Modified Newtonian Dynamics as an Alternative to the Planet Nine Hypothesis

Author:

Brown KatherineORCID,Mathur HarshORCID

Abstract

Abstract A new class of Kuiper Belt objects (KBOs) that lie beyond Neptune with semimajor axes greater than 250 astronomical units show orbital anomalies that have been interpreted as evidence for an undiscovered ninth planet. We show that a modified gravity theory known as modified Newtonian dynamics (MOND) provides an alternative explanation for the anomalies using the well-established secular approximation. We predict that the major axes of the orbits will be aligned with the direction toward the Galactic center and that the orbits cluster in phase space, in agreement with observations of KBOs from the new class. Thus, MOND, which can explain galactic rotation without invoking dark matter, might also be observable in the outer solar system.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

Cited by 2 articles. 订阅此论文施引文献 订阅此论文施引文献,注册后可以免费订阅5篇论文的施引文献,订阅后可以查看论文全部施引文献

1. Strong constraints on the gravitational law from Gaia DR3 wide binaries;Monthly Notices of the Royal Astronomical Society;2023-11-03

2. Generalizations of quasilinear MOND;Physical Review D;2023-10-03

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