The next step is to figure out the size of your planet, and the strength of its gravity. This information is derived from your planet's mass, radius &
density. With only 2 of these variables you can figure out gravity, and anything else relating to your planet's size. Given the same mass, the denser a planet is, the higher the gravity. Jupiter with over 300 times the mass of earth has a gravity of less than 3 times that of earth's (on the theoretical, unobserved surface of Jupiter) because it is very diffuse, made out of gas rather than iron and stone.
Mass can be pretty much whatever you want, within certain bounds. Dole estimates
(see Habitable Planets for Man, free PDF.) that a planet needs at least 0.4 Earth Masses to retain a human-breathable atmosphere. Depending on who you ask, 5, 10, or even 14 earth masses is the upper limit for a
terrestrial planet. Beyond that it will retain so much atmosphere that it crosses over into gas giant territory.
Radius can also be whatever you want, as long it doesn't force the other variables into something silly. Just be aware that radius has a strong effect on the surface area of your planet. If you double the radius, the surface area increases four times.
Density is a little trickier. But here are the basics. Density is primarily determined by what a planet (or moon) is made out of. Gas, such as helium and hydrogen, tends to be least dense and then in increasing density are ice (water), rock, and iron. These are the main ingredients of the known planets. It is easy to find the
densities for these materials at normal, surface of the earth conditions. But as the mass of a planet increases, so does the pressure inside, and thus the density of various materials.