Submitted:
24 June 2024
Posted:
25 June 2024
Read the latest preprint version here
Abstract
Keywords:
1. Introduction

2. The “x-Shaped Structure” and Peanut Shape of the Bar: The Possible another Supermassive Black Hole
2.1. The Bar
2.2. The Arms and Hill Sphere
2.3. The Mass and Position of Black Hole B
3. Discussion
Newton established the theory of orbit in 1660s. But, Newton’s theory has not been completely understood till now. As soon as comparing Poincaré’s equation of Three-body problem with Newtonian orbital perturbation theory, we shall know what is the problem in current understanding about Newtonian theory of gravity. The Sun-Earth-Moon system is the oldest Three-Body problem. It is clear, the orbits about it was well resolved by Newton. But, there is a famous old problems: calculating with , the attractive force of the Sun on the Moon is almost 2.2 times that of the Earth, but the orbit of the Moon around the Earth cannot be broken off by the Sun. It is clear, as Poincaré’s equation for Three-body problem is applied on the solar system, the orbits in it should be broken off in a short time. We think, this is the crucial evidence to show that the Poincaré’s equation for Three-body problem is wrong. And, the triple star system and multiple star systems, including Six-star system, were observed. The orbit in these systems are stable and certain.
The Poincaré’s equation for Three-body problem is very strange. First, no orbit of the celestial body is chaotic. A broken orbit also is predictable. So, Poincaré’s equation cannot be related with any real orbit. Second, the orbits of the typical Three-body system, such as the Sun-Earth-Moon system and Sun-Pluto-Charon system, are stable. Poincaré’s equation is invalid to understand these orbits. Third, Poincaré’s equation is invalid to design an artificial orbit. It is very clear, the Poincaré’s equation is nonsense in understanding any real orbit. Additionally, the relationship between the Poincaré’s equation and other theory is very weak. If there was not Poincaré’s equation, the celestial dynamics could not be affected. But, very unfortunately, Poincaré’s equation is the mainstream understanding about Newtonian theory of gravity. It results in that, the current theory of orbit about the galaxy is questioned.
4. Conclusion
References
- Oort J. H., Kerr F. J. & Westerhout G. 1958, The galactic system as a spiral nebula (Council Note), MNRAS, 118, 379.
- Georgelin Y. M. & Georgelin Y. P. 1976, The spiral structure of our Galaxy determined from H II regions, A&A, 49, 57.
- Oort, J. H., & Rougoor, G. W. 1959, The interstellar gas in the central part of the galaxy, AJ, 64, 130.
- Rougoor G. W. & Oort J. H. 1960, Distribution and Motion of Interstellar Hydrogen in the Galactic System with Particular Reference to the Region Within 3 Kiloparsecs of the Center, Proceedings of the National Academy of Science, 46, 1.
- de Vaucouleurs G. 1964, in IAU Symposium, Vol. 20, The Galaxy and the Magellanic Clouds, ed. F. J. Kerr, 195.
- Genzel R., Eisenhauer F. and Gillessen S., 2010, The Galactic Center Massive Black Hole and Nuclear Star Cluster, Reviews of Modern Physics, 82.4, 3121-3195.
- Issaoun S., Johnson M. D., Blackburn L., Brinkerink C. D., et al., 2019, The Size, Shape, and Scattering of Sagittarius A* at 86 GHz: First VLBI with ALMA, Astrophysical Journal, 871, 1. F.
- Shen J. and Zheng X., 2020, The bar and spiral arms in the Milky Way: structure and kinematics, RAA, 20, 159.
- Busetti F., Beust H. and Harley C., 2018, Stability of planets in triple star systems, A&A619, A91.
- Zhou Y., et al., The Circular Velocity Curve of the Milky Way from 5–25 kpc Using Luminous Red Giant Branch Stars, ApJ, 946, 73 (2023). [CrossRef]
- Jiao Y., Hammer F., Wang H., Wang J., et al., 2023, Detection of the Keplerian decline in the Milky Way rotation curve, A&A678, A208.
- Eilers A., Hogg D. W., Rix H. and Ness M. K., 2019, The Circular Velocity Curve of the Milky Way from 5 to 25 kpc, ApJ, 871 120. [CrossRef]
- Yu S. and Ho L. C. 2020, The Statistical Properties of Spiral Arms in Nearby Disk Galaxies, ApJ, 900, 150. [CrossRef]
- Mondal D., Chattopadhyay T., 2021, Role of galactic bars in the formation of spiral arms: a study through orbital and escape dynamics—I. Celest Mech Dyn Astr 133, 43.
