L. Bogan et al., THE LIGHT CURVES OF THE ASTEROIDS (198) AMPELLA, (481) EMITA AND (772) TANETE, Journal of the Royal Astronomical Society of Canada, 88(1), 1994, pp. 55-68
The light curve of the main belt asteroid (198) Ampella was measured a
t phase angles 1, 6 and 13 degrees during 10 nights. The periodicity o
f the light curve is 10.378 +/- 0.003 hours. Ampella's photometric amp
litude at opposition is 0.13 magnitudes and increases with phase angle
by 0.006 magnitude/degree. Its two dimensional symmetric profile has
been determined from its light curve and is nearly circular with a bre
adth ratio of 1.13. Less than one quarter of the curve of the asteroid
(481) Emita was measured on one night which gave a lower limit of 20
hours for the period and 0.15 magnitude for the amplitude. A half peri
od or less was measured of the light curve of (772) Tanete which gives
a lower limit for the period of 12 hours and a minimum amplitude of 0
.13 magnitude.