In the
Tholen classification, Laodamia is a stony
S-type asteroid, while in the
SMASS taxonomy, it is a transitional type between the stony S-type and rare
R-type asteroids.
Rotation period and spin axis In March 2002, a rotational
lightcurve of Laodamia was obtained from photometric observations by French amateur astronomers
Laurent Bernasconi and
Silvano Casulli. Lightcurve analysis gave a well-defined
rotation period of 5.17247 hours with a brightness amplitude of 0.44
magnitude (). Two other lightcurve gave a concurring period of 5.17 and 5.175 hours, respectively (). Photometry taken at the
Rozhen Observatory over a period of more than a decade allowed to model the asteroid's shape and gave two spin axis of (95.0°, −85.5°) and (272.0°, −88.0°) in
ecliptic coordinates (λ, β) ().
Diameter and albedo According to the survey carried out by NASA's
Wide-field Infrared Survey Explorer and its subsequent
NEOWISE mission, Laodamia measures 7.56 kilometers in diameter and its surface has an
albedo of 0.248, while the
Collaborative Asteroid Lightcurve Link adopts an albedo of 0.259 and derives a diameter of 7.39 kilometers based on an
absolute magnitude of 12.74. This makes Laodamia one of the largest mid-sized
Mars-crossing asteroids comparable with
1065 Amundsenia (9.75 km),
1139 Atami (9.35 km),
1474 Beira (14.9 km),
1727 Mette (5.44 km),
1131 Porzia (7.13 km),
1235 Schorria (5.55 km),
985 Rosina (8.18 km),
1310 Villigera (15.24 km) and
1468 Zomba (7 km), but far smaller than the largest members of this dynamical group, namely,
132 Aethra,
323 Brucia,
1508 Kemi,
2204 Lyyli and
512 Taurinensis, which are all larger than 20 kilometers in diameter. == Naming ==