Rotation period and photoelectric lightcurves of Asteroid 471 Papagena

Details Rotation period and photoelectric lightcurves of Asteroid 471 Papagena Rotation period and photoelectric lightcurves of Asteroid 471 Papagena

Oct 1977

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1977a%26as...30..121s&link_type=abstract

Astronomy and Astrophysics Supplement Series, vol. 30, Oct. 1977, p. 121-124.

Astronomy and Astrophysics

Astrophysics

6

Asteroids, Electrophotometry, Light Curve, Planetary Rotation, Albedo, Amplifiers, Declination, Interstellar Extinction, Light Modulation, Solar Orbits, Telescopes

Scientific paper

Asteroid 471 Papagena was observed during the 1976 opposition with a photoelectric photometer attached to the 61-cm Bochum telescope at the European Southern Observatory. The light curve shows a very unusual triple maximum and minimum. The synodic period found is 7 hr 9 min 23 plus or minus 19 sec and the maximum amplitude of the light curve is 0.13 magnitude.

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