In the
Tholen classification,
Dysonas
spectral type is ambiguous, closest to a primitive
P-type and somewhat similar to a
D- and
C-type asteroid (PDC).
Rotation period and pole In April 2006, a rotational
lightcurve of
Dysona was obtained by
Julian Oey at Leura Observatory () in Australia. Lightcurve analysis gave a
rotation period of 8.6080 hours with a brightness variation of 0.24
magnitude (), superseding photometric observations by Jean-Gabriel Bosch and Laurent Brunetto in October 2010, who measured a period of 8.355 hours and an amplitude of 0.25 magnitude (). In 2016, a modeled lightcurve using data from UAPC, the
Palomar Transient Factory survey, and individual observers, gave a concurring period of 8.60738 hours as well an
astronomical pole of (125.0°, −68.0°) in
ecliptic coordinates (λ, β).
Diameter and albedo According to the surveys carried out by the Infrared Astronomical Satellite
IRAS, the Japanese
Akari satellite and the
NEOWISE mission of NASA's
Wide-field Infrared Survey Explorer,
Dysona measures between 70.757 and 83.05 kilometers in diameter and its surface has an
albedo between 0.04 and 0.0585. The
Collaborative Asteroid Lightcurve Link adopts the results obtained by IRAS, that is, an albedo of 0.0425 and a diameter of 83.05 kilometers based on an
absolute magnitude of 9.45. == Naming ==