1. Topography of polygonal structures at the Phoenix landing site on mars through the relief retrieval from the HiRISE images with the improved photoclinometry method

   • N. V. Bondarenko
   • I. A. Dulova
   • Yu. V. Kornienko

   OriginalPaper 25 July 2014 Pages: 243 - 258

2. Secular resonances as a source of dynamic chaoticity in the long-term orbital evolution of uncontrolled satellites

   • T. V. Bordovitsyna
   • I. V. Tomilova
   • I. N. Chuvashov

   OriginalPaper 25 July 2014 Pages: 259 - 268

3. Formation of a reference coordinate network as a basis for studying the physical parameters of phobos

   • I. E. Nadezhdina
   • A. E. Zubarev

   OriginalPaper 25 July 2014 Pages: 269 - 278

4. CHOMIK: a multi-method approach for studying Phobos

   • H. Rickman
   • E. Słaby
   • R. Wawrzaszek

   OriginalPaper 25 July 2014 Pages: 279 - 286

5. Quick numerical evaluation of the probability that an asteroid will collide with a planet

   • V. A. Avdyushev
   • T. Yu. Galushina

   OriginalPaper 25 July 2014 Pages: 287 - 294

6. Mass determinations for 27 asteroids by the dynamic method

   • O. M. Kochetova
   • Yu. A. Chernetenko

   OriginalPaper 25 July 2014 Pages: 295 - 301

7. Results of the new reduction of positional observations of the asteroid Ceres

   • K. V. Kuimov
   • G. V. Romanova
   • V. V. Chazov

   OriginalPaper 25 July 2014 Pages: 302 - 304

8. Relation of the green coronal line intensity to sunspot areas and magnetic fields of different scales

   • O. G. Badalyan
   • N. G. Bludova

   OriginalPaper 25 July 2014 Pages: 305 - 315