[Iaude] CBET 5373: (1879) BROEDERSTROOM
quai at eps.harvard.edu
quai at eps.harvard.edu
Tue Mar 26 20:19:14 EDT 2024
Electronic Telegram No. 5373
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
(1879) BROEDERSTROOM
V. Benishek, Belgrade Astronomical Observatory; P. Pravec, Ondrejov
Observatory; A. Marchini and R. Papini, Dipartimento di Scienze Fisiche, Della
Terra e Dell'Ambiente, University of Siena; F. Pilcher, Organ Mesa
Observatory, Las Cruces, NM, USA; N. Ruocco, Osservatorio Astronomico Nastro
Verde, Sorento, Italy; and R. Durkee, Shed of Science South Observatory,
Pontotoc, TX, USA, report that photometric observations taken with a 0.35-m
telescope at the Sopot Observatory in Serbia, a 0.30-m telescope at the
Astronomical Observatory of the University of Siena, a 0.35-m telescope at
the Organ Mesa Observatory, a 0.35-m telescope at the Nastro Verde
Observatory, and a 0.50-m telescope at the Shed of Science South Observatory
during Jan. 22-Mar. 3 reveal that minor planet (1879) is a binary system with
an orbital period of 47.83 +/- 0.02 hr. The primary shows a period of
3.01543 +/- 0.00008 hr and has a light-curve amplitude of 0.16 magnitude at
solar phases 1-5 degrees, suggesting a nearly spheroidal shape. Mutual
eclipse/occultation events that are 0.12 magnitude deep indicate a
secondary-to-primary mean-diameter ratio of 0.34 +/- 0.02.
NOTE: These 'Central Bureau Electronic Telegrams' are sometimes
superseded by text appearing later in the printed IAU Circulars.
(C) Copyright 2024 CBAT
2024 March 26 (CBET 5373) Daniel W. E. Green
More information about the Iaude
mailing list