- Lindblad P. A. B. & Kristen H. 1996, Hydrodynamical simulations of the barred spiral galaxy NGC 1300. Dynamical interpretation of observations, Astronomy and Astrophysics, 313, 733-749.
- Yoon Y. & Lee M. I, et al. 2019, Observational evidence for bar formation in disk galaxies via cluster–cluster interaction. Nat Astron 3, 844–850.
- Roshan M., Ghafourian N., Kashfi T., Banik I., Haslbauer M., et al. 2021, Fast galaxy bars continue to challenge standard cosmology, Monthly Notices of the Royal Astronomical Society, 508(1) 926–939. [CrossRef]
- Mondal D., Chattopadhyay T. 2021, Role of galactic bars in the formation of spiral arms: a study through orbital and escape dynamics—I. Celest Mech Dyn Astr 133, 43.
- Davis B. L., et al., 2012, Measurement of Galactic Logarithmic Spiral Arm Pitch Angle Using Two-Dimensional Fast Fourier Transform Decomposition, ApJS, 199, 33.
- Dolores Mata-Chávez M., et al., 2019, On the Dynamical Relevance of Galaxy Spiral Arm Evolution. I. Arm Density Structure, ApJ, 876, 6.
- Zhu Y., The Mass of the Center of the Milky Way Revalued from the Fastest Orbits around the Center and the Circular Velocity Curve of the Milky Way[v3] | Preprints.org.
- Zhu Y., Interaction of Gravitational Field and Orbit in Sun-planet-moon system[v1] | Preprints. [CrossRef]
- Yoon Y., Park C., Chung H. and Zhang K. 2021, Rotation Curves of Galaxies and Their Dependence on Morphology and Stellar Mass, ApJ, 922, 249.
- McGaugh S. S., Lelli F. and Schombert J.M. 2016, Radial Acceleration Relation in Rotationally Supported Galaxies, Physical Review Letters, 117, 201101.
- Peißker F., Eckart A. and Parsa M. 2020, S62 on a 9.9 yr Orbit around SgrA*, ApJ, 889, 61.
- Peißker F., Eckart A., Zajaček M. and Britzen S., 2022, Observation of S4716- A star with a 4 year orbit around Sgr A*, ApJ, 933, 49.
- Peißker F., Eckart A., Zajaček M., Britzen S., Ali B. and Parsa M. 2020, S62 and S4711: Indications of a Population of Faint Fast-moving Stars inside the S2 Orbit—S4711 on a 7.6yr Orbit around Sgr A*, ApJ, 899, 50.
- Peißker F., Eckart A. and Ali B. 2021, Observation of the Apoapsis of S62 in 2019 with NIRC2 and SINFONI, APJ, 918, 25.
- GRAVITY Collaboration, et al., 2022, Deep images of the Galactic center with GRAVITY, A&A 657, A82.
- GRAVITY Collaboration, et al., 2022, Mass distribution in the Galactic Center based on interferometric astrometry of multiple stellar orbits, A&A 657, L12.
- Mróz P., Udalski A., Skowron D. M., Skowron J., et al., 2019, Rotation Curve of the Milky Way from Classical Cepheids, ApJL 870, L10.
- Wang H., ChrobákováŽ., López-Corredoira M. and Labini F. S., 2023, Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to ≈30 kpc, ApJ, 942, 12.
- Ou X., Eilers A., Necib L. and Frebel A. 2024, The dark matter profile of the Milky Way inferred from its circular velocity curve, MNRAS 528, 693–710.
- Fragkoudi F., Grand R. J. J., Pakmor R., Springel V., et al., 2021, Revisiting the tension between fast bars and the CDM paradigm, A&A650, L16.
- Corsini E. M., Aguerri J. A. L., Debattista V. P., Pizzella A., Barazza F. D. and Jerjen H. 2007, The Bar Pattern Speed of Dwarf Galaxy NGC 4431, ApJ, 659, L121.
- Aguerri J. A. L., Méndez-Abreu J., Falcón-Barroso J.,. Amorin A, et al., 2015, Bar pattern speeds in CALIFA galaxies I. Fast bars across the Hubble sequence, A&A,576, A102.
- James Q. F. and Gallo C. F. 2011, Modeling the Newtonian dynamics for rotation curve analysis of thin-disk galaxies, Res. Astron. Astrophys., 11, 1429.
- Hofmeister A. M. & Criss R. E., 2020, Debated Models for Galactic Rotation Curves: A Review and Mathematical Assessment, Galaxies, 8, 47.


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