Ondrejov NEO Photometric Program |
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(Now updated frequently!)
New page on binary NEAs has been added. This composite lightcurve of 2001 OE84, a large superfast rotating monolithic Amor asteroid is an example of data resulted from the Near-Earth Object Photometric Program conducted at the Ondrejov Observatory . Main tasks of the NEO project are:
People involved:
Petr Pravec, Marek Wolf,
Lenka Sarounova,
Peter Kusnirak, and Mirek Velen.
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The following NEAs have been photometrized from Ondrejov. The (p) or (l) symbol means that a period or a constraint on it, respectively, has been derived (or confirmed) for a particular object using our data. If you are interested in a particular object, please contact Petr Pravec.
A table with unpublished periods and amplitudes derived using our NEA observations is available. The list is considered as a "pre-publication" of our results so that they could be added to the list of Lightcurve Parameters compiled by Alan Harris. We recommend to contact us if you are interested in a particular object.
Apollos and Atens (q < 1 AU) |
Amors (q > 1 AU) |
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(1620) Geographos (p) [3] (1863) Antinous (p) + (1864) Daedalus (p) [2] + (1865) Cerberus (p) + (1866) Sisyphus (p) + (2063) Bacchus (p) [11] (2100) Ra-Shalom (p) [11] + (2102) Tantalus (p) [7] (2201) Oljato (2212) Hephaistos (l) [7] (3103) Eger (p) [11] + (3200) Phaethon (p) [11] (3671) Dionysus (p) [8] + (3752) Camillo (p) [11] (3838) Epona (p) + (4179) Toutatis (l) [1] (4183) Cuno (p) + (4197) 1982 TA (p) [14] (4341) Poseidon (p) [11] (5131) 1990 BG (5143) Heracles [11] (5645) 1990 SP (l) + (5786) Talos (l) + (5836) 1993 MF (p) + (6037) 1988 EG (l) + (6455) 1992 HE (l) + (6611) 1993 VW [2] (7092) Cadmus (7341) 1991 VK (p) [11] (7482) 1994 PC1 (p) [11] (7822) 1991 CS (p) [11] (7889) 1994 LX (p) [4] + (8176) 1991 WA (p) + (8201) 1994 AH2 (l) [4] + (10115) 1992 SK (p) + (11500) 1989 UR (p) + (12711) 1991 BB (p) + (12923) 1999 GK4 (p) + (20429) 1998 YN1 (p) + (23187) 2000 PN9 (p) + (31669) 1999 JT6 (p) + (33342) 1998 WT24 (p) + (35107) 1991 VH (p) [10]             1950 DA (p) +             1989 UQ (p) [11]             1989 VA (p) [7]             1992 CC1 (p) [11]             1992 QN (p) [11]             1993 UC (p) [4]             1994 CB (p) [4]             1994 RC             1996 FG3 (p) [12] [15]             1997 BQ             1997 BR (p) [11]             1997 GL3 (l) [11]             1997 UR             1997 US9 (l) +             1997 WU22 (p) +             1998 BZ7 (p) +             1998 KY26 (p) [9] [13]             1998 MT24 (p) +             1998 QR52 (p) +             1998 RO1 (l) +             1998 ST27             1998 SF36 (l) +             1998 UO1             1998 XS16 (p) +             1999 CV3 (p) +             1999 FA (p) +             1999 GJ4 (p) +             1999 HF1 (p) [19] +             1999 JD6 (p) +             1999 JM8 (l) +             1999 KV4             1999 KW4 (p) [22] +             1999 NC43 (l) +             1999 SM5 (p) +             1999 TY2 (p) [16]             2000 DP107 (p) +             2000 EX106 (p) +             2000 GU127 (l) +             2000 GK137 (p) +             2000 JG5 (p) +             2000 NM (p) +             2000 PH5 (p) +             2000 RM12             2000 UG11 +             2000 UV13 (l) +             2000 XG47 (p) +             2000 XK47             2000 YA (p) +             2001 CB21 (p) +             2001 CC21 (p) +             2001 CP36 +             2001 JM1 (p) +             2001 KA67 +             2001 OG108 (l) +             2001 SL9 (p) [21] +             2001 WG2             2001 YP3             2002 AA (p) +             2002 AL14 (l) +             2002 BK25 +             2002 DH2             2002 FD6 +             2002 JB9 (p) +             2002 JR9 (p) +             2002 LV (p) +             2002 LB6 |
(719) Albert (p) + (1627) Ivar (p) [4] + (1916) Boreas (p) + (1943) Anteros (p) [7] [11] (1951) Lick (p) + (1980) Tezcatlipoca (p) [18] (3102) Krok + (3122) Florence (p) [11] + (3199) Nefertiti (p) [7] + (3352) McAuliffe (l) + (3691) 1982 FT (p) [11] (3908) Nyx (p) [18] (4055) Magellan (p) + (4954) Eric (p) [2] (4957) Brucemurray (p) [4] [11] (5407) 1992 AX (p) [15] (5587) 1990 SB (p) [11] + (5653) 1992 WD5 + (5751) Zao (l) [7] + (6050) 1992 AE (p) + (6053) 1993 BW3 (p) [6] (6178) 1986 DA + (6318) 1990 WA (6322) 1991 CQ (p) [7] (6489) Golevka (6569) 1993 MO (p) [4] (7025) 1993 QA (p) [11] (7336) 1989 RS1 (7358) 1995 YA3 (l) + (7474) 1992 TC (p) [7] (7480) 1994 PC (p) [11] (7977) 1977 QQ5 (p) + (8034) 1992 LR (l) [11] (11054) 1991 FA (p) + (11398) 1998 YP11 (p) + (14402) 1991 DB (p) + (18109) 2000 NG11 (p) + (18172) 2000 QL7 (19764) 2000 NF5 (l) + (20790) 2000 SE45 (l) + (26760) 2001 KP41 (p) + (31345) 1998 PG (p) [15] (38071) 1999 GU3 (p) [17] +             1994 AW1 (p) [2] [5]             1994 GY (p) [2]             1994 JF1 [2]             1994 LW             1994 QC (l) +             1995 FX (l) [11]             1997 GH3 (p) [11]             1997 LY4 (p) [14]             1997 SE5 (p) [11]             1998 FX2 (p) +             1998 FM5 (p) +             1998 QR15 (l) +             1999 CW7 (p) +             1999 GJ2             1999 JO8 (p) +             1999 LF6 (l) +             1999 LN28             1999 ND43             1999 ML             1999 PJ1 (p) +             1999 RH27 (p) +             1999 TA10 (l)             1999 TX16 (p) +             1999 VN6 (l) +             1999 VM40 (p) +             2000 JQ66 (p) +             2000 LC16 (p) +             2000 OG8 (p) +             2000 QW7 +             2000 QN130 +             2000 RD53 (p) +             2000 SS164 (p) +             2001 MF1 (p) +             2001 PD1 (l) +             2001 OE84 (p) [20] +             2001 SK162 (p) +             2001 SE286 (l) +             2001 VS78 (p) +             2001 XN254 |
"+" means that we have useful unpublished data (there maybe also a paper in preparation)
Some (old) images obtained with our instrument:
  Fragmented periodic comet Machholz 2
  (1620) Geographos changing brightness
For questions about the NEO research at the Ondrejov Observatory please contact:
ppravec@asu.cas.cz Astronomical Institute AS CR