Planetary radar targets 1999 AP10, 2000 TO64, 2000 UJ1, and 2000 XK44: Four S-complex near-Earth asteroids.
ATel #2323; M. Hicks (JPL/Caltech), K. Lawrence (JPL/Caltech)
on 2 Dec 2009; 21:25 UT
Credential Certification: Michael D. Hicks (Michael.Hicks@jpl.nasa.gov)
Subjects: Optical, Asteroid, Planet (minor), Solar System Object
Referred to by ATel #: 2371
We report taxonomic classifications of four near-Earth asteroids (1999 AP10, 2000 TO64,
2000 UJ1, and 2000 XK44) scheduled for radar observation by the JPL radar group at the
Arecibo facility in Oct-Nov 2009, using long-slit CCD spectroscopy acquired at the
Palomar 5-m telescope on 2009 Nov 09 UT. Table 1 lists the observation circumstances.
Normalized reflectance spectra are shown in Figures 1-4
[1][2][3][4]
A comparison of our optical spectra with the 1341 asteroid spectra as archived in the
SMASS II database (Bus & Binzel 2002) was used to determine taxonomy and we found
1999 AP10 (L-type), 2000 TO64 (Sq-type), 2000 UJ1 (S-type), and 2000 XK44 (S-type) to
all be members of the S-type spectral complex. Table 2 list the five best-fit SMASS II
analogs for each of our asteroids. All targets excluding 2000 XK44 were observed on
2009 Oct 19 UT (ATEL#2283), with similar results. Due to evolution of the observational
geometry, 2000 UJ1 had brightened by 4.3 magnitudes from Oct 19 to Nov 9, therefor
taxonomy from the later date is significantly more robust.
Near-IR spectroscopy and thermal flux measurements for each target over the remainder
of their apparitions would be extremely useful to help further constrain size, albedo,
and surface composition.
Copyright 2009. All rights reserved. The research described in this telegram was carried o
ut at the Jet Propulsion Laboratory, under a contract with the National Aeronautics and Space Administration.
Table 1: Observational Circumstances.
Object Name r (AU) delta (AU) p (deg) V (mag) Exp Time (min)
1999 AP10 1.013 0.118 75.9 14.0 16.0
2000 TO64 1.053 0.115 54.4 14.3 17.0
2000 UJ1 1.077 0.114 38.4 14.7 10.0
2000 XK44 1.066 0.077 10.9 13.3 11.0
Table 2: Best-fit SMASS II spectral analogs.
TAXONOMIC CLASS
MISFIT OBJECT NAME (THOLEN) (BUS)
- for 1999 AP10 -
0.666 42 Isis S L
0.785 824 Anastasia S L
0.790 3287 Olmstead L
0.799 1882 Rauma K
0.846 100 Hekate S S
- for 2000 TO64 -
0.387 1995 BM2 Sq
0.492 1293 Sonja Sq
0.518 2042 Sitarski Sq
0.543 2902 Westerlund Sq
0.566 7056 Kierkegaard Sq
- for 2000 UJ1 -
0.288 2282 Andres Bello S
0.387 4200 Shizukagozen S
0.446 5534 1941 UN S
0.457 5552 Studnicka S
0.465 2478 Tokai S
- for 2000 XK44 -
0.433 2282 Andres Bello S
0.480 4200 Shizukagozen S
0.515 462 Eriphyla S S
0.525 2478 Tokai S
0.532 403 Cyane S S