Contents on 12 November '08
- IAU Minor Planet Center
- NEOCP Activity -- none
- New MPECs -- two MPECs
- Observers -- seven observing facilities
- Impact Risk Monitoring -- three objects
- Chronology
Resources:
- Consolidated Risk Tables - the CRT page
- Earth's Busy Neighborhood Traffic Report
- Ephemerides for risk-rated and nearby objects
- Old & new CRT Archive
- Old News Archive & Small Objects Archive
The latest A/CC news is available via framed access,
RSS news feed, or redirection. - Note: A/CC has a main Web site and also a backup site with its own duplicate RSS news feed.
Navigation tips: Use the << and >> arrows on the menus for each regular section (Observers, Risks, etc.) to move to the previous and next day's news for that section. Use the Index menu item to access specific days through a calendar interface. And use the all-up news archive to access news from any time since A/CC began in early 2002. To keep track of what's new each day, watch the Chronology section.
NEOCP Activity on 12 November '08
The MPC's NEO Confirmation Page is currently empty
The NEOCP is currently empty. There were five listings noted earlier today.
New MPECs on 12 November '08
Minor Planet Electronic Circulars
As of last check at 2358 UTC, there have been two MPECs issued today from the International Astronomical Union's Minor Planet Center in Cambridge, Massachusetts.
- MPEC 2008-V57 time-stamped "03:47 UT" - 2001 XQ = 2008 VV4 - see below
- MPEC 2008-V58 time-stamped "07:14 UT" - Daily Orbit Update
<< DOU on 12 Nov. '08 >> MPEC 2008-V58 - "07:14 UT" - Daily Orbit Update
- Observations of risk-listed objects
- K08V14L 2008 VL14 (arc=3 days, H=21.0 ~214m) from Great Shefford Obs. (Nov. 11.98-00p2)
- K08U99W 2008 UW99 (small asteroid, arc=10 days, H=24.7 ~39m) from Astronomical Research Obs. (ARO) (Nov. 5.24-25p3 & 10.39-40p3)
- Observations of recently (no longer) risk-listed objects
- K08V00E 2008 VE (small asteroid, Q=4.418 AU, arc=5 days, H=22.1 ~129m) from ARO (Nov. 5.23-24p4)
- K08U95B 2008 UB95 (small asteroid, arc=7 days, H=24.7 ~39m) from ARO (Nov. 5.02-05p3)
- K08U07E 2008 UE7 (arc=16 days, H=20.5 ~269m) from Lumijoki Obs. (Nov. 2.94-95p3 & 4.96p3), ARO (Nov. 5.21-22p5), and Desert Moon Obs. (Nov. 11.41-43p4)
- K08U05T 2008 UT5 (small asteroid, arc=17 days, H=24.5 ~43m) from Balzaretto Obs. (Nov. 9.82p1)
- K08S82H 2008 SH82 (arc=46 days, H=21.0 ~214m) from Desert Moon Obs. (Nov. 11.11-16p3)
- Observations of small asteroids (H>22.0)
- K08V03U 2008 VU3 (Q=4.025 AU, arc=8 days, H=23.4 ~71m) from ARO (Nov. 10.37p4)
- K08V00K 2008 VK (arc=3 days, H=23.4 ~71m) from ARO (Nov. 5.15-16p3)
- K08UA0P 2008 UP100 (arc=7 days, H=23.9 ~56m) from ARO (Nov. 5.08-09p3)
- K08U91Z 2008 UZ91 (arc=12 days, H=22.4 ~112m) from ARO (Nov. 5.13-14p3)
- K08T09Y 2008 TY9 (arc=30 days, H=24.9 ~35m) from ARO (Nov. 5.16-18p3)
- Observations of other objects
- K08V00N 2008 VN (Q=5.166 AU, arc=6 days, H=16.7 ~1.55 km) from ARO (Nov. 5.27p5)
- K08V00F 2008 VF (arc=6 days, H=19.4 ~446m) from ARO (Nov. 5.28-29p6)
- K08U95C 2008 UC95 (arc=9 days, H=18.4 ~708m) from ARO (Nov. 5.35-36p5)
- K08U91W 2008 UW91 (arc=11 days, H=21.7 ~155m) from ARO (Nov. 5.06-07p2)
- K08U90L 2008 UL90 (IEO, Q=0.959 AU, arc=16 days, H=18.4 ~708m) from Desert Moon Obs. (Nov. 11.46-49p3)
- K08U07D 2008 UD7 (arc=16 days, H=18.9 ~562m) from Desert Moon Obs. (Nov. 11.36-39p3)
- K08T02R 2008 TR2 (arc=31 days, H=19.9 ~355m) from ARO (Nov. 5.12p1)
- K08T02Q 2008 TQ2 (arc=33 days, H=20.8 ~234m) from ARO (Nov. 5.30-31p2)
- K08S07V 2008 SV7 (arc=42 days, H=21.6 ~162m) from ARO (Nov. 5.32p4)
- K08R26T 2008 RT26 (arc=59 days, H=19.3 ~467m) from ARO (Nov. 5.33-35p3)
- K08Q01D 2008 QD1 (arc=75 days, H=19.0 ~537m) from ARO (Nov. 5.10-11p4)
- K08M00Z 2008 MZ (Q=4.207 AU, arc=145 days, H=18.6 ~645m) from ARO (Nov. 5.25-26p6)
- K05W56J 2005 WJ56 from the Catalina Sky Survey (CSS) (Nov. 1.45-47p4)
- 66146 66146 1998 TU3 from LINEAR (Oct. 1.41-46p5)
- 07358 7358 Oze (1995 YA3) from LINEAR (Oct. 28.42-47p4)
- 01627 1627 Ivar (1929 SH) from LINEAR (Sept. 29.36-40p4)
MPEC 2008-V57 - "03:47 UT" - 2001 XQ = 2008 VV4
- K01X00Q 2001 XQ (Q=6.249 AU, H=19.3 ~467m)
Observers on 12 November '08
Seven observing facilities appear in today's MPEC.
