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Entering orbit…
Habitability
20/ 100
Extremely Harsh
Barnard e rendered in TerraForge from its measured mass, orbit and star

Barnard e

Also written Barnarde

Rocky Terrestrial6 light years awayFound 2025
Mass
0.19 × Earth
Radius
0.64 × Earth
Gravity
0.48 g
Surface (est.)
350 K
Year
6.7 days
From Earth
6 ly
Mass
0.19 × Earth
Radius
0.64 × Earth
Gravity
0.48 g
Surface (est.)
350 K
Year
6.7 days
From Earth
6 ly

Barnard's star system

Type
M-type (Red Dwarf)
Spectral type
M3.5-4 V
Temperature
3,195 K
Radius
0.185 ☉
Mass
0.162 ☉
Planets
4
Luminosity
3.55e-3 ☉

Published by the NASA Exoplanet Archive. This world’s temperature and habitability score are computed from this star’s measured luminosity, not from a stand-in for its class.

Habitable zone

Star and planets drawn to scale: the star is 32 times as wide as Barnard e, so only its edge is in view. Orbits spaced as in the star system view.

Estimated: this planet doesn't transit its star, so its size is inferred, not measured

Barnard e is among the lightest planets ever found by the radial velocity method, which detects a planet from the small back-and-forth motion its gravity gives its star. Its minimum mass is about a fifth of Earth's. It is the outermost of four small planets now known around Barnard's Star, the closest single star to the Sun at about six light-years.

Surface. Rocky surface with impact craters, possible volcanic features

✓ Conditions could support life. This planet’s modelled conditions could support biological processes: stable temperatures, liquid water and the chemistry life as we know it needs. That makes life possible, not present.

Rocky Terrestrial
Life possibleNone Activity
Barnard e is dominated by silicate (25.0%) and iron (12.5%) content, forming a rocky terrestrial body.
Rocky terrestrial planets are primarily composed of silicate rocks and metals. They're the most common type of small planet in the universe.
Classification Criteria:
✓ Silicon: 25.0% + Iron: 12.5% + Magnesium: 3.8%✓ Mass: 0.2x Earth (terrestrial range)

Reading Barnard e’s atmosphere

Dominant elements: O, Si, Fe, N, C, HThis is what a telescope would measure while Barnard e crosses in front of its star: starlight passes through the atmosphere and spreads into a rainbow band. Each dark line marks a wavelength the atmosphere absorbed.Every element absorbs its own signature wavelengths — hydrogen always darkens the same two spots, calcium another pair, and so on. Astronomers match the lines in a real spectrum against a library of these signatures to say what an atmosphere is made of, light-years away, without ever visiting. A deeper line generally means more of that element is present.Barnard e sits about 6 light-years away, found by the radial velocity method. Most catalogued distances trace back to parallax: as Earth orbits the Sun, a nearby star appears to shift very slightly against the distant background stars, and the size of that shift gives its distance directly.
Habitability ScoreExtremely Harsh
20
Contributing Factors
temperature33
Hot - near boiling, only heat-loving microbes would thrive
atmosphere70

Thin CO₂ and nitrogen atmosphere

Nitrogen atmosphere provides protection but not breathable
water22
Limited water content (low gravity lets water escape to space)
magnetic Field30
No magnetic field - vulnerable to solar radiation
geology30
Geologically dead - no nutrient recycling
Organic Chemistry80
Core organic elements (CHNO) present
rotation30
Very slow rotation - days and nights each last several Earth days, bringing extreme temperature swings

Physical Properties

Mass
0.19x Earth (1.15e+24 kg)
Radius
0.58x Earth (3,682 km)
This planet: 0.58× Earth radiusEarth: 1× (baseline)
Surface Gravity
0.58x Earth (5.7 m/s²)
Surface Temperature
350 K (77 °C / 170 °F)
Rotation Period
161.8 hours/day (slower than Earth)
This planet: 162 h/dayEarth: 24 h/day

Elemental Composition

How TerraForge built this world

Barnard e, from the NASA Exoplanet Archive (found 2025). Measured: 0.193 Earth masses, 0.0381 AU, a 3195 K M-type star. Composition inferred from an estimated bulk density of 0.75x Earth's, modeled rather than measured since this isn't a transiting planet — the radius is the archive's estimate, so it can't settle how much water there is; read as rock and iron, with a day locked to its 6.7-day year, as anything orbiting this close would be.

A dark ringed planet hanging over the horizon of a rocky moon, its rings lit by a distant sun

New: Stand on Your Moons 🌒

A planet's surface view isn't the only ground any more. Press the surface button on a planet with moons and it asks where to stand: the planet itself, or any moon still in orbit, each tagged with what it became — ocean, ice, carbon, volcanic. Every moon gets its own ground and sky from its own physics: airless rock under a black sky, ice cracked by geysers over a hidden sea, sulfur plains shaking with eruptions, or orange haze you can't see the sun through. And hanging over the horizon, there's the planet you built.

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