Compiled at 2359 UTC on 30 September 2008
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Missing something? Here are 99942 Apophis (2004 MN4) and 144898 2004 VD17. Check the archives for others.
| 0000NNN000 Object | Risk Monitor | A/CC Noted Time & Day UTC | 0000T0000 Year Range | VI # | 000NN00 Prob Cum | T0000 PS Cum | T0000 PS Max | T S | Notes for Latest Risk Assessments |
| 2008 SH148 | NEODyS | 1516 Sept. 30 | 2011-2087 | 66 | 4.42e-07 | -6.72 | -7.53 | 0 | Based on 11 optical observations (of which 0 are rejected as outliers) from 2008/09/29.190 to 2008/09/29.292. |
| JPL Sentry | 0215 Sept. 30 | 2011-2107 | 189 | 1.0e-06 | -6.43 | -7.12 | 0 | Analysis based on 11 observations spanning .10211 days (2008-Sep-29.18897 to 2008-Sep-29.29108). Diameter approximately 0.020 km. from mean, weighted H=26.1. | |
| Assessment postings were noted by A/CC on 30 Sept. - References: MPEC 2008-S91 | |||||||||
| 2008 SE85 | NEODyS | 1515 Sept. 30 | 2011-2090 | 103 | 1.96e-07 | -3.02 | -3.27 | 0 | Based on 20 optical observations (of which 0 are rejected as outliers) from 2008/09/28.449 to 2008/09/29.408. |
| JPL Sentry | 1515 Sept. 30 | 2013-2107 | 39 | 6.5e-08 | -3.72 | -3.78 | 0 | Analysis based on 20 observations spanning .95911 days (2008-Sep-28.44782 to 2008-Sep-29.40693). Diameter approximately 0.390 km. from mean, weighted H=19.7. | |
| Assessment postings were noted by A/CC on 29 Sept. & 30 Sept. - References: MPECs 2008-S89 & 2008-S93 | |||||||||
| 2008 SJ82 | NEODyS | 1456 Sept. 28 | 2088 | 1 | 7.46e-09 | -6.36 | -6.36 | 0 | Based on 15 optical observations (of which 0 are rejected as outliers) from 2008/09/26.748 to 2008/09/27.783. |
| JPL Sentry | 1456 Sept. 28 | 2088-2096 | 4 | 3.2e-08 | -5.67 | -6.07 | 0 | Analysis based on 15 observations spanning 1.0351 days (2008-Sep-26.74755 to 2008-Sep-27.7827). Diameter approximately 0.240 km. from mean, weighted H=20.8. | |
| Assessment postings were noted by A/CC on 27 Sept. & 28 Sept. - References: MPECs 2008-S80 & 2008-S83 | |||||||||
| 2008 SH82 | NEODyS | 1515 Sept. 30 | 2032-2088 | 14 | 2.0e-07 | -4.85 | -5.40 | 0 | Based on 18 optical observations (of which 0 are rejected as outliers) from 2008/09/26.214 to 2008/09/29.261. |
| JPL Sentry | 2111 Sept. 29 | 2032-2106 | 29 | 3.0e-07 | -4.66 | -5.26 | 0 | Analysis based on 18 observations spanning 3.0472 days (2008-Sep-26.21299 to 2008-Sep-29.26018). Diameter approximately 0.215 km. from mean, weighted H=21.0. | |
| Assessment postings were noted by A/CC on 28 Sept., 29 Sept. & 30 Sept. - References: MPECs 2008-S79, 2008-S83 & 2008-S93 | |||||||||
| 2008 SV11 | NEODyS | 2249 Sept. 30 | 2034-2089 | 13 | 9.07e-08 | -3.41 | -3.67 | 0 | Based on 44 optical observations (of which 0 are rejected as outliers) from 2008/09/25.263 to 2008/09/30.378. |
