1993) 67.5 ---- Fomenkova et al. (1995) 66.5 ---- Sekanina, (1981) 69.6 ---- Jorda&Lecacheux(IAUC5664) 110P/Hartley 3 10 ---- Lamy et al. (2003b) 126P/IRAS 4.9 ---- Groussin et al. (2004) 133P/Elst-Pizarro 3.47 0.39 Hsieh et al. (2004) 137P/Shoemaker-Levy 2 ----- >0.4 Licandro et al. (2000) 143p/Kowal-Mrkos 17.2 ---- Lamy et al. (2003b) 147P/Kushida-Muramatsu 9.5 ---- Lamy et al. (2003b) P/Levy 1991 XI 8.34 0.35 Fitzsimmons, Williams (1994) C/1995 O1 Hale-Bopp 11.23 ---- Ortiz and Rodriguez (1999) 11.47 ---- Lecacheux et al. (1997) 11.35 ---- Jorda et al. (1999) 11.31 ---- Schleicher et al. (1998) Levy 1990 XX 17.0 ---- Feldman et al. (1992) 18.9 ---- Magdziarz et al. (1995) 37.8 ---- Schleicher et al. (1991) 24 ---- Fulle et al. (1992) ======================================================================== Table 1. (Continued) ROTATIONAL PERIODS AND PEAK TO VALLEY AMPLITUDES. ====================================================================== Comet PROT [hr] AROT[mag] REFERENCES ====================================================================== Alcock 1963b 24 ---- UR Whipple-Fedtke- 540 ---- Bobrovnikoff (1945) Tevzadze 1942g Bennett 1970 II 35 ---- Larson and Minton (1973) Hyakutake 1996B2 6.30 ---- Lisse et al., (1999) 6.274 ---- Schleicher and Osip (2002) Burnham 1960 II 94 ---- UR Austin 1982g 84 ---- UR Comet 1744 115.2 ---- Pansechi and Fulle (1991) Brooks 1893 IV 91 ---- Vorontsov-Velyaminov, (1930) West 1976 VI 48 ---- Sekanina and Farrel, (1978) Mrkos 1957 V 19.7 ---- Sekanina and Farrel, (1982) Iras-Araki-Alcock 83VII 51 ---- Sekanina, (1988) Bakharew-Macfarlane- 474 1.1 Ferrin (2002) Krienke 1996 PW 35.44 0.44 Davies et al. (1998) C/1999 S4 LINEAR 5.2 ---- Toth and Lisse (2006) C/2001 OG 108 LONEOS 57.19 0.3 Abell et al. (2003) C/2001 Q4 NEAT 23.2 ---- Lecacheux and Frappa (2004) C/2002 V1 NEAT 60 ---- Navarro and Riquelme (2003) C/2002 C1 Ikeya-Zhang 35.5 ---- Manzini et al. (2006) C/2004 Q2 Machholz 9.1 ---- Sastri&Vasundhara(IAUC8480) C/2004 F4 Bradfield 12 ---- Sekanina (IAUC8326) ======================================================================= *1P/Halley and 2P/Encke exhibit complex rotation (two periods). Statistics: 4.9 h<Prot<540 h, Prot = 39.98±82.60 h (91 observations) 0.05<ptv-Amplitude < 1.3 magnitudes, ptv-Amplitudes = 0.52±0.26 (58 observations). UR= Unpublished Result, Ferrín (2006). Totals: 72 comets, 94 rotational periods, 71 peak-to-valley rotational amplitudes, 90 references. ======================================================================= REFERENCES. Abell, P.A., and 10 other colleagues, 2003. Physical Characteristics of Asteroid-Like Comet Nucleus C/2001 OG108 LONEOS. 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