What will Gaia tell us about the Galactic disk?
C.A.L. Bailer-Jones

TL;DR
Gaia will revolutionize our understanding of the Galactic disk by providing precise 3D positions, velocities, and stellar properties for a billion stars, enabling detailed studies of Galactic structure, evolution, and Earth's climate history.
Contribution
This paper discusses Gaia's expected capabilities and their implications for mapping the Galactic disk, including new insights into spiral arms, stellar populations, and the Sun's orbit.
Findings
Gaia will measure distances with 15% accuracy for stars 6 kpc away.
Gaia will provide 3D maps of stellar positions and velocities.
Potential to link Galactic dynamics with Earth's climate history.
Abstract
Gaia will provide parallaxes and proper motions with accuracy ranging from 10 to 1000 microarcsecond on up to one billion stars. Most of these will be disk stars: for an unreddened K giant at 6 kpc, it will measure the distance accurate to 15% and the transverse velocity to an accuracy of about 1 km/s. Gaia will observe tracers of Galactic structure across the whole HR diagram, including Cepheids, RR Lyrae, white dwarfs, F dwarfs and HB stars. Onboard low resolution spectrophotometry will permit -- in addition to a Teff estimate -- dwarf/giant discrimination, metallicity measurement and extinction determination. For the first time, then, Gaia will provide us with a 3D spatial/properties map and at least a 2D velocity map of these tracers (RVs will be obtained too for brighter stars.) This will be a goldmine of information from which to learn about the origin and evolution of the…
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