description GJ 3293 e Overview
GJ 3293 e is an exoplanet orbiting the red dwarf star GJ 3293, which lies roughly 65 light-years from the Sun. It was identified through measurements of the star's motion using the radial-velocity method and is the outermost of the system's known planets, not the innermost. Its reported classification and orbital properties place it among the cooler, lower-mass planets found around nearby red dwarfs.
help GJ 3293 e FAQ
What is GJ 3293 e?
GJ 3293 e is an exoplanet orbiting the red dwarf star GJ 3293. The system lies roughly 65 light-years from the Sun.
How was GJ 3293 e detected?
Astronomers identified GJ 3293 e by measuring the star's motion with the radial-velocity method. The planet's gravity produces small, repeated shifts in the star's observed spectrum.
Is GJ 3293 e the innermost planet in its system?
No. GJ 3293 e is described as the outermost of the system's known planets, not the innermost one.
What kind of star does GJ 3293 e orbit?
GJ 3293 e orbits a red dwarf, a small and relatively cool type of star. Its host lies about 65 light-years away, making the system a nearby exoplanetary target.
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