TOI-700 c is the largest planet around TOI-700, a quiet red dwarf about 100 light-years away, and the odd one out in a system of Earth-sized worlds. It is about 2.6 times Earth's width, a sub-Neptune, between Earth and Neptune in size, and orbits every 16.1 days.
It was discovered together with TOI-700 b and d in 2020 by a team led by Emily Gilbert, using NASA's TESS satellite, which caught the dips in starlight as each planet crossed the star. The team ruled out common false alarms with ground-based observations and validated all three. They noted that, while studying the atmosphere of the habitable-zone planet TOI-700 d with the James Webb Space Telescope will be challenging, the larger TOI-700 c will be an excellent target, because a bigger planet blocks more light and leaves a stronger signal of any atmosphere. In 2023 a fourth planet, TOI-700 e, was found orbiting between c and d.
So the system has a sub-Neptune sitting between rocky-sized planets, a pattern that tests how planets of different sizes form and keep their atmospheres around the same star. According to the NASA Exoplanet Archive, TOI-700 c receives about 2.6 times the light Earth gets from the Sun. Its mass has not been measured; the archive's figure of about 7 Earth masses is an estimate from its size. At this size it is likely to have a thick envelope of gas, not a rocky surface.
