![K2-3 d: Habitable Zone, 45-Day Year](https://cdn.slatesource.com/a/c/2/ac20a703-10e8-4309-8007-1dd1f0d27a9f.webp)

# K2-3 d: Habitable Zone, 45-Day Year

- [Made in Slatesource](https://slatesource.com/@steph/k2-3-d-habitable-zone-45-day-year)
- By [Steph](https://slatesource.com/@steph)
- Created on Sep 19, 2026

## Super-earth around K2-3

It is 1.46 times Earth's radius, closest in size to Earth, and 2.2 times Earth's mass. A year there lasts 44.56 days, on an orbit 2 times closer to its star than Mercury is to the Sun. Its equilibrium temperature is 305 K, in the range where liquid water is possible. The host star K2-3 runs at 3844 K with 0.55 times the Sun's mass.

What this planet has and has not got

0%

Inside the habitable zone, computed from the star's luminosity. Yes.

A measured mass, not just a radius. Yes.

A measured temperature rather than one derived from the star. Yes.

Any detection of an atmosphere. Not recorded in the archive.

journey·3 Planets

# K2-3 from the inside out

Orbit

/

Planet

"mini-Neptune, 501 K.

"super-Earth, 372 K.

"super-Earth, 305 K.

Radius

1.46 Earth radii

Mass

2.2 Earth masses

Equilibrium temperature

305 K (measured)

One year

44.56 days

Orbit radius

0.2014 AU

Host star

K2-3 at 3844 K

Distance

144 light-years

Starlight blocked

0.060% at each transit

What you get from the shadow

The depth of the dip is the ratio of the two discs, so the radius follows.

K2-3 has 3 known planets. Planets in company tug on each other, and those tugs are measurable, which is how masses get pinned down without a wobble.

Found by K2 in 2015, the second life of the Kepler spacecraft after two of its reaction wheels failed and it could no longer hold a fixed stare.

Size from the shadow, mass from elsewhere. Most transiting planets never get the second half, and without it composition stays a guess.

# K2-3 d sits in the habitable zone on the arithmetic alone. That says where it \\

orbits, not what it is like. What would you want measured next before calling it promising?

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[NASA Exoplanet Archive: the full record for K2-3 d](https://exoplanetarchive.ipac.caltech.edu/overview/K2-3%20d?utm_source=slatesource)