Transylvania has been characterized as a carbonaceous
C-type asteroid by
PanSTARRS photometric survey.
Rotation period In September 2004, a rotational
lightcurve of Transylvania was obtained from photometric observations by French amateur astronomer
Laurent Bernasconi. Analysis of the fragmentary lightcurve gave a
rotation period of 12 hours with a brightness amplitude of 0.15
magnitude (). As of 2017, no other lightcurve has been obtained, and Transylvania's period is still uncertain.
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, Transylvania measures between 13.77 and 21.49 kilometers in diameter and its surface has an
albedo between 0.05 and 0.1619. The
Collaborative Asteroid Lightcurve Link derives an albedo of 0.1047 and a diameter of 13.60 kilometers based on an
absolute magnitude of 12.4. == Naming ==