@article{https://doi.org/10.48550/arxiv.astro-ph/0508670,<br/><span class="tab"></span>
  doi = {10.48550/ARXIV.ASTRO-PH/0508670},<br/><span class="tab"></span>
  url = {https://arxiv.org/abs/astro-ph/0508670},<br/><span class="tab"></span>
  author = {Süli,<br/><span class="tab"></span> Áron and Dvorak,<br/><span class="tab"></span> Rudolf and Freistetter,<br/><span class="tab"></span> Florian},<br/><span class="tab"></span>
  keywords = {Astrophysics (astro-ph),<br/><span class="tab"></span> FOS: Physical sciences,<br/><span class="tab"></span> FOS: Physical sciences},<br/><span class="tab"></span>
  title = {The stability of the terrestrial planets with a more massive "Earth"},<br/><span class="tab"></span>
  publisher = {arXiv},<br/><span class="tab"></span>
  year = {2005},<br/><span class="tab"></span>
  copyright = {Assumed arXiv.org perpetual,<br/><span class="tab"></span> non-exclusive license to distribute this article for submissions made before January 2004}
}