"Now, Gilbert and her colleagues say that TOI 700 d has a third sibling, and an intriguing one. This planet, dubbed TOI 700 e, isn't quite in the region astronomers have typically dubbed the habitable zone, but that definition is in flux. In particular, since astronomers have realized that Venus and Mars likely both once held water on their surfaces, some have proposed an "optimistic" habitable zone, which TOI 700 e resides in. Gilbert and her colleagues estimate that TOI 700 e is about 95% the size of Earth, so it's likely rocky and orbits about once every 28 Earth days — putting it in between TOI 700 c and d. The newly discovered world is also likely tidally locked, always showing the same side to its star. "That's most of what we know at this time from TESS data alone, but we do have some other campaigns currently underway to characterize this more," Gilbert said. "No results yet, but exciting things are coming."
Currently, the exoplanet sites show 3 confirmed for TOI 700.
The Extrasolar Planet Encyclopaedia — TOI-700 d (exoplanet.eu)
TOI-700 | NASA Exoplanet Archive (caltech.edu)
The .eu site indicates 700 d is 2.26 earth mass and 1.19 earth radii size. The mean density could be a bit more than 7 g cm^-3. Surface gravity compared to earth about 1.6 g so 100 lbs on earth would weigh 160 lbs on 700 d. Escape velocity 15.4 km/s, higher than earth escape velocity so our present rocket programs since 1957 would not work on 700 d. None of the TOI-700 exoplanets are confirmed with an atmosphere at present.
Exoplanet atmospheres (iac.es)
*that matches Earth's*, small differences above I note should be clearly pointed out when reporting. 700 e will need more follow up work to confirm and provide properties it seems.