The recently improved orbit of the minor planet (loll) Laodamia (Rabe 1956) reveals a remarkable relationship to the orbit of Mars. The trajectories interlock near to the ascending node of Laodamia on Mars, and to the aphelion of Mars. The orbits approach to 0.04 a.u., yet the approach is so asymptotic that the distance between the two curves is of the order of 0.1 a.u. for orbital arcs of nearly 900, between the approximate heliocentric longitudes of 960 and 1810. The orbits deviate by less than ...
Tópico(s): Planetary Science and Exploration
1959 - Institute of Physics | The Astronomical Journal
G. Apostolovska, Z. Donchev, A. Kostov, V. Ivanova, G. Borisov, B. Bilkina,
... analysis of photometric observations of Mars crosser asteroid 1011 Laodamia conducted at Bulgarian National Astronomical Observatory Rozhen over ... sense of rotation, and preliminary shape model of (1011) Laodamia have been determined using the lightcurve inversion method. ...
Tópico(s): Isotope Analysis in Ecology
2014 - Astronomical Observatory, Department of Astronomy, Belgrade | Serbian Astronomical Journal