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Trash exoplanet 12 EP

Kepler-1984 b

RA 291.2850° · Dec 40.7300° · exoplanet

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Score breakdown

· 3 badges
12 pts · Trash
Trash 15 pts → Common
  • Confirmed exoplanet +5
  • Gas giant +4
  • Found by Kepler +3
Total score 12

3 more points to reach Common.

Badges

  • Confirmed exoplanet · +5
  • Gas giant · +4
  • Found by Kepler · +3

Trivia

Standing on it

  • A year here. A full year lasts just 2 Earth days.

By the numbers

  • Size. About 6.8× the width of Earth.
  • Volume. About 316 Earths could fit inside it.
  • Mass. About 37.3× the mass of Earth.
  • Your weight. You'd weigh about 0.8× your Earth weight standing here.
  • Density. Less dense than water — drop it in a big enough ocean and it would float.
  • Temperature. A scorching 402°C on average.

How we found it

  • Discovery. Found by Kepler using the transit method.

Properties

density gcc
0.649
discovery facility
Kepler
discovery method
Transit
eccentricity
0
eq temp k
675
insolation
48.82
mass earth
37.3
name
Kepler-1984 b
orbital period days
1.9928
radius earth
6.81
sys num planets
1

About Kepler-1984 b

Kepler-1984 b is a trash exoplanet. It has an equilibrium temperature near 675 K, spans roughly 6.81 Earth radii, weighs about 37.3 Earth masses and completes an orbit every 1.99 days.

About 6.8× the width of Earth.

How to see it

Like any astronomical target, Kepler-1984 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 Kepler-1984 b is a trash exoplanet

Kepler-1984 b scores 12 points on Spacedle's rarity scale, which places it in the trash tier. Another 3 points would lift it into a rarer tier.

That score comes from 3 science badges — Confirmed exoplanet, Gas giant and Found by Kepler — 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.