Zwicky is a bright, stony
S-type asteroid, in line with the overall spectral type for members of the
Phocaea family.
Lightcurves In July 2018, a rotational
lightcurve of
Zwicky was obtained from
photometric observations by the
TESS-team which gave a
rotation period of () hours and an amplitude of ()
magnitude (). Observations by
Tom Polakis, who also discovered a satellite
(see below) determined a very similar period of () hours with a brightness variation of () (). These more recent result are replacing a previous observation from March 2003, of a fragmentary lightcurve by French amateur astronomer
Laurent Bernasconi that gave a tentative period of 27.1 hours and an amplitude of 0.08 ().
Diameter and albedo According to the surveys carried out by the Japanese
Akari satellite and NASA's
Wide-field Infrared Survey Explorer with its subsequent
NEOWISE mission,
Zwicky measures between and kilometers in diameter, and its surface has an
albedo of and , respectively. The
Collaborative Asteroid Lightcurve Link assumes a standard albedo for Phocaea asteroids of 0.23, and calculates a diameter of 10.06 kilometers based on an
absolute magnitude of 12.2. The WISE team also published an alternative mean-diameters of () and () kilometers with a corresponding albedo of () and ().
Satellite Photometric observations at the Command Module Observatory by Tom Polakis on 21 February 2021 revealed that
Zwicky has a
satellite in its orbit. The moon has a diameter of approximately 2.50 kilometers, or 26% of that of its primary, and an orbital period of 28.46 hours. == References ==