  Properties of solar twins reported by Lehmann et al. (2023) at kiloparsec
distances from the local standard of rest (LSR) are compared to solar twins
within 100 pc of the Sun. These have velocity distributions closely similar to
those of the nearby twins in addition to closely matching $T_{\rm eff}$,
$\log{(g)}$ and $[Fe/H]$. The new twins are at slightly higher galactic
latitudes, and are somewhat closer to the Galactic center. Additionally, they
may be significantly older than nearby solar twins.
