Catalogue of the Solar System Small Bodies Orbital Evolution

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Asteroids Approaches Archive

Object
Period
#
AsteroidHDateObjectr, AU  r, kmRisk
10821
2000 BD19 (137924)17.4904/23/2088 00:00:00 AMSun0.09255313 845 7720.85
10822
2000 BD19 (137924)17.4909/30/2049 00:00:00 AMSun0.09255413 845 8360.85
10823
2000 BD19 (137924)17.4905/16/1882 00:00:00 AMSun0.09255513 846 1040.85
10824
2004 UL (374158)18.6409/30/1923 00:00:00 AMSun0.09256013 846 7090.60
10825
2004 UL (374158)18.6401/15/1851 00:00:00 AMSun0.09256113 846 8810.60
10826
2000 BD19 (137924)17.4903/26/2093 00:00:00 AMSun0.09256413 847 3200.85
10827
2004 UL (374158)18.6411/07/1806 00:00:00 AMSun0.09258513 850 4720.60
10828
2004 UL (374158)18.6409/12/1876 00:00:00 AMSun0.09259313 851 6900.60
10829
2000 BD19 (137924)17.4902/26/2098 00:00:00 AMSun0.09259913 852 6790.85
10830
2000 BD19 (137924)17.4906/09/2037 00:00:00 AMSun0.09261113 854 4470.85
10831
2004 UL (374158)18.6410/24/1960 00:00:00 AMSun0.09262013 855 7120.60
10832
2004 UL (374158)18.6411/26/1987 00:00:00 AMSun0.09262713 856 7710.60
10833
2000 BD19 (137924)17.4909/11/2095 00:00:00 AMSun0.09263413 857 8660.85
10834
2000 BD19 (137924)17.4902/16/2121 00:00:00 AMSun0.09264113 858 9010.85
10835
2016 GU224.0504/15/1850 00:00:00 AMSun0.09264413 859 3620.12
10836
2004 UL (374158)18.6407/23/1946 00:00:00 AMSun0.09264513 859 4410.60
10837
2017 TC120.7812/22/2116 00:00:00 AMSun0.09264513 859 4660.32
10838
2000 BD19 (137924)17.4907/17/2073 00:00:00 AMSun0.09265313 860 6400.85
10839
2017 TC120.7804/30/1892 00:00:00 AMSun0.09266713 862 7280.32
10840
2000 BD19 (137924)17.4901/26/1870 00:00:00 AMSun0.09267113 863 4260.85
1 ... 423 ... 508 ... 529 ... 535 ... 538 539 540 541 542 543 544 545 546 547 ... 551 ... 563 ... 605
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The table contains the archive of approaches of asteroids with major planets and the Moon at a distance less than 0.01 astronomical units and with the Sun at a distance less than 0.1 astronomical units, defined by calculations with use of equations of motion, considering gravitational, non-gravitational forces, relativistic effects, effects of planets nonsphericity. This method was used in calculations with use of input data from 12/13/2017 and more earlier.

This project was supported by the Federal Agency of Education (project codes RNP 2.1.1.1689, RNP 2.1.1.745).
Samara State Technical University
Applied Mathematics and Information Science Department
Яндекс.Метрика