| JPL Sentry | 2116 Sept. 30 | 2009-2085 | 11 | 1.4e-07 | -3.00 | -3.33 | 0 | Analysis based on 44 observations spanning 5.1147 days (2008-Sep-25.26245 to 2008-Sep-30.37718). Diameter approximately 0.756 km. from mean, weighted H=18.3. | |
| Assessment postings were noted by A/CC on 26 Sept., 27 Sept., 29 Sept. & 30 Sept. - References: MPECs 2008-S65, 2008-S85 & 2008-S93 | |||||||||
| 2008 ST7 | NEODyS | 1515 Sept. 30 | 2050-2089 | 9 | 4.18e-06 | -5.08 | -5.41 | 0 | Based on 51 optical observations (of which 6 are rejected as outliers) from 2008/09/24.301 to 2008/09/29.327. |
| JPL Sentry | 1515 Sept. 30 | 2073-2102 | 47 | 2.7e-05 | -4.37 | -5.10 | 0 | Analysis based on 48 observations spanning 5.0264 days (2008-Sep-24.29993 to 2008-Sep-29.32635). Diameter approximately 0.053 km. from mean, weighted H=24.0. | |
| Assessment postings were noted by A/CC on 25 Sept., 26 Sept., 27 Sept., 29 Sept. & 30 Sept. - References: MPECs 2008-S56, 2008-S69, 2008-S85 & 2008-S93 | |||||||||
| 2008 ST | NEODyS | 1445 Sept. 27 | 2047-2082 | 12 | 2.9e-05 | -5.91 | -6.07 | 0 | Based on 31 optical observations (of which 0 are rejected as outliers) from 2008/09/22.162 to 2008/09/26.045. |
| JPL Sentry | 1445 Sept. 27 | 2047-2108 | 24 | 6.9e-05 | -5.62 | -6.05 | 0 | Analysis based on 31 observations spanning 3.8835 days (2008-Sep-22.16113 to 2008-Sep-26.04466). Diameter approximately 0.013 km. from mean, weighted H=27.1. | |
| Assessment postings were noted by A/CC on 22 Sept., 23 Sept., 25 Sept. & 27 Sept. - References: MPECs 2008-S33, 2008-S36, 2008-S51 & 2008-S69 | |||||||||
| 2008 KN11 | NEODyS | 1931 Sept. 30 | 2046 | 1 | 2.32e-07 | -5.62 | -5.62 | 0 | Based on 132 optical observations (of which 0 are rejected as outliers) from 2008/05/30.335 to 2008/06/21.154. |
| Assessment postings were noted by A/CC on 22 Sept. & 30 Sept. - References: no MPECs | |||||||||
| 2006 CD | JPL Sentry | 1759 Sept. 17 | 2015-2094 | 58 | 3.1e-08 | -5.30 | -5.97 | 0 | Analysis based on 12 observations spanning 1.9971 days (2006-Feb-01.1555 to 2006-Feb-03.15263). Diameter approximately 0.213 km. from mean, weighted H=21.0. |
| An assessment posting was noted by A/CC on 17 Sept. - References: no recent MPECs | |||||||||
| C L E A R E D | |||||||||
| 2008 SU1 | JPL Sentry | 1514 Sept. 25 | R E M O V E D | Risk listing removed at 0852 UTC 25 Sept. | |||||
| NEODyS | 1514 Sept. 25 | R E M O V E D | |||||||
| Assessment postings were noted by A/CC on 24 Sept. & 25 Sept. - References: MPECs 2008-S42, 2008-S51, 2008-S63, 2008-S69 & 2008-S85 | |||||||||
| 2008 SR | JPL Sentry | 1353 Sept. 23 | R E M O V E D | Risk listing removed at 0849 UTC 23 Sept. | |||||
| Assessment postings were noted by A/CC on 22 Sept. & 23 Sept. - References: MPECs 2008-S31, 2008-S36, 2008-S45 & 2008-S63 | |||||||||
| 2008 SO | JPL Sentry | 1353 Sept. 23 | R E M O V E D | Risk listing removed at 0849 UTC 23 Sept. | |||||
