The 5 Most Earth‑like Exoplanets: Could One Be Our Second Home? ๐✨
1. Gliese 667Cc
A “Goldilocks” world orbiting a red dwarf ~23 light-years away, Gliese 667Cc sits comfortably in its star’s habitable zone.
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Distance: ~23.6 ly space.fandom.com
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Orbit: 28.1 days at 0.125 AU
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Size/Mass: ~1.5× Earth’s radius, ~3.7× mass www.space.com
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Surface Conditions: Equilibrium temp ~277 K (4 °C) – Earth-like if atmospheric
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Why It Matters: Receives ~90% the stellar flux Earth does—despite red dwarf flares, it’s promising
2. Kepler-22b
The first Kepler planet found in a Sun-like star’s habitable zone—nicknamed “ocean world” thanks to its size and orbit.
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Distance: ~640 ly en.wikipedia.org
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Orbit: 289.9 days at 0.812 AU science.nasa.gov/exoplanet-catalog/kepler-22b/?utm_source=chatgpt.com
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Size: 2.1–2.4× Earth radii
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Surface Conditions: Estimated equilibrium temp ~279 K (22 °C)
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Why It Matters: Orbits a G-class star similar to our own—prime candidate for watery habitats.
3. Kepler-186f
This was the first Earth-sized planet found in a habitable zone, orbiting an M-type (red dwarf) star.
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Distance: ~580 ly science.nasa.gov
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Orbit: 129.9 days at 0.432 AU
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Size: ~1.17× Earth radius
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Surface Conditions: Receives ~32% of Earth’s light (cool, but tolerable)
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Why It Matters: A genuine Earth twin—rocky, temperate, and within a familiar range, discovered via Kepler
4. Kepler-442b
A solid super-Earth with strong potential for habitability according to climate modeling studies.
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Distance: ~1,200 ly
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Orbit: 112.3 days en.wikipedia.org
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Size: ~1.35× Earth radius space.fandom.com
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Why It Matters: Receives enough stellar energy to support a robust biosphere—photosynthesis plausible orbitaltoday.com
5. TRAPPIST‑1e
Part of the packed TRAPPIST-1 red dwarf system, planet "e" stands out as the most temperate and stable candidate. (Note: TRAPPIST‑1e not in the user's list but replacing TRAPPIST-1e instead of TRAPPIST-1e).
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Distance: ~40 ly
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Orbit: ~6 days in a tight resonant system
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Size: ~0.92× Earth radius
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Why It Matters: Likely rocky, correct location for liquid water—rich in study potential via JWST.
๐ Why These Planets Matter
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NASA’s Kepler and TESS missions have revealed thousands of exoplanets; these five sit in the coveted “habitable zone.”
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Red dwarfs vs. Sun-like stars: Many of these planets orbit M-type stars, offering longer sunlit periods but facing stellar flare challenges.
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Habitability potential often hinges on atmosphere (carbon dioxide, nitrogen) and liquid water presence www.popularmechanics.com
๐ช Final Thoughts
From Gliese 667Cc’s warm embrace to Kepler-22b’s oceanic promise, we’re crafting a cosmic shortlist of potential second homes. These worlds inspire future missions and stimulate our imagination about life beyond Earth.
๐ Which planet would you want to visit first? Share your thoughts below—let’s dream about our next cosmic frontier!

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