Fast stars reveal the Sun’s galactic path ✛ ✎

Original: "Kinematics of High-Velocity Stars Utilizing LAMOST and Gaia DR3 Archives within 100 kpc"
· W. H. Elsanhoury
arXiv:2501.12478 · 2025-01-21 · arXiv non-exclusive · independent analysis · 1 min
The velocities of 1,200 runaway stars have helped pinpoint the Sun's movement through the Galaxy.

Our Galaxy is a grand highway where stars race along their paths. Just as a driver gauges their speed by watching neighboring cars, astronomers determined the trajectory of the Sun from the motion of nearly 1,200 ultrafast stars. For each one, they measured the velocity along the line of sight (spectroscopy) and the shift on the sky, assembling a complete 3D picture. An unexpected twist: some of these stars are accelerated so powerfully by the central black hole that they are flung off the galactic “road” forever.

But the key is that these “runaways” reveal the invisible skeleton of the Galaxy. Their trajectories betray the pull of dark matter — the mysterious mass that doesn’t shine but holds the stars together. This method of “weighing” the cosmos was first proposed by Fritz Zwicky and Vera Rubin, who noticed that visible matter alone cannot explain the speeds of stars and galaxies.

One of these stars is racing at 1,200 km/s — fast enough to travel from Earth to the Moon in five minutes.

Fast stars leaving the Galaxy evoke generation ships from science fiction, where the stars themselves are the eternal travelers.

V_r = -2A(R_{gc} - R_o) \sin l \cos b + K
The radial velocity of a star relative to the Sun depends on its position in the Galaxy and the Oort constant A, which describes differential rotation.
(\sigma_2/\sigma_1)^2 = -B/(A-B)
The ratio of velocity dispersions along two axes of the velocity ellipsoid is related to the Oort constants, allowing B to be computed given A and the dispersions.
Scientists
Fritz ZwickyMichael FaradayHendrik LorentzSubrahmanyan ChandrasekharJocelyn Bell BurnellAdam Riess
Concepts
galactic kinematics stellar motion proper motion kilometer per second galaxy rotation curve stellar radius velocity dispersion kilometer spin rate speed of light variable star massive star galactic winds solar radius gaia luminosity velocity cosmic rays spiral galaxy megaparsec