Asteroid Impact Risk List
| Object | Torino | Cumulative odds | Palermo | Window | Diameter |
|---|---|---|---|---|---|
29075 29075 |
0 | 1 in 2,653 | -0.93 | 2880-2880 | 1.3 km |
Bennu 101955 |
0 | 1 in 1,749 | -1.40 | 2178-2290 | 490 m |
2008 JL3 2008 JL3 |
0 | 1 in 6,031 | -2.38 | 2027-2122 | 29 m |
1979 XB 1979 XB |
0 | 1 in 1,174,376 | -2.69 | 2056-2113 | 660 m |
2000 SG344 2000 SG344 |
0 | 1 in 365 | -2.77 | 2069-2122 | 37 m |
2010 RF12 2010 RF12 |
0 | 1 in 10 | -2.97 | 2095-2122 | 7 m |
2007 FT3 2007 FT3 |
0 | 1 in 1,291,265 | -3.06 | 2030-2119 | 341 m |
2005 QK76 2005 QK76 |
0 | 1 in 14,175 | -3.10 | 2030-2059 | 31 m |
2022 PX1 2022 PX1 |
0 | 1 in 309,502 | -3.10 | 2040-2040 | 120 m |
2021 GX9 2021 GX9 |
0 | 1 in 12,162 | -3.18 | 2032-2052 | 29 m |
2023 DO 2023 DO |
0 | 1 in 2,198 | -3.55 | 2057-2092 | 26 m |
620100 620100 |
0 | 1 in 130,276 | -3.57 | 2124-2124 | 180 m |
2019 VB37 2019 VB37 |
0 | 1 in 17,550 | -3.59 | 2049-2067 | 43 m |
2013 TP4 2013 TP4 |
0 | 1 in 28,361 | -3.60 | 2026-2026 | 11 m |
2008 UB7 2008 UB7 |
0 | 1 in 29,547 | -3.61 | 2044-2101 | 58 m |
2023 BZ 2023 BZ |
0 | 1 in 26,192 | -3.62 | 2026-2026 | 16 m |
2024 JW16 2024 JW16 |
0 | 1 in 431,803 | -3.63 | 2082-2121 | 220 m |
2024 TK5 2024 TK5 |
0 | 1 in 2,988 | -3.63 | 2028-2028 | 10 m |
2007 DX40 2007 DX40 |
0 | 1 in 12,892 | -3.64 | 2035-2122 | 40 m |
2016 YM4 2016 YM4 |
0 | 1 in 74,738 | -3.69 | 2121-2121 | 110 m |
2000 SB45 2000 SB45 |
0 | 1 in 6,310 | -3.71 | 2067-2118 | 46 m |
2026 CQ4 2026 CQ4 |
0 | 1 in 199 | -3.72 | 2072-2125 | 10 m |
2007 KE4 2007 KE4 |
0 | 1 in 50,976 | -3.76 | 2029-2096 | 31 m |
2008 EX5 2008 EX5 |
0 | 1 in 18,792 | -3.77 | 2056-2093 | 59 m |
2025 DT2 2025 DT2 |
0 | 1 in 2,258 | -3.77 | 2044-2071 | 16 m |
2026 MT1 2026 MT1 |
0 | 1 in 443,722 | -3.79 | 2030-2119 | 180 m |
2020 VV 2020 VV |
0 | 1 in 431 | -3.81 | 2044-2122 | 12 m |
2020 VW 2020 VW |
0 | 1 in 142 | -3.81 | 2074-2079 | 7 m |
2018 DQ 2018 DQ |
0 | 1 in 4,650 | -3.82 | 2027-2121 | 5 m |
2017 WT28 2017 WT28 |
0 | 1 in 87 | -3.83 | 2083-2121 | 8 m |
2012 HG2 2012 HG2 |
0 | 1 in 504 | -3.83 | 2052-2122 | 14 m |
2013 VW13 2013 VW13 |
0 | 1 in 2,277 | -3.85 | 2063-2095 | 19 m |
2010 ER12 2010 ER12 |
0 | 1 in 751,032,670 | -3.86 | 2026-2094 | 1.0 km |
2006 DM63 2006 DM63 |
0 | 1 in 7,032 | -3.89 | 2031-2122 | 15 m |
2023 VD3 2023 VD3 |
0 | 1 in 6,705 | -3.90 | 2034-2042 | 13 m |
2021 GE2 2021 GE2 |
0 | 1 in 1,368 | -3.91 | 2030-2030 | 5 m |
2023 SN8 2023 SN8 |
0 | 1 in 11,630 | -3.93 | 2026-2123 | 9 m |
2008 CC71 2008 CC71 |
0 | 1 in 24,653 | -3.98 | 2034-2082 | 36 m |
2020 UL3 2020 UL3 |
0 | 1 in 28,942 | -3.98 | 2122-2124 | 75 m |
2021 EU 2021 EU |
0 | 1 in 18,336 | -4.01 | 2056-2123 | 28 m |
A handful of asteroids are kept on a long-term monitoring list because their orbits aren’t yet pinned down tightly enough to rule out a very distant future approach. The table above shows the most significant, ranked by the Palermo scale — a measure that compares an object’s risk to the natural background chance of a similar impact over the same period. A negative Palermo value means the risk is below that background level, and almost every object here sits well below zero with a Torino rating of 0 (no hazard).
None of these is a prediction of impact. The odds shown are cumulative across many possible dates spread over decades or centuries, so the chance on any single date is far smaller. As telescopes gather more observations, objects are steadily removed — Apophis and 2024 YR4 are two recent examples that were taken off the list entirely. See the close-approach calendar for objects passing soon.