LHS 1140 b is a fascinating exoplanet orbiting a cool, red dwarf star named LHS 1140. Discovered back in 2017 by the diligent MEarth Project using a trusty Apogee CCD Sensor, this world made its debut thanks to a neat trick called the transit method—basically, it cleverly dims its star's light as it passes in front. Imagine a rocky planet that's just the right size, nestled close enough to its star to be intriguingly warm but far enough to keep things stable. Though it’s tucked away in the cosmic neighborhood millions of light-years from Earth, LHS 1140 b invites us to dream about what it might be like to stand under skies lit by a red sun, pondering the mysteries of its alien horizons.
