A/CC's Consolidated Risk Tables

Earth Impact Risk Ratings Posted in the Last 28 Days

Compiled at 1548 UTC on 9 February 2010

[ 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 CLOMON (backup) 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
2010 CANEODyS1548 Feb. 92019-206364.65e-05-3.45-3.460Based on 28 optical observations (of which 0 are rejected as outliers) from 2010/02/05.197 to 2010/02/08.173.
JPL Sentry1548 Feb. 92019-202844.5e-05-3.46-3.470Analysis based on 28 observations spanning 2.9758 days (2010-Feb-05.19638 to 2010-Feb-08.172148). Diameter approximately 0.041 km. from mean, weighted H=24.6.
Assessment postings were noted by A/CC on 6 Feb., 7 Feb., 8 Feb. & 9 Feb.   -   References: MPECs 2010-C16, 2010-C18, 2010-C22 & 2010-C24
2009 XONEODyS1750 Jan. 172038-208323.56e-07-4.16-4.260Based on 221 optical observations (of which 0 are rejected as outliers) from 2009/12/09.153 to 2010/01/16.546.
JPL Sentry1750 Jan. 172038-208123.0e-07-4.19-4.260Analysis based on 221 observations spanning 38.393 days (2009-Dec-09.152 to 2010-Jan-16.54518). Diameter approximately 0.270 km. from mean, weighted H=20.5.
Assessment postings were noted by A/CC on 12 Jan., 13 Jan., 14 Jan., 15 Jan. & 17 Jan.   -   References: MPECs 2010-A60, 2010-A66, 2010-A74, 2010-A79 & 2010-B03
2009 WM1NEODyS1521 Jan. 25207813.99e-09-6.27-6.270Based on 84 optical observations (of which 0 are rejected as outliers) from 2009/11/17.465 to 2010/01/24.561.
JPL Sentry1502 Jan. 25209119.3e-08-4.98-4.980Analysis based on 84 observations spanning 68.097 days (2009-Nov-17.4641 to 2010-Jan-24.5607). Diameter approximately 0.280 km. from mean, weighted H=20.4.
Assessment postings were noted by A/CC on 25 Jan.   -   References: MPEC 2010-B39
C   L   E   A   R   E   D
2010 BU2NEODyS1637 Jan. 23R E M O V E D
JPL Sentry1637 Jan. 23R E M O V E DRisk listing removed at 1049 UTC 23 Jan.
Assessment postings were noted by A/CC on 22 Jan. & 23 Jan.   -   References: MPECs 2010-B29, 2010-B34, 2010-B37, 2010-B39, 2010-B42, 2010-B45, 2010-B56, 2010-B60, 2010-B68 & 2010-C01
2010 BL2NEODyS1637 Jan. 23R E M O V E D
JPL Sentry1637 Jan. 23R E M O V E DRisk listing removed at 1052 UTC 23 Jan.
Assessment postings were noted by A/CC on 20 Jan., 21 Jan. & 23 Jan.   -   References: MPECs 2010-B17, 2010-B26, 2010-B34, 2010-B37, 2010-B45, 2010-C03 & 2010-C15
2010 BBJPL Sentry1503 Jan. 18R E M O V E DRisk listing removed at 1040 UTC 18 Jan.
Assessment postings were noted by A/CC on 17 Jan. & 18 Jan.   -   References: MPECs 2010-B05, 2010-B07, 2010-C03, 2010-C05, 2010-C15 & 2010-C24
2010 AF40NEODyS1502 Jan. 15R E M O V E D
JPL Sentry1502 Jan. 15R E M O V E DRisk listing removed at 1056 UTC 15 Jan.
Assessment postings were noted by A/CC on 13 Jan., 14 Jan. & 15 Jan.   -   References: MPECs 2010-A68, 2010-A74, 2010-A79, 2010-B01, 2010-B07, 2010-B09, 2010-B14 & 2010-B56, radar: 25 Jan.
2010 AE30JPL Sentry1501 Jan. 12R E M O V E DRisk listing removed at 0951 UTC 12 Jan.
An assessment posting was noted by A/CC on 12 Jan.   -   References: MPECs 2010-A60, 2010-A66, 2010-A74, 2010-A79, 2010-B01, 2010-B03 & 2010-B07
2005 UONEODyS1505 Jan. 21R E M O V E D
JPL Sentry1800 Jan. 20R E M O V E DRisk listing removed at 1703 UTC 20 Jan.
Assessment postings were noted by A/CC on 20 Jan. & 21 Jan.   -   References: MPEC 2010-B15

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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