In the
SMASS classification,
Gothlandia is a stony
S-type asteroid, which corresponds to the overall
spectral type for Florian asteroids.
Rotation period and poles Several rotational
lightcurves of
Gothlandia have been obtained from photometric observations since the 1990s. Lightcurve analysis gave a consolidated
rotation period of 3.4916 hours with a brightness variation of 0.81
magnitude (). A high brightness amplitude typically indicates a non-spherical shape. Modeled lightcurves using data from the Uppsala Asteroid Photometric Catalogue (UAPC) and other sources gave a concurring period 3.491820 hours. In 2013, another modeled lightcurve obtained form photometric data collected by the
Catalina Sky Survey also determined a spin axis of (334.0°, −84.0°) 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,
Gothlandia measures between 11.19 and 14.255 kilometers in diameter and its surface has an
albedo between 0.2065 and 0.41. The
Collaborative Asteroid Lightcurve Link derives an albedo of 0.2631 and a diameter of 12.46 kilometers based on an
absolute magnitude of 11.59. == Naming ==