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Astrometric observations near the maximum approach of the Potentially Hazardous Asteroid (66391) 1999 KW4

ATel #13002; J. Ricra (Instituto Geofisico del Peru), M. Zegarra-Valles (Instituto Geofisico del Peru), N. O. Baella (Instituto Geofisico del Peru), R. Villanueva (Observatorio y Planetario Moche)
on 8 Aug 2019; 02:21 UT
Credential Certification: Nobar Baella (nbaella@igp.gob.pe)

Subjects: Optical, Asteroid, Near-Earth Object, Potentially Hazardous Asteroid, Asteroid (Binary)

Referred to by ATel #: 13005

Our team decided to collaborate with the campaign to observe the maximum approach of the PHA (66391) 1999 KW4, organized by the International Asteroid Warning Network (IAWN).

The observations were made from CIEASEST, in the Universidad Nacional San Luis Gonzaga de Ica, Peru (Long. 75 44 12.5 W, Lat. 14 05 21.1 S, Alt. 401 m). A 60 cm Nishimura telescope (f10) and a ZWO ASI 071MC camera were used.

The night of the maximum approach (May 25, 2019) we had cloudy skies; however, the night of May 26-27 we had clear skies and we were able to take 147 images with a exposure time of 4 seconds. Dimension 4 software was used to synchronize our time with special purpose Internet Time Servers, ensuring less than one second accuracy.

The astrometric measurements were made with the Astrometrica software, using between 15 and 25 stars in the field identified by means of the Gaia DR2 catalog.

Table 1 shows the best measurements obtained.

Here is a gif animation of the 1999 KW4 passage.

Table 1
Object Date (UTC, Mid-exposure) RA DEC Mag SNR
66391 C2019 05 27.12028 09 40 11.314 -20 26 45.93 14.92G 50.68
66391 C2019 05 27.12066 09 40 12.737 -20 26 29.84 14.11G 41.49
66391 C2019 05 27.12100 09 40 13.876 -20 26 17.92 14.65G 52.45
66391 C2019 05 27.12361 09 40 22.658 -20 24 28.28 14.57G 53.50
66391 C2019 05 27.12562 09 40 29.578 -20 23 06.89 14.86G 55.15
66391 C2019 05 27.12657 09 40 32.864 -20 22 28.30 14.81G 48.48