Other
Scientific paper
Jun 1987
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987jbaa...97..220h&link_type=abstract
Journal of the British Astronomical Association, vol.97, no.4, p.220-223
Other
4
Asteroids, Photometry, Physical Properties, Flora, Photoelectric Methods, Rotation, Period, Amplitude, Magnitude, Parameters, Optical Properties, Lightcurves, Earth-Based Observations, Telescope Methods, Popular
Scientific paper
(8) Flora was observed during its perihelic opposition in 1984. From photoelectric observations a possible rotation period of 12.790 +/- 0.005 hours was derived, though other longer periods may also fit the data obtained. The linear portion of the phase curve was found to be described by V(1, a) = (6.673 +/- 0.032) +/- (0.028 +/- 0.001)a for phase angles, a, between 7 and 30 . Using the measured light curve amplitude of 0.07 +/- 0.005 magnitudes, together with results previously published, a longitude for one pole of 148 +/- 10 is deduced.
Bembrick C. S.
Dumont Michel
Hollis Andrew J.
Miles Richard
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