  We report the discovery of a new ultra-faint Milky Way satellite candidate,
Horologium II, detected in the Dark Energy Survey Y1A1 public data. Horologium
II features a half light radius of $r_{h}=47\pm10$ pc and a total luminosity of
$M_{V}=-2.6^{+0.2}_{-0.3}$ that place it in the realm of ultra-faint dwarf
galaxies on the size-luminosity plane. The stellar population of the new
satellite is consistent with an old ($\sim13.5$ Gyr) and metal-poor
([Fe/H]$\sim-2.1$) isochrone at a distance modulus of $(m-M)=19.46\pm0.20$, or
a heliocentric distance of $78\pm8$ kpc, in the color-magnitude diagram.
Horologium II has a distance similar to the Sculptor dwarf spheroidal galaxy
($\sim82$ kpc) and the recently reported ultra-faint satellites Eridanus III
($87\pm8$ kpc) and Horologium I ($79\pm8$ kpc). All four satellites are well
aligned on the sky, which suggests a possible common origin. As Sculptor is
moving on a retrograde orbit within the Vast Polar Structure when compared to
the other classical MW satellite galaxies including the Magellanic Clouds, this
hypothesis can be tested once proper motion measurements become available.
