Contents on 27 January '08
- IAU Minor Planet Center
- NEOCP Activity -- none
- New MPECs -- one MPEC
- Observers -- eight observing facilities
- Impact Risk Monitoring -- one object
- 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 27 January '08
The MPC's NEO Confirmation Page is currently empty
The NEOCP is currently empty. There was one listing noted earlier today.
New MPECs on 27 January '08
Minor Planet Electronic Circulars
As of last check at 2354 UTC, there has been one MPEC issued today from the International Astronomical Union's Minor Planet Center in Cambridge, Massachusetts.
<< DOU on 27 Jan. '08 >> MPEC 2008-B51 - "07:07 UT" - Daily Orbit Update
- Observations of risk-listed objects
- K08A04F 2008 AF4 (arc=17 days, H=19.8 ~371m) from Verona Obs. (Jan. 23.99-00p4) and Naef Obs. (Jan. 26.92-95p6)
- Observations of small asteroids (H>22.0)
- K07P09S 2007 PS9 (arc=160 days, H=23.4 ~71m) from Naef Obs. (Jan. 26.89-94p3)
- Observations of other objects
- K07Y01X 2007 YX1 (Q=4.542 AU, arc=2 opp, H=17.2 ~1.23 km) from Klet Obs. (Jan. 25.77-78p4)
- K07T24U 2007 TU24 (arc=108 days, H=20.4 ~282m) from Eschenberg Obs. (Jan. 26.73-75p7) and Petit Jean Mtn. South Obs. (PJMSO) (Jan. 27.02-03p19)
- K05X01D 2005 XD1 (arc=2 opp, H=19.4 ~446m) from Stia Obs. (Jan. 23.79-80p4) and Klet Obs. (Jan. 25.82-83p2)
- K05T45U 2005 TU45 (arc=3 opp, H=17.1 ~1.29 km) from Verona Obs. (Jan. 26.95-96p4)
- J89A00Z 1989 AZ (arc=3 opp, H=19.7 ~389m) from Klet Obs. (Jan. 25.79-80p7) and Begues Obs. (Jan. 26.85p3)
- F3591 153591 2001 SN263 from Begues Obs. (Jan. 26.79p3)
- E4922 144922 2005 CK38 from Naef Obs. (Jan. 26.89-94p4)
- D8947 138947 2001 BA40 from Stia Obs. (Jan. 24.82-84p4)
- 90403 90403 2003 YE45 from Begues Obs. (Jan. 26.89-90p3)
- 68359 68359 2001 OZ13 from Begues Obs. (Jan. 26.78p3)
- 05131 5131 1990 BG from Begues Obs. (Jan. 26.88p3)
- 04450 4450 Pan (1987 SY) from Libbiano Obs. (Jan. 27.02-03p2)
Observers on 27 January '08
Eight observing facilities appear in today's MPEC.
| Code | Observer / observatory |
|---|---|
| 170 | Begues Obs. in Spain, 5 in MPEC 2008-B51 -- 1989 AZ, 90403, 68359, 153591, 5131 |
| 151 | Eschenberg Obs. in Switzerland, 1 in MPEC 2008-B51 -- 2007 TU24 |
| 046 | Klet Obs. in the Czech Republic, 3 in MPEC 2008-B51 -- 2007 YX1, 2005 XD1, 1989 AZ |
| B33 | Libbiano Obs. in Italy, 1 in MPEC 2008-B51 -- 4450 |
| A13 | Naef Obs. in Switzerland, 3 in MPEC 2008-B51 -- 2008 AF4, 2007 PS9, 144922 |
| H45 | Petit Jean Mtn. South Obs. in Arkansas, 1 in MPEC 2008-B51 -- 2007 TU24 |
| A78 | Stia Obs. in Italy, 2 in MPEC 2008-B51 -- 2005 XD1, 138947 |
| A48 | Verona Obs. in Italy, 2 in MPEC 2008-B51 -- 2008 AF4, 2005 TU45 |
Impact Risk Monitoring on 27 January '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 AF4 | NEODyS | 1618 | 2078-2090 | 9 | 1.77e-06 | -3.45 | -3.59 | 0 | NEODyS: "Based on 290 optical observations (of which 3 are rejected as outliers) from 2008/01/10.397 to 2008/01/26.954." |
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.