2006 October notes: 2006 RZ and 2006 TA8

The month started off with Apollo 2006 RZ (mentioned last month) passing close by the Earth on Oct 6/7. It was tracked on the 6th until about 20:15UT, moving at 86"/min at 15th mag. those positions being the last reported of the object. However, it was picked up again 4.5 hours later, through a gap in the trees, just 10 degrees above the north horizon, moving very obviously between frames. By then it was at the unusually large phase angle of 119 degrees, but unfortunately there were too few comparison stars visible in the images to measure positions.

A number of good nights during October were used to go for some very faint NEOs, an increasing number of which are being put on the NEOCP, mainly by the Catalina and Spacewatch surveys. However, there were also a proportion of bright and often fast moving objects discovered, including 2006 TA8, discovered by LINEAR at high northern declinations on Oct 12 and followed as a 16th mag object on Oct 13, 17 & 22 from Great Shefford, after which it disappeared south in the morning sky.

2006 September notes: 2006 RZ, 2006 SU49 and 2006 SO198

Generally poor weather continued here during September, still, some work was done on 14 nights, but again few long runs on any particular object could be done.

2006 RZ is a relatively rare amateur NEO discovery, having been picked up at 18th mag by H. Michels from Herrenberg on Sep 4th. It was followed from early September through to the end of the month, passing about 5 lunar distances away in the first week of October having brightened to mag 14.

Some other interesting objects were followed, 2006 SU49 being posted as an impact risk at Torino scale 1 for a number of days before being removed after being found on old NEAT and Sloan archive images going back 5 years.

2006 SO198 was discovered by LONEOS on Sep 29 and was confirmed from Great Shefford while on the NEOCP. It was at the 'fast' end of it's uncertainty area, mag 18 and moving at about 3"/min, about 11' away from the prediction. Less than 4 days later it was to make a pass just outside the orbit of the moon. It was last seen the day before at 16th mag moving at 30"/min, but would have been 14th mag and moving at 800"/min at closest, but it would have been only visible from S. Africa-India and was not reported.

2006 August notes: 2006 ON1, 2006 QV89, 6Q0B44E

Although some work was done on 16 nights in August, many sessions were interrupted by cloud with just a couple of nights judged as good. Most of the NEOs followed were observed on single nights only, the exception being Apollo 2006 ON1 with three nights.

Apollo 2006 QV89 was observed while it was on the NEOCP and is interesting because its minimum orbital intersection distance with the Earth (MOID) is currently given as 0.00001 AU or about 1,000 miles. At the time of writing (Sep 5th) it is listed with a 1 in ~800 chance of collision with Earth in 2019, so just as well it is only about 30 metres in diameter... Further positions in the coming days are desirable.

On Aug 29th positions for 6Q0B44E were obtained, discovered by the Catalina survey the day before and subsequently found to be in an unstable 80 day orbit around the Earth. It is still unclear whether this is an artificial satellite re-captured by the Earth similar to the Apollo 12 S-IVB third stage J002E3 back in 2003 or whether it is a very small (1-5 metre diameter) NEO temporarily captured by Earth. As noted by Bill Gray, with the current data, it looks as if this object probably entered the Earth/Moon system sometime between about 2000 and 2003, though dates as far back as 1991 are quite possible. Paul Chodas (JPL) comments that it will stay in Earth orbit for at least three more years.

2006 July notes

With the summer monsoon having taken hold in the southern USA, stopping the big surveys from operating for most of the month, time was spent catching some NEOs at their second and subsequent oppositions.

Working with Roger Dymock we also went after some more normal main belt minor planets on the FUAP (Follow Up Astrometric Program) target list at http://asteroidi.uai.it/ which is maintained by Sergio Foglia on behalf of the UAI Minor Planets Section. This site lists minor planets of mag +18.5 or brighter that are in need of observation, whether newly discovered and under-observed, or awaiting recovery at their second or subsequent oppositions.

The last week of the month saw a flurry of NEO discoveries from the surveys in a brief respite from their bad weather, with several objects at mag 16-17.

2006 June notes: 2006 KZ112 and 2006 MU6

Several objects were followed over a period of a couple of weeks during the month, including 2006 KZ112 which has an interesting 'Encke like' orbit (2006 KZ112: q=0.29, e=0.89, i=38, P=4.0, Encke: q=0.33, e=0.85, i=12, P=3.3).

Of the other objects observed, 2006 MU6 was picked up on June 27 after being discovered by Spacewatch on June 20th and is a possible Mars Trojan (though the uncertainties on the orbital elements are still large). Already very faint it is predicted to fade quickly.