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Common exoplanet 21 EP

G 268-110 b

RA 16.2237° · Dec -18.1248° · exoplanet

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Score breakdown

· 2 badges
21 pts · Common
Common 24 pts → Uncommon
  • Earth-sized +16
  • Confirmed exoplanet +5
Total score 21

3 more points to reach Uncommon.

Badges

  • Confirmed exoplanet · +5
  • Earth-sized · +16

Trivia

Standing on it

  • A year here. A full year lasts just 1.4 Earth days.

By the numbers

  • Size. About 1.1× the width of Earth.
  • Mass. About 1.5× the mass of Earth.
  • Your weight. You'd weigh about 1.2× your Earth weight standing here.
  • Temperature. A scorching 261°C on average.

How we found it

  • Discovery. Found by Calar Alto Observatory using the radial velocity method.

Properties

density gcc
5.79
discovery facility
Calar Alto Observatory
discovery method
Radial Velocity
eccentricity
0
eq temp k
534
insolation
13.57
mass earth
1.52
name
G 268-110 b
orbital period days
1.4326
radius earth
1.13
sys num planets
1

About G 268-110 b

G 268-110 b is a common exoplanet. It has an equilibrium temperature near 534 K, spans roughly 1.13 Earth radii, weighs about 1.52 Earth masses and completes an orbit every 1.43 days.

About 1.1× the width of Earth.

How to see it

Like any astronomical target, G 268-110 b is best seen from a dark site away from city lights, and when it is above the horizon depends on your latitude and the time of year. The visibility panel above works out tonight's viewing window for your saved location.

Why G 268-110 b is a common exoplanet

G 268-110 b scores 21 points on Spacedle's rarity scale, which places it in the common tier. Another 3 points would lift it into a rarer tier.

That score comes from 2 science badges — Confirmed exoplanet and Earth-sized — each earned for a real, measurable property of the object. Rarity on Spacedle is never random: the more remarkable an object's astrophysics, the more badges it collects, the higher it scores, and the rarer it ranks.

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Sky imagery and survey data courtesy of Aladin Lite & CDS, Strasbourg. Object data from the NASA Exoplanet Archive, JPL Small-Body Database, and the ATNF Pulsar Catalogue.