zoom_in Click to enlarge

Kepler-1649c

▲ ▼

description Kepler-1649c Overview

Kepler-1649c is an exoplanet roughly Earth-sized orbiting a red dwarf star named Kepler-1649. Its location within its star’s habitable zone—the region where liquid water could exist on the surface—makes it notable. Scientists study this super-Earth to assess the potential for habitability around M-dwarf stars and understand planetary formation processes. The planet is of interest to researchers investigating Earth analogs beyond our solar system.

help Kepler-1649c FAQ

How was Kepler-1649c originally discovered?

Kepler-1649c was initially missed by an automated algorithm but was later identified by a team of scientists reviewing data from NASA's Kepler Space Telescope. The exoplanet was found hiding in the archival data years after the original observations were made.

How does the size of Kepler-1649c compare to Earth?

Kepler-1649c is remarkably close to Earth in size, measuring at about 1.06 times the radius of our planet. This makes it one of the most Earth-sized exoplanets discovered within the habitable zone of another star.

What kind of star does Kepler-1649c orbit?

This exoplanet orbits a red dwarf star, which is significantly smaller and cooler than our Sun. Because of this, the planet's habitable zone is located much closer to the star, meaning Kepler-1649c completes a full orbit roughly every 19 days.

Could humans survive on Kepler-1649c?

While it sits in the habitable zone where liquid water could exist, it is unknown if humans could survive there due to its red dwarf sun. Red dwarfs are known for emitting intense stellar flares, which could strip away the planet's atmosphere or bombard it with dangerous radiation.

swap_horiz

Looking for Kepler-1649c alternatives? Compare top competitors ranked & scored

arrow_forward