[Iaude] CBET 5412: 2021 CJ_16
quai at eps.harvard.edu
quai at eps.harvard.edu
Wed Jul 10 10:48:14 EDT 2024
Electronic Telegram No. 5412
Central Bureau for Astronomical Telegrams
Mailing address: Hoffman Lab 209; Harvard University;
20 Oxford St.; Cambridge, MA 02138; U.S.A.
e-mail: cbatiau at eps.harvard.edu (alternate cbat at iau.org)
URL http://www.cbat.eps.harvard.edu/index.html
Prepared using the Tamkin Foundation Computer Network
2021 CJ_16
P. Pravec, P. Kusnirak, K. Hornoch, H. Kucakova, and P. Fatka, Ondrejov
Observatory, report that photometric observations taken with a 1.54-m
telescope at the La Silla station of the European Southern Observatory during
2024 Apr. 9-May 12 reveal that the Amor-type minor planet 2021 CJ_16 is a
binary system with an orbital period of 16.28 +/- 0.02 hr. Mutual eclipse/
occultation events that are 0.56 to 0.70 magnitude deep indicate a lower limit
on the secondary-to-primary mean-diameter ratio of 0.82. There is apparent a
rotational lightcurve at orbital phases outside the mutual events with a
period equal to the orbital period and an amplitude of 0.22 magnitude at solar
phases 7-35 degrees, suggesting that one or both components of the binary
system are synchronous and moderately elongated. The system's mean absolute
magnitude is H = 20.20 +/- 0.04 with a phase-relation slope parameter G = 0.29
+/- 0.03. The color index in the Johnson-Cousins photometric system is
(V - R) = +0.41 +/- 0.02. Follow-up observations (e.g., photometric or
spectroscopic) taken during the rest of the current observable apparition of
the minor planet are encouraged so as to improve the characterization of the
binary system.
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2024 CBAT
2024 July 10 (CBET 5412) Daniel W. E. Green
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