A/CC's Consolidated Risk Tables

Earth Impact Risk Ratings Posted in the Last 31 Days

Compiled at 1327 UTC on 21 May 2013

[ The Tracking News | ephemerides | cleared ]

Missing something? Check the archives for objects not under active observation or recent analysis.

Notes: The time horizon for JPL is 100 years from today and for NEODyS is usually the year 2090. Both risk monitors also post a few special objects with impact solutions beyond 100 years. For the latest official risk assessments, and for explanations of terminology and methodology, see the JPL NEO Program Sentry and NEODyS CLOMON2 risk pages.
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
2013 JD34NEODyS1333 May 182058-205817.93e-10-8.87-8.870Based on 16 optical observations (of which 0 are rejected as outliers) from 2013-05-15.384 to 2013-05-17.312.
JPL Sentry2359 May 17205813.8e-10-9.19-9.190Analysis based on 16 observations spanning 1.9279 days (2013-May-15.3829 to 2013-May-17.31075). Diameter approximately 0.032 km. from mean, weighted H=25.1.
Assessment postings were noted by A/CC on 17 May & 18 May   -   References: MPEC 2013-K08
2013 HT14NEODyS0000 April 242071-207731.22e-06-6.36-6.490Based on 23 optical observations (of which 0 are rejected as outliers) from 2013-04-21.260 to 2013-04-23.276.
JPL Sentry2302 April 232021-207775.1e-06-5.04-5.050Analysis based on 23 observations spanning 2.0169 days (2013-Apr-21.25884 to 2013-Apr-23.27569). Diameter approximately 0.019 km. from mean, weighted H=26.3.
Assessment postings were noted by A/CC on 23 April & 24 April   -   References: MPEC 2013-H39
2013 GA55JPL Sentry2359 April 292070-2113211.2e-05-6.50-7.190Analysis based on 14 observations spanning 1.7271 days (2013-Apr-09.44557 to 2013-Apr-11.17271). Diameter approximately 0.010 km. from mean, weighted H=27.7.
An assessment posting was noted by A/CC on 29 April   -   References: no MPECs
2013 GW38JPL Sentry2359 April 292061-2113136.4e-06-7.07-7.610Analysis based on 18 observations spanning 1.3411 days (2013-Apr-09.45225 to 2013-Apr-10.79339). Diameter approximately 0.007 km. from mean, weighted H=28.5.
An assessment posting was noted by A/CC on 29 April   -   References: no MPECs
2013 GM3JPL Sentry2359 April 292028-21131741.5e-04-4.62-5.490Analysis based on 62 observations spanning 9.9806 days (2013-Apr-03.32112 to 2013-Apr-13.30177). Diameter approximately 0.019 km. from mean, weighted H=26.2.
NEODyS1516 April 242028-20901158.53e-05-4.81-5.530Based on 62 optical observations (of which 2 are rejected as outliers) from 2013-04-03.322 to 2013-04-13.303.
Assessment postings were noted by A/CC on 24 April & 29 April   -   References: DOU 2013-H42
2013 FU13JPL Sentry2359 April 292081-209852.1e-04-5.04-5.110Analysis based on 21 observations spanning 17.219 days (2013-Mar-24.34961 to 2013-Apr-10.568711). Diameter approximately 0.012 km. from mean, weighted H=27.2.
An assessment posting was noted by A/CC on 29 April   -   References: no MPECs
2013 ED28JPL Sentry2359 April 29203613.2e-07-4.18-4.180Analysis based on 41 observations spanning 21.868 days (2013-Mar-07.21735 to 2013-Mar-29.085141). Diameter approximately 0.170 km. from mean, weighted H=21.4.
An assessment posting was noted by A/CC on 29 April   -   References: no MPECs
2012 YR1JPL Sentry2359 April 29207717.4e-07-7.09-7.090Analysis based on 30 observations spanning 23.330 days (2012-Dec-20.20945 to 2013-Jan-12.53922). Diameter approximately 0.017 km. from mean, weighted H=26.5.
An assessment posting was noted by A/CC on 29 April   -   References: no recent MPECs
2012 WR10JPL Sentry2359 April 292087-211225.7e-07-8.36-8.420Analysis based on 45 observations spanning 26.156 days (2012-Nov-22.21759 to 2012-Dec-18.37324). Diameter approximately 0.007 km. from mean, weighted H=28.5.
An assessment posting was noted by A/CC on 29 April   -   References: no recent MPECs
