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K2-136 b: 24.0 Grams Per Cubic Centimetre

K2-136 b: 24.0 Grams Per Cubic Centimetre

Terrestrial around K2-136

It is 1.01 times Earth's radius, closest in size to Earth, and 4.3 times Earth's mass, at 24.00 g/cm3, denser than Earth. A year there lasts 7.98 days, on an orbit 5 times closer to its star than Mercury is to the Sun. Its equilibrium temperature is 610 K, hotter than any desert. The host star K2-136 runs at 4500 K with 0.74 times the Sun's mass.

24.0g/cm3: denser than iron at Earth surface pressure

journey·3 Planets

K2-136 from the inside out

Orbit

/

Planet

K2-136 b (this one)K2-136 cK2-136 d12345
terrestrial, 610 K.
ice giant, 470 K.
super-Earth, 420 K.

Radius

1.01 Earth radii

Mass

4.3 Earth masses

Equilibrium temperature

610 K (measured)

One year

7.98 days

Orbit radius

0.0707 AU

Host star

K2-136 at 4500 K

Distance

193 light-years

Starlight blocked

0.019% 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.

A transit gives the radius and a separate measurement gives the mass. Having both is what makes a density, and a density is the only clue to composition at this range.

Found by K2 in 2017, the second life of the Kepler spacecraft after two of its reaction wheels failed and it could no longer hold a fixed stare.

K2-136 has 3 known planets. Systems like this are the ones where architecture can be studied instead of guessed at.