Scientists are already considering the possibility of life on, or inside, Venus (atmosphere or past life on surface), Mars (subsurface), and Ceres, and in subglacial oceans on the Jovian satellites Europa, Ganymede and Callisto, and the Saturnian satellites Enceladus and Titan (see
https://en.wikipedia.org/Extraterrestrial_life and links). The possibility of life-bearing subglacial oceans on the satellites Rhea, Titania, Oberon and Triton and the dwarf planets Pluto, Eris, Sedna and Orcus, has also been mentioned, but at present we know very little about these bodies. Of course, the life-forms on these bodies, if they exist at all, would be extremophile micro-organisms; we are not talking about 'flying saucers' or 'men from Mars' here, and it would certainly be impossible for humans to live on these bodies. Also it would be very difficult to design probes that could travel to these bodies and search for evidence of life without contaminating the planet's environment with terrestrial organisms, so that it will be a long time before scientists can obtain evidence either way. However, although the probability of life on these planets and satellites is very low (perhaps 0.0001?), it is not zero.
According to E.A. Petigura (2013), 'Prevalence of Earth-size planets orbiting Sun-like stars',
https://pnas/org/content/early/2013/10/31/1319909110 , analysis of the observations by the
Kepler telescope implies 'that 11±4% of Sun-like stars harbor an Earth-size planet receiving between one and four times the stellar intensity as Earth', and that '5.7[±2]% of Sun-like stars harbor an Earth-size planet with orbital periods of 200-400 d' (i.e. in the period range of Venus and Earth). This implies that, in the Milky Way alone, there may be around a billion Earth-size planets in the habitable zones of Sun-like stars -
https://en.wikipedia.org/List_of_potentially_habitable_exoplanets. Thus there are likely to be many planets, in the Milky Way and in other galaxies, where life could have originated and evolved.
It is a small step to be able to infer the existence of so many Earth-like planets in stellar habitable zones; it would be a giant leap to conclude that these planets are actually inhabited, even by primitive micro-organisms. The discovery of an exoplanetary atmosphere that was out of chemical equilibrium would be evidence for life on the planet, and the presence of seasonally variable quantities of methane in the atmosphere of Mars may constitute such evidence. However, at present the evidence both from the solar system and from exoplanets suggests only that planetary and satellite environments exist that might be inhabitable by simple life-forms, and that the probability of the existence of such life-forms is above zero.