Solar System
Dynamics
Group 		Impact orbits of
Potentially Hazardous Asteroids


In this page we list all the Potentially Hazardous Asteroids for which we determined the impact orbits compatible with the existing set of observations. Our investigation were performed from the present days till 2100, except some special asteroids as (29075) 1950 DA. We listed also objects classified as PHA's that were analysed by us and any impact orbit were possible to detemine up to 2100.

We can "clone" the impact orbit, compute impact parameters, and can determine a path of the impact locations on the Earth surface (example 2).

In the table given below we indicate the entries to all the asteroids for which we derived impact orbits ( yes button) and to asteroids we have found no impact orbits ( no button).



Object Impact orbit Current status Diameter [m] Other informations
2011 AG5 yes recently observed 100—230 older results
2010 JH110 yes not recently observed 10—30 older results
2010 HP20 yes not recently observed 0—20
2010 FD yes not recently observed 10—40
2010 CR5 yes not recently observed 310—700 older results
2010 CA yes not recently observed 32—73
2009 XO yes not recently observed 230—530 older results
2009 WM1 yes not recently observed 250—560 older results
2009 VA yes not recently observed 0—10
2009 TM8 yes not recently observed 0—10
2009 TH8 yes not recently observed 30—70
2009 TD17 yes not recently observed 0—10
2009 SH1 yes not recently observed 0—10
2009 MG1 yes not recently observed 40—100 older results
2009 KK yes not recently observed 220—490 older results
2009 JF1 yes not recently observed 10—20
2009 FJ yes not recently observed 30—70
2009 BD yes not recently observed 0—10
2009 AV no not recently observed 700—1600 older results
2009 AL no not recently observed 130—290 older results
2008 YU32 no not recently observed 310—700 older results
2008 YF29 yes not recently observed 40—100
2008 YC3 yes not recently observed 20—50 older results
2008 XQ2 no not recently observed 310—700 older results
2008 XC1 yes not recently observed 50—120
2008 WY94 no not recently observed 20—50 older results
2008 WK96 no not recently observed 70—160 older results
2008 UV99 yes not recently observed 360—800
2008 UB7 yes not recently observed 50—110
2008 TE yes not recently observed 0—10
2008 ST7 yes not observable 40—100 older results
2008 OO yes not observable, but possible to recover 350 — 730
2008 JL3 yes not recently observed 20 — 50
2008 ER7 no not recently observed 300 — 670 older results
2008 AF4 yes not observable, but possible to recover 340 — 770
2007 VK184 yes not observable, but possible to recover 110 — 260
2007 RY19 yes not observable, but possible to recover 90 — 210
2006 SU49 = 2001 UV17 no not observable, but possible to recover 360 — 800 older results
2006 SC yes not recently observed 20 — 60
2006 QV89 yes not recently observed 20 — 50
2005 QK76 yes not recently observed 20 — 60
(144898)
2004 VD17 		yes not observable, but possible to recover 320(a) older results
2004 LV3 no not recently observed 500 — 1200
2004 NL8 no not recently observed 1100 — 2600
(99942)Apophis
2004 MN4 		yes not recently observed 270 ± 60(c) older results
2004 FU4 no not recently observed 600 — 1300 older results
(144332) 2004 DV24 no not recently observed 1400 — 3200 older results
2001 WN5 yes recently observed 700 — 1500 older results
2000 WO107 no not recently observed 410 — 920
2000 SG344 yes not recently observed 30 — 70
(101955)
1999 RQ36 		yes not recently observed 200 older results
(137108)
1999 AN10 		no not observable, but possible to recover 800 — 1800 older results
1997 XR2 no not observable, but possible to recover 200 — 460 older results
(35396)
1997 XF11 		no not observable, but possible to recover 1300 — 2800 older results
1994 WR12 yes lost object, but possible to recover 110 — 260
(2340) Hathor yes not recently observed 5300
(29075)
1950 DA 		yes not recently observed 1400(b)
R e f e r e n c e s
(a) De Luise et al. 2007, Icarus 191, 828-635
(b) Binzel, R.P. et al. 2002, in 'Asteroids III' (Eds. W.F.Bottke et al.), Univ.Ariz.Press, Tucson, USA, pp. 255-271. (Physical Properties of NEOs)
(c) Delbò M., Cellino A., and Tedesco E. F., 2007, Icarus, 188, 266





Solar System Dynamics & Planetology Group, 2008. All rights reserved