| Code | Observer / observatory |
|---|---|
| H55 | Astronomical Research Obs. (ARO) in Illinois, 19 in MPEC 2008-V58 -- 2008 VU3, 2008 VN, 2008 VK, 2008 VF, 2008 VE, 2008 UZ91, 2008 UW99, 2008 UW91, 2008 UP100, 2008 UE7, 2008 UC95, 2008 UB95, 2008 TY9, 2008 TR2, 2008 TQ2, 2008 SV7, 2008 RT26, 2008 QD1, 2008 MZ |
| A81 | Balzaretto Obs. in Italy, 1 in MPEC 2008-V58 -- 2008 UT5 |
| 703 | Catalina Sky Survey in Arizona, 1 in MPEC 2008-V58 -- 2005 WJ56 |
| 448 | Desert Moon Obs. in New Mexico, 4 in MPEC 2008-V58 -- 2008 UL90, 2008 UE7, 2008 UD7, 2008 SH82 |
| J95 | Great Shefford Obs. in England, 1 in MPEC 2008-V58 -- 2008 VL14 |
| 704 | LINEAR in New Mexico, 3 in MPEC 2008-V58 -- 66146, 7358, 1627 |
| A70 | Lumijoki Obs. in Finland, 1 in MPEC 2008-V58 -- 2008 UE7 |
| For a list of all participating observatories that have Web addresses, see A/CC's Observatory Links page. | |
Impact Risk Monitoring on 12 November '08
| 0000NNN000 Object | Risk Monitor | When Noted UTC | 0000T0000 Year Range | VI # | 000NN00 Prob Cum | T0000 PS Cum | T0000 PS Max | T S | Notes for Today's Latest Risk Assessments |
| 2008 VL14 | NEODyS | 1358 | 2047-2076 | 7 | 6.29e-07 | -3.89 | -4.07 | 0 | NEODyS: "Based on 24 optical observations (of which 0 are rejected as outliers) from 2008/11/09.266 to 2008/11/12.005." |
| JPL Sentry | 1357 | 2032-2103 | 13 | 8.9e-07 | -3.78 | -4.05 | 0 | JPL: "Analysis based on 24 observations spanning 2.7383 days (2008-Nov-09.2656 to 2008-Nov-12.00394)." Diameter approximately 0.219 km. from mean, weighted H=21.0. | |
| 2008 VV4 | NEODyS | 1357 | R E M O V E D | - | |||||
| 2008 UW99 | JPL Sentry | 1357 | 2085-2093 | 2 | 3.2e-07 | -6.67 | -6.96 | 0 | JPL: "Analysis based on 31 observations spanning 9.9448 days (2008-Oct-31.45784 to 2008-Nov-10.40268)." Diameter approximately 0.038 km. from mean, weighted H=24.7. |
Legend: VI# = VI count, Prob Cum = cumulative probability, PS Cum/Max = cumulative/maximum Palermo Scale, TS = Torino Scale
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" to learn more.
Chronology on 12 November '08
Times are UTC for when items were noted or added by The Tracking News.
| 1607 | The NEOCP has become empty |
| 1358 | Noted that NEODyS has updated its 2008 VL14 risk assessment - see above |
| 1357 | Noted that JPL Sentry has reposted 2008 UW99 as an impact risk - see above Noted that JPL Sentry has updated its 2008 VL14 risk assessment - see above Noted that NEODyS has removed 2008 VV4 as an impact risk - see above Grabbed MPEC 2008-V58 - Daily Orbit Update - see above |
| 0359 | Grabbed MPEC 2008-V57 - 2001 XQ = 2008 VV4 - see above |