July 2001 - monthly monitor




Highlights from the month

The present summary includes activities and results conducted from June 10 to July 8, 2001. A total of 18 NEOs were discovered, 16 single-opposition targets were recovered and a few more interesting observations were made.

None among the newly discovered NEAs seems to be particularly hazardous for the Earth in the near future.




NEO discoveries of the month

This month 17 new NEAs were discovered by 3 observing programs: 8 by LINEAR (code 704), 7 by PALOMAR-NEAT (644), and 2 by LONEOS. While some of the discovery programs have suffered from cloudy weather especially during the second half of the lunation, PALOMAR-NEAT has confirmed the great potential of the system thanks also to nice weather conditions, pretty common in southern California during the summer.

As for the cometary component of NEOs, one such comet was discovered, among those with a perielion distance < 1.3 AU, bringing the total number of discoveries of the month to 18. This comet, designated P/2001 MD7 (LINEAR), has a revolution period of 7.50 years, and has a typical orbit of a short-period comet.

In the following table, the first column reports the provisional designation assigned by the MPC to the new object, the second shows the MPC code of the discovery site and the third reports the follow-up status of the object. This is indicated by a letter which corresponds to a specific interval of values of the object MUR.



where

- T is given for  MUR > 20.0
- U is given for  5.0 < MUR < 20.0
- V is given for  1.0 < MUR <  5.0
- W is given for  0.3 < MUR <  1.0
- X is given for  0.1 < MUR <  0.3
- Y is given for  MUR <  0.1
A list of the MUR status for all NEAs is available here. It has been made available according to this nomenclature and it does not include numbered objects.


Additional notes:


- 2001 MS3 a small NEA (about 100 meter in size) was discovered a few days after a close encounter with the Earth at 0.025 AU.

- 2001 LO7 and 2001 MZ7 are rather large NEAs, with sizes around 3 to 5 km. 2001 LO7, which shows a very large eccentricity was discovered in the outer side of the main-belt region.




NEO follow-up observations

Follow-up efforts have been pretty successful during the past lunation. They have concentrated towards the recovery of single apparition targets while only a few objects in urgent need of observations were followed in the course of the discovery apparition.

The following sections provide more details on these results.


Critical observations of NEOs in urgent need of observations

The following list is a summary of critical observations, made when these targets were flagged as a Urgent in the Priority List


     Object      Obs. type   observatory code  (MPC)

  • 2001 KD68 - UR - 691
  • 2001 MG1 - UR - 046, 360, 649
  • 2001 MS3 - UR - 671, 649, 422
  • 2001 BO60 - UR - 413(1)
  • 2001 BF10 - UR + SP - 807
  • 2001 KO20 - UR - 413(1)
  • 2000 KO41 - UR - 413(1)
  • 2001 KY66 - UR - 413(1)
  • 2001 LL5 - UR - 413(1)
  • 2001 ME1 - UR - 413(1)
  • 2001 MY7 - UR - 413(1)
SC = special campaign directly coordinated by the Spaceguard Central Node

UR = Targets listed as urgent at the time of observation, either in the Priority List or in the Faint NEO List.

radar = radar observations

FNL = targets reported as Necessary on the Faint NEO List or made under special conditions, beyond the threshold of the FNL. For example, observations of faint targets made at small solar elongations (SSE).

The number in parenthesis next to some observatory codes indicates the team that was observing from that observing site, according to the MPC nomenclature.


Missing observations of targets in urgent need of observations

We briefly summarize a list of NEOs insufficiently observed, which terminated their visibility apparition during this monthly period, according to this plot. These objects, recently reported in urgent need of observations, should be now considered lost because of insufficient follow-up and/or because of the intrinsic limits of optical astrometry. Next to the target designation we have reported its absolute magnitude.



NEO recoveries of the month

In the past month, 16 NEOs have been added to the list of multiple-opposition list. The great bulk of this effort was provided by DANEOPS in the form of targeted searches with a 1.5-m reflector at Calar Alto Observatory in Spain. Six NEOs were precovered on photographic archives, mostly by DANEOPS and by R.H. McNaught. No identifications on pre-existing data or accidental recoveries were made during this lunation.

In the following scheme we report the object designation, the kind of recovery and the observatory codes involved in the observations.


R indicates a targeted recovery at the telescope
P indicates a precovery on some archival collection
I indicates an identification from pre-existing observations
A indicates an accidental recovery at the telescope

Further notes:



Missing Recoveries

We report a list of single opposition NEAs that have not been recovered during the current apparition, and ended their visibility during this monthly period, according to this plot:


These targets were recently listed in the Recovery and Bright Lost NEOs services during the past recovery opportunity.


Summary of special campaigns

During this monthly period further observations of 2001 BF10 were reported by a team working with TNOs from Cerro Tololo. Although the observing campaign of this object was terminated with the availability of radar observations during the past lunation, the new data has been still very useful and would have been mentioned in the closing announcement if reported earlier to the MPC and SCN.

There are no NEOs under special surveillance at the moment. Around July 24th, a relatively small Aten, 2000 PH5, is expected to have a very close encounter with the Earth at 0.010 AU. Radar observation may take place on July 27, 28 if a recovery is made before the radar opportunity: in fact, the sky uncertainty of 2000 PH5 will be of many degrees.

For more information or short-term changes, please keep looking at the section related to Special Campaigns, or directly on the New Announcement list or, if solved, on the list of Successful campaigns.


Sky coverage summary of the big surveys

This month there was a significant decrease of the number of discoveries respect to the previous lunation because the search activity was significantly reduced during the second half of the lunation. Nevertheless, it is not clear exactly how much was the total sky coverage operated by the big surveys since there is still no information about the work done with the Palomar-NEAT system. No NEO searching could be performed on five nights concentrated near full Moon: June 26, July 1, 6, 7 and 8.

These comments and sky coverage analysis are based on sky coverage plots available at the Lowell Observatory and the Minor Planet Center.