458 real rocky terrestrials

Tau Ceti h orbits Tau Ceti, the closest single Sun-like star to us, about 12 light-years away, once every 49 days. Its minimum mass is about 1.8 Earth masses.

Gl 725 A b is a probable super-Earth, a planet heavier than Earth but lighter than Neptune, orbiting a red dwarf about 11.5 light-years away.

K2-72 d is about the size of Earth and is the second of four planets around K2-72, a red dwarf about 220 light-years away.

YZ Ceti b may be the first planet beyond the solar system with a magnetic field detected through radio waves.

Barnard e is among the lightest planets ever found by the radial velocity method, which detects a planet from the small back-and-forth motion its gravity gives its star.

L 98-59 c is a rocky planet about a third larger than Earth whose atmosphere has been searched for with both Hubble and Webb.

TOI-700 b is the innermost of four planets around TOI-700, a quiet red dwarf about 100 light-years away. It is about Earth's size and orbits every 9.98 days.

Wolf 1061 b is the innermost of three planets around Wolf 1061, a red dwarf about 14 light-years away. It orbits every 4.89 days. In 2016 a team led by D. J.

Barnard c is the heaviest of the four small planets around Barnard's Star, the closest single star to the Sun at about six light-years.

K2-72 b is the innermost of four small planets around K2-72, a red dwarf about 220 light-years away. It crosses in front of its star every 5.58 days.

Barnard d is the innermost known planet of Barnard's Star, the closest single star to the Sun at about six light-years.

Barnard's Star is the closest single star to the Sun, about six light-years away, and for most of a century it was the most famous place where planets were claimed and…