The dynamics of the elliptic Hill problem : Periodic orbits and stability regions

Autor: Voyatzis, G., Gkolias, I., Varvoglis, H.

The motion of a satellite around a planet can be studied by the Hill model, which is a modification of the restricted three body problem pertaining to motion of a satellite around a planet. Although the dynamics of the circular Hill model have been e

Externí odkaz: http://arxiv.org/abs/1111.3843

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The Path to Establishing an Effective Framework for Space Debris Remediation on the Basis of Mitigation: Legal Proposals Resulting from the Technical Results of the Redshift Project

Autor: Popova, R., Alessandro Rossi, Kim, Y., Colombo, C., Alessi, E. M., Gkolias, I., Schaus, V., Tsiganis, K., Beck, J.

Publikováno v: Scopus-Elsevier

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::18379f70cf0ebb8f34d1245db5467d1a
http://hdl.handle.net/11311/1118898

Surfing the phase space of Earth’s oblateness and third body perturbations

Autor: Colombo, C., Scala, F., Gkolias, I.

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=od______3731::ec5e9d4773ed30cdb5e30d917502593e
http://hdl.handle.net/11311/1079470

Time characterization of the coupled solar radiation pressure-planetary oblateness dynamics

Autor: Alessi, E. M., Gkolias, I., Colombo, C.

Publikováno v: 70th International Astronautical Congress, Washington D.C., United States, 21-25/10/2019
info:cnr-pdr/source/autori:Elisa Maria Alessi; Ioannis Gkolias; Camilla Colombo/congresso_nome:70th International Astronautical Congress/congresso_luogo:Washington D.C., United States/congresso_data:21-25%2F10%2F2019/anno:2019/pagina_da:/pagina_a:/intervallo_pagine

Recent works demonstrated that the dynamics caused by the planetary oblateness coupled with the solar radiation pressure can be described by means of an analytical model based on singly-averaged equations of motion. The coupled perturbations affect t

Externí odkaz: https://explore.openaire.eu/search/publication?articleId=dedup_wf_001::25476144285a544dd0f2821a7f8c2298
http://www.cnr.it/prodotto/i/408261