  We report the discovery of two transiting extrasolar planets by the HATSouth
survey. HATS-9b orbits an old (10.8 $\pm$ 1.5 Gyr) V=13.3 G dwarf star, with a
period P = 1.9153 d. The host star has a mass of 1.03 M$_{\odot}$, radius of
1.503 R$_\odot$ and effective temperature 5366 $\pm$ 70 K. The planetary
companion has a mass of 0.837 M$_J$, and radius of 1.065 R$_J$ yielding a mean
density of 0.85 g cm$^{-3}$ . HATS-10b orbits a V=13.1 G dwarf star, with a
period P = 3.3128 d. The host star has a mass of 1.1 M$_\odot$, radius of 1.11
R$_\odot$ and effective temperature 5880 $\pm$ 120 K. The planetary companion
has a mass of 0.53 M$_J$, and radius of 0.97 R$_J$ yielding a mean density of
0.7 g cm$^{-3}$ . Both planets are compact in comparison with planets receiving
similar irradiation from their host stars, and lie in the nominal coordinates
of Field 7 of K2 but only HATS-9b falls on working silicon. Future
characterisation of HATS-9b with the exquisite photometric precision of the
Kepler telescope may provide measurements of its reflected light signature.
