The «non-detections» place upper limits on the number of certain types of planets; that is, if there were any more planets of a certain mass or
orbital distance then these surveys would have found them.
Not exact matches
If so,
then conditions would be more favorable for the existence of stable orbit for an Earth - like planet (with liquid water) centered around 1.5 AU from around Iota Persei — around the
orbital distance of Mars in the Solar System.
If so,
then conditions would be more favorable for the existence of stable orbit for an Earth - like planet (with liquid water) centered around 1.15 AU from around 15 Sge — between the
orbital distances of Earth and Mars in the Solar System.
If so,
then conditions would be more favorable for the existence of stable orbit for an Earth - like planet (with liquid water) centered around 1.12 AU from around 37 Gem — between the
orbital distances of Earth and Mars in the Solar System.