Astromart
And Just Like That… All the Imaginary Dark Matter in the Universe Disappeared
Guy Pirro
August 14, 2023
Excerpt:
A new study of the orbital motions of long-period, widely separated, binary stars (referred to as wide binaries) reports conclusive evidence that standard Newtonian gravity breaks down at extremely low acceleration. The study carried out by Kyu-Hyun Chae, professor of physics and astronomy at Sejong University in Seoul, used up to 26,500 wide binaries within 650 light years as observed by the European Space Agency (ESA) Gaia Space Telescope.
For a key improvement over other studies, Chae’s study focused on calculating gravitational accelerations experienced by binary stars as a function of their separation or, equivalently the orbital period, by a Monte Carlo de-projection of observed sky-projected motions in three-dimensional space. Chae further explains the point: “From the start it seemed clear to me that gravity could be most directly and efficiently tested by calculating accelerations, because the gravitational field itself is an acceleration. My recent research experiences with galactic rotation curves led me to this idea. Galactic disks and wide binaries share some similarity in their orbits, though wide binaries follow highly elongated orbits while hydrogen gas particles in a galactic disk follow nearly circular orbits.”
LINK
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Modified gravity?
And Just Like That… All the Imaginary Dark Matter in the Universe Disappeared
Guy Pirro
August 14, 2023
Excerpt:
A new study of the orbital motions of long-period, widely separated, binary stars (referred to as wide binaries) reports conclusive evidence that standard Newtonian gravity breaks down at extremely low acceleration. The study carried out by Kyu-Hyun Chae, professor of physics and astronomy at Sejong University in Seoul, used up to 26,500 wide binaries within 650 light years as observed by the European Space Agency (ESA) Gaia Space Telescope.
For a key improvement over other studies, Chae’s study focused on calculating gravitational accelerations experienced by binary stars as a function of their separation or, equivalently the orbital period, by a Monte Carlo de-projection of observed sky-projected motions in three-dimensional space. Chae further explains the point: “From the start it seemed clear to me that gravity could be most directly and efficiently tested by calculating accelerations, because the gravitational field itself is an acceleration. My recent research experiences with galactic rotation curves led me to this idea. Galactic disks and wide binaries share some similarity in their orbits, though wide binaries follow highly elongated orbits while hydrogen gas particles in a galactic disk follow nearly circular orbits.”
LINK
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Modified gravity?