SkyTracko

Kepler-62 e

Orbits Kepler-62 · 981 light-years from Earth

Super-EarthTransit2013ESI 85 · Very Earth-like
Earth1.61 R⊕
Radius
1.61×
Earth
Mass
36.0×
Earth
Year
122d
Temp
270 K
-3°C
Gravity
13.9×
Earth
Distance
981
ly

What it would be like

Kepler-62 e is a super-Earth — larger than our planet but likely still rocky or ice-rich. Whether it has a thin atmosphere like Mars or a crushing one like Venus remains unknown.

At 13.9g, gravity is crushing by Earth standards. Walking would feel like carrying a 902 kg backpack permanently.

With an equilibrium temperature around -3°C, this planet sits in the temperature range where liquid water could potentially exist on the surface — a key ingredient for life as we know it.

An orbital period of 122 days makes the year 3.0× shorter than Earth's. You'd celebrate your birthday more often here.

Earth comparison

Logarithmic bars so Jupiter-class planets fit the same scale as Earth-size worlds.

Radius1.61R⊕
1/25×Earth = 125×
Mass36M⊕
1/10000×Earth = 110000×
Surface gravity14g
1/100×Earth = 1100×
Equilibrium temp270 K(-3°C)
0 KEarth 255 K2500 K

Side-by-side with Earth

Radius
1.61 R⊕
1.00 R⊕
Mass
36.00 M⊕
1.00 M⊕
Surface gravity
13.89g
1.00g
Year length
122.39 days
365.25 days
Eq. temperature
270 K (-3°C)
255 K (−18°C)
Orbital eccentricity
0.0000
0.0167
Semi-major axis
0.427 AU
1.000 AU

Temperature in context

Liquid N₂Mars avgEarth eq.Earth sfc.Boiling H₂OVenus

Host star — Kepler-62

Spectral type
K2 V

Orange dwarf, cooler and longer-lived than the Sun.

Temperature
4,925 K

Cooler than the Sun. Orange or red dwarf.

Radius
0.64 R☉
Mass
0.69 M☉
Luminosity
0.210 L☉
Distance
300.9 pc (981 ly)

Discovery & orbit

Method
Transit

Detected by measuring the tiny dip in starlight as the planet crosses in front of its star.

Year
2013
Facility
Kepler
Semi-major axis
0.4270 AU
Period
122.39 days
Eccentricity
0.0000

Nearly circular orbit.

Density
Discovered via · Transit

Tiny dip in starlight as the planet crosses in front of its star

A transit photometer watches a star nonstop and measures its brightness to ~0.01%. When a planet passes between us and the star, the star dims briefly — the deeper the dip, the bigger the planet. This is how Kepler and TESS found most known exoplanets.

Overall share
~75% of all confirmed worlds
Best for
Earth-to-Neptune-sized planets on short orbits

Orbital Animation

Kepler-62Kepler-62 eOrbitEarth orbitHabitable zone
Drag to rotate · scroll to zoom
Semi-major axis: 0.427 AUEccentricity: 0.0000Period: 122.4 days

Hertzsprung–Russell Diagram

Where this host star sits among exoplanet host stars. The main sequence band runs diagonally — giants and supergiants sit above, white dwarfs below.

OBAFGKMCurrent star

How far is 981 light-years?

  • A light beam leaving Earth right now would arrive in 981 years.
  • At Voyager 1's speed (17 km/s), the trip would take approximately 17.3 million years.
  • A radio signal sent today would arrive in 981.3 years — and the reply wouldn't come back for twice that.

Earth Similarity Index

85/100
0 — Nothing like Earth100 — Identical to Earth

ESI combines radius similarity and equilibrium temperature similarity. Earth = 100. Mars ≈ 73. Venus ≈ 44. This score reflects two physical parameters only — not atmosphere, water, or magnetic field.