description GJ 3293 c Overview
GJ 3293 c is an exoplanet detected by measuring the gravitational effect it produces on its host star, the red dwarf GJ 3293. It is one member of a multi-planet system identified through long-term radial-velocity observations. The planet is generally described as a Neptune-mass world, but its minimum mass is the quantity directly constrained by the radial-velocity method because the orbital inclination is not known. It is studied as part of the population of planets orbiting low-mass stars.
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How good is GJ 3293 c?
GJ 3293 c scores 5.70/10 (Mediocre) on Lunoo, making it rated in the Exoplanet category.
What are the best alternatives to GJ 3293 c?
See our alternatives page for GJ 3293 c for a ranked list with scores. Top alternatives include: GJ 273 c, GJ 357 c, 61 Virginis c.
How does GJ 3293 c compare to GJ 273 c?
See our detailed comparison of GJ 3293 c vs GJ 273 c with scores, features, and an AI-powered verdict.
Is GJ 3293 c worth it in 2026?
With a score of 5.70/10, GJ 3293 c is a solid option in Exoplanet. See all Exoplanet ranked.
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