SkyTracko

HD 40307 g

Orbits HD 40307 · 42.2 light-years from Earth

Neptune-likeRadial Velocity2013ESI 85 · Very Earth-like
Earth2.56 R⊕
Radius
2.56×
Earth
Mass
7.1×
Earth
Year
198d
Temp
255 K
-18°C
Gravity
1.1×
Earth
Distance
42.2
ly

What it would be like

HD 40307 g is a Neptune-like world — probably wrapped in thick layers of hydrogen, helium, and ices. There may be no solid surface at all, just clouds all the way down.

Surface gravity is about 1.1g — noticeably heavier what you're used to on Earth.

With an equilibrium temperature around -18°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 198 days makes the year 1.8× 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.

Radius2.56R⊕
1/25×Earth = 125×
Mass7.10M⊕
1/10000×Earth = 110000×
Surface gravity1.08g
1/100×Earth = 1100×
Equilibrium temp255 K(-18°C)
0 KEarth 255 K2500 K

Side-by-side with Earth

Radius
2.56 R⊕
1.00 R⊕
Mass
7.10 M⊕
1.00 M⊕
Surface gravity
1.08g
1.00g
Year length
197.80 days
365.25 days
Eq. temperature
255 K (-18°C)
255 K (−18°C)
Orbital eccentricity
0.2900
0.0167
Semi-major axis
0.600 AU
1.000 AU

Temperature in context

Liquid N₂Mars avgEarth eq.Earth sfc.Boiling H₂OVenus

Host star — HD 40307

Spectral type
K2.5 V

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

Temperature
4,956 K

Cooler than the Sun. Orange or red dwarf.

Radius
0.72 R☉
Mass
0.77 M☉
Luminosity
0.230 L☉
Distance
12.9 pc (42.2 ly)

Discovery & orbit

Method
Radial Velocity

Detected by the star's wobble — gravitational tug from the orbiting planet shifts spectral lines.

Year
2013
Facility
La Silla Observatory
Semi-major axis
0.6000 AU
Period
197.80 days
Eccentricity
0.2900

Noticeably elliptical. Seasons (if any) would vary in intensity.

Density
2.33 g/cm³

Low density — probably icy or gas-rich.

Discovered via · Radial velocity

The star's wobble — gravitational tug from the planet shifts its spectrum

A planet orbiting a star pulls it slightly back and forth. That motion compresses the star's light when moving toward us (blueshift) and stretches it away (redshift). Precision spectrographs detect the wobble at metres-per-second — enough to infer a planet's mass and orbit.

Overall share
~19% of discoveries
Best for
Massive, close-in planets around nearby bright stars

Orbital Animation

HD 40307HD 40307 gOrbitEarth orbitHabitable zone
Drag to rotate · scroll to zoom
Semi-major axis: 0.600 AUEccentricity: 0.2900Period: 197.8 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 42.2 light-years?

  • A light beam leaving Earth right now would arrive in 42.2 years.
  • At Voyager 1's speed (17 km/s), the trip would take approximately 744,080 years.
  • A radio signal sent today would arrive in 42.2 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.