THE LIGHT CURVES OF THE ASTEROIDS (198) AMPELLA, (481) EMITA AND (772) TANETE

Citation
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
Citations number
NO
Categorie Soggetti
Astronomy & Astrophysics
ISSN journal
0035872X
Volume
88
Issue
1
Year of publication
1994
Pages
55 - 68
Database
ISI
SICI code
0035-872X(1994)88:1<55:TLCOTA>2.0.ZU;2-U
Abstract
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.