| Assessment postings were noted by A/CC on 22 Sept. & 23 Sept. - References: MPECs 2008-S28, 2008-S36, 2008-S45, 2008-S51, 2008-S69 & 2008-S93 | |||||||||
| 2008 RM98 | NEODyS | 1445 Sept. 27 | R E M O V E D | ||||||
| JPL Sentry | 1445 Sept. 27 | R E M O V E D | Risk listing removed at 0851 UTC 27 Sept. | ||||||
| Assessment postings were noted by A/CC on 26 Sept. & 27 Sept. - References: MPECs 2008-S61 & 2008-S69 | |||||||||
| 2008 RJ1 | NEODyS | 1702 Sept. 10 | R E M O V E D | ||||||
| JPL Sentry | 1702 Sept. 10 | R E M O V E D | Risk listing removed at 0849 UTC 10 Sept. | ||||||
| Assessment postings were noted by A/CC on 5 Sept., 6 Sept., 7 Sept. & 10 Sept. - References: MPECs 2008-R28, 2008-R32, 2008-R55, 2008-R61, 2008-S13, 2008-S19, 2008-S20, 2008-S45, 2008-S63 & 2008-S93 | |||||||||
| 2008 RH1 | NEODyS | 1627 Sept. 7 | R E M O V E D | ||||||
| Assessment postings were noted by A/CC on 6 Sept. & 7 Sept. - References: MPECs 2008-R27, 2008-R32, 2008-R35, 2008-R64, 2008-S03, 2008-S12, 2008-S13, 2008-S45, 2008-S51, 2008-S63, 2008-S85 & 2008-S93 | |||||||||
| 2008 RG1 | NEODyS | 1627 Sept. 7 | R E M O V E D | ||||||
| JPL Sentry | 1627 Sept. 7 | R E M O V E D | Risk listing removed at 0852 UTC 7 Sept. | ||||||
| Assessment postings were noted by A/CC on 5 Sept., 6 Sept. & 7 Sept. - References: MPECs 2008-R26, 2008-R32, 2008-R35, 2008-R64, 2008-S01, 2008-S19, 2008-S20, 2008-S45 & 2008-S93 | |||||||||
| 2008 RV | JPL Sentry | 1348 Sept. 6 | R E M O V E D | Risk listing removed at 0850 UTC 6 Sept. | |||||
| Assessment postings were noted by A/CC on 4 Sept. & 6 Sept. - References: MPECs 2008-R18, 2008-R31, 2008-R32, 2008-R55, 2008-R61, 2008-S13, 2008-S19, 2008-S36, 2008-S69 & 2008-S83 | |||||||||
| 2008 OO | JPL Sentry | 1448 Sept. 2 | R E M O V E D | Risk listing removed at 0852 UTC 2 Sept. | |||||
| An assessment posting was noted by A/CC on 2 Sept. - References: MPECs 2008-R10 & 2008-R15 | |||||||||
| 2008 LA | NEODyS | 1445 Sept. 27 | R E M O V E D | ||||||
| JPL Sentry | 1445 Sept. 27 | R E M O V E D | Risk listing removed at 0851 UTC 27 Sept. | ||||||
| Assessment postings were noted by A/CC on 27 Sept. - References: MPEC 2008-S69 | |||||||||
Legend: VI# = VI count, Prob Cum = cumulative probability, PS Cum/Max = cumulative/maximum Palermo Scale, TS = Torino Scale
For a list of risk-rated objects currently under observation, see our ephemerides page.
An impact solution, also known as a "virtual impactor" (VI), is not a prediction but rather a possibility derived from a variant orbit calculation that cannot be eliminated yet based on the existing data. Elimination can come quickly with just a little further observation or may take weeks or months, sometimes years. Once superceded or eliminated, a former impact solution has zero relevance to an object's risk. See Jon Giorgini's "Understanding Risk Pages" for more information.