2009 VZ39JPL Sentry0404 May 92013-21107886.9e-06-6.25-7.480Analysis based on 8 observations spanning .04342 days (2009-Nov-10.27204 to 2009-Nov-10.31546). Diameter approximately 0.009 km. from mean, weighted H=27.9.
An assessment posting was noted by A/CC on 9 May   -   References: no recent MPECs
99942 Apophis (2004 MN4)NEODyS1916 May 12060-2105125.71e-06-3.19-3.320Based on 3987 optical observations (of which 0 are rejected as outliers) from 2004-03-15.126 to 2013-04-15.157 and also on twenty radar data points on 2005-01-27, 2005-01-29, 2005-01-30, 2005-08-07, 2006-05-06, 2012-12-21, 2012-12-22, 2013-01-03, 2013-01-05, 2013-01-06, 2013-01-09, 2013-01-10, 2013-01-14, 2013-01-16, 2013-02-18, 2013-02-20 and 2013-03-15.
JPL Sentry1916 May 12060-2105125.7e-06-3.19-3.320Analysis based on 13 radar delay, 7 Doppler, and 3987 optical observations spanning 3318.0 days (2004-Mar-15.126289 to 2013-Apr-15.15729). Diameter approximately 0.330 km. from mean, weighted H=19.7.
Assessment postings were noted by A/CC on 1 May   -   References: DOUs 2013-H24, 2013-H48, 2013-J01, 2013-J05, 2013-J18, 2013-J26 & 2013-J33
C   L   E   A   R   E   D
2013 JR28NEODyS1333 May 18R E M O V E D
JPL Sentry1333 May 18R E M O V E DRisk listing removed at 0950 UTC 18 May
Assessment postings were noted by A/CC on 15 May, 16 May & 18 May   -   References: MPEC 2013-J70 plus DOUs 2013-K12 & 2013-K32
2013 JM22JPL Sentry2008 May 20R E M O V E DRisk listing removed at 1955 UTC 20 May
NEODyS1236 May 16R E M O V E D
Assessment postings were noted by A/CC on 13 May, 14 May, 15 May, 16 May, 17 May & 20 May   -   References: MPEC 2013-J59 plus DOUs 2013-J69, 2013-K01, 2013-K12 & 2013-K32
2013 JW17JPL Sentry1258 May 14R E M O V E DRisk listing removed at 0949 UTC 14 May
Assessment postings were noted by A/CC on 12 May, 13 May & 14 May   -   References: MPEC 2013-J49 plus DOUs 2013-J53, 2013-J60, 2013-K14 & 2013-K24
2013 JS17NEODyS1333 May 18R E M O V E D
JPL Sentry1333 May 18R E M O V E DRisk listing removed at 0951 UTC 18 May
Assessment postings were noted by A/CC on 12 May, 13 May & 18 May   -   References: MPEC 2013-J45 plus DOUs 2013-J53 & 2013-K12
2013 JM14JPL Sentry1459 May 12R E M O V E DRisk listing removed at 0951 UTC 12 May
NEODyS1459 May 12R E M O V E D
Assessment postings were noted by A/CC on 10 May, 11 May & 12 May   -   References: MPEC 2013-J37 plus DOUs 2013-J43, 2013-J60, 2013-K12 & 2013-K24
2013 JH14JPL Sentry1422 May 13R E M O V E DRisk listing removed at 0950 UTC 13 May
Assessment postings were noted by A/CC on 10 May & 13 May   -   References: MPEC 2013-J34 plus DOUs 2013-J53, 2013-K24 & 2013-K32
2013 JE1JPL Sentry1504 May 6R E M O V E DRisk listing removed at 1150 UTC 6 May
NEODyS1504 May 6R E M O V E D
Assessment postings were noted by A/CC on 4 May & 6 May   -   References: MPEC 2013-J12 plus DOUs 2013-J20, 2013-J26, 2013-J32, 2013-J41, 2013-J53, 2013-J60, 2013-K14 & 2013-K24
2013 HT25JPL Sentry1402 May 10R E M O V E DRisk listing removed at 0956 UTC 10 May
NEODyS1402 May 10R E M O V E D
Assessment postings were noted by A/CC on 7 May & 10 May   -   References: MPEC 2013-J24 plus DOU 2013-J33
2013 HRJPL Sentry1349 April 21R E M O V E DRisk listing removed at 0951 UTC 21 April
NEODyS1349 April 21R E M O V E D
Assessment postings were noted by A/CC on 21 April   -   References: DOUs 2013-H25 & 2013-H26
2013 GG69JPL Sentry1622 April 30R E M O V E DRisk listing removed at 1549 UTC 30 April
NEODyS1349 April 21R E M O V E D
Assessment postings were noted by A/CC on 20 April, 21 April, 22 April, 29 April & 30 April   -   References: DOUs 2013-H24, 2013-H26, 2013-H50, 2013-J05, 2013-J11, 2013-J41 & 2013-K14
2013 GF69JPL Sentry1457 April 22R E M O V E DRisk listing removed at 0951 UTC 22 April
NEODyS1349 April 21R E M O V E D
Assessment postings were noted by A/CC on 21 April & 22 April   -   References: DOUs 2013-H25, 2013-H26, 2013-J05, 2013-J11, 2013-J32 & 2013-J60

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.


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