Abstract
The Kuiper belt objects (KBOs) exhibit an orbital clustering of the outer planets lying at perihelion distances larger than Neptune and semimajor axes greater than 150 AU from the Sun. This implies a hitherto unknown dynamical mechanism to counter randomizing of the orbital elements caused by the giant solar system planets. Using the toroidal field induced frame-dragging we deduce here the observed range of the Kuiper belt region, the semi-major axis of Sedna like objects in the Kuiper belt, as well as the orbital clustering of the KBOs in the ecliptic, without assuming dynamical effects induced by trans-Neptunian-objects (TNOs). We also calculate the orbital precession rates for the inner planets and show their correspondence, within the range of observational accuracy, with recent planetary ephemerides.
Similar content being viewed by others
References
Batygin, K., Brown, M.E.: Astron. J. 151, 22 (2016a)
Batygin, K., Brown, M.E.: Astrophys. J. Lett. 833, L3 (2016b)
Batygin, K., Brown, M.E., Fraser, W.C.: Astrophys. J. 738, 13 (2011)
Batygin, K., et al.: Phys. Rep. 805, 1 (2019)
Brown, M.E., Batygin, K.: Astrophys. J. Lett. 824, L23 (2016)
Buie, M.W., Folkner, W.N.: Astron. J. 149, 22 (2015)
Ciolfi, R.: Astron. Nachr. 335, 285 (2014)
de la F. Marcos, C., de la F. Marcos, R.: Mon. Not. R. Astron. Soc. 443, L59 (2014)
Debono, I., Smoot, G.F.: Universe 2, 23 (2016)
Harding, A., Lai, D.: Rep. Prog. Phys. 69, 2631 (2006)
Iorio, L.: Sol. Phys. 281, 815 (2012)
Iorio, L.: Universe 1, 38 (2015a)
Iorio, L.: Int. J. Mod. Phys. D 24, 1530015 (2015b)
Iorio, L.: Astrophys. Space Sci. 326, 11 (2017)
Iorio, L.: Mon. Not. R. Astron. Soc. 476, 1811 (2018)
Iorio, L.: Astron. J. 157, 220 (2019)
Iorio, L., Giudice, G.: New Astron. 11, 600 (2006)
Iorio, L., et al.: Astrophys. Space Sci. 331, 351 (2011)
Lense, J., Thirring, H.: Phys. Z. 19, 156 (1918). English translation in Mashhoon, B., Heh, F.W., Theiss, D.S.: GRG 16, 711 (1986)
Levison, H.F., Morbidelli, A., Van Laerhoven, C., Gomes, R., Tsiganis, K.: Icarus 196, 258 (2008)
Lucchesi, D., et al.: Universe 5, 141 (2019)
Madigan, A.-M., McCourt, M.: (2015). arXiv:1509.08920
Makishima, K., et al.: Phys. Rev. Lett. 112, 171102 (2014)
Mereghetti, S.: Astron. Astrophys. Rev. 15, 225 (2008)
Mirza, B.M.: Int. J. Mod. Phys. D 16, 1705 (2007)
Mirza, B.M.: Astrophys. J. 847, 73 (2017)
Mirza, B.M.: Mon. Not. R. Astron. Soc. 489, 3232 (2019)
Mitchell, J.P., et al.: Mon. Not. R. Astron. Soc. 447, 1213 (2015)
Muhlberger, C.D., et al.: Phys. Rev. D 90, 104014 (2014)
Nottale, L.: preprint (2003). arXiv:gr-qc/0307042
Oron, A.: Phys. Rev. D 66, 023006 (2002)
Petit, P., et al.: Mon. Not. R. Astron. Soc. 388, 80 (2008)
Pétri, J.: Mon. Not. R. Astron. Soc. 433, 986 (2013)
Renzetti, G.: Open Phys. 11, 531 (2013)
Rindler, W.: Phys. Lett. A 233, 25 (1997)
Tartaglia, A., Ruggiero, M.L.: Il Nuovo Cimento B 117, 743 (2002)
Thompson, C., Duncan, R.C.: Mon. Not. R. Astron. Soc. 275, 255 (1995)
Tiengo, A., et al.: Nature 500, 312 (2013)
Trujillo, C.A., Sheppard, S.S.: Nature 507, 471 (2014)
Acknowledgement
I gratefully acknowledge the anonymous reviewer for suggestions regarding recent planetary ephemerides.
Author information
Authors and Affiliations
Additional information
Publisher’s Note
Springer Nature remains neutral with regard to jurisdictional claims in published maps and institutional affiliations.
Rights and permissions
About this article
Cite this article
Mirza, B.M. Can orbital clustering of KBOs in the ecliptic be due to the solar toroidal field generated spacetime dragging?. Astrophys Space Sci 365, 31 (2020). https://doi.org/10.1007/s10509-020-3722-x
Received:
Accepted:
Published:
DOI: https://doi.org/10.1007/s10509-020-3722-x