Transiting Exoplanets, Part 2 Codexery

K2-332 b

A potentially habitable Mini-Neptune in the habitable zone of a red dwarf.

K2-332 b (also known as EPIC 211579112.01) is a transiting exoplanet discovered in 2016 by the K2 'Second Light' mission. It is notable as a potentially habitable Super-Earth or Mini-Neptune located 402 light-years away, orbiting a dim M4V red dwarf star. The planet lies within the empirical habitable zone, receiving 1.17 times the insolation Earth receives from the Sun.

Quick Facts

Period
17.7 days
Mean Radius
2.2 R / 🜨
Density
2.83 g/cm3
Discovered
2016
Extrasolarplanet
yes
Eccentricity
<0.05
Mass
5.47 M / 🜨
Single Temperature
266 K

Facts from the source article.

Lore & Background

K2-332 b was detected via the transit method, with an average transit duration of 2 hours and 2 minutes and a transit depth of 0.6508%. Its host star, K2-332, is a dim red dwarf with about 20% the mass and size of the Sun. The planet's radius of 2.2 Earths and estimated mass of 5.47 Earths yield a density consistent with a watery or gaseous Mini-Neptune rather than a rocky Super-Earth. Its equilibrium temperature of 266 K is somewhat higher than Earth's, and it orbits within the inner part of the habitable zone, about one-third of the way between the runaway greenhouse limit for Super-Earths and the absolute inner edge. The planet is likely tidally locked due to its close orbit and low eccentricity, with one side permanently facing the star.

Reader's Guide

K2-332 b's significance lies in its potential habitability despite its low density. While a solid surface is typically considered necessary for life to develop spontaneously, studies from 2021 indicate that sub-Neptunes can harbor abundant water and life-friendly molecules such as nitrogen, oxygen, and CO₂ in their atmospheres, with stable habitable temperatures and pressures. If the system contains a leftover dust disk or asteroid/comet belt, panspermia from a terrestrial planet or Earthlike moon could introduce microbial life, which might have enough time to reproduce before succumbing to harsh conditions. Tidal locking would create a hot dayside and cold nightside, but oceanic currents and wind could distribute heat, potentially warming the nightside past the freezing point of the atmosphere and cooling the dayside below 100°C. Under such conditions, the habitable region could extend to 55° in both hemispheres on the dayside and around the nightside near the equator, with a maximum temperature of about 42°F. Higher carbon dioxide levels could expand this zone across most of the planet, excluding the nadir and high polar regions. These findings, supported by 2019 studies of the TOI-270 system, suggest that Mini-Neptunes like K2-332 b may possess life-friendly atmospheres rich in organic